Guide to the WMO/GAW

 World Ultraviolet Radiation Data Centre

 

 

Version 5.1

 

 

                             

 

 

 

 

Atmospheric Environment Service

Environment Canada

 

1998

 

 

 

 

 


 

Guide to the WMO/GAW

 World Ultraviolet Radiation Data Centre

 

Atmospheric Environment Service

Environment Canada*

 

 

Version 1 - December 10, 1996

Version 2 - January 2, 1997

Version 3 - May 10, 1997  (Version 3.2 - June 9, 1997)

Version 4 - November, 1997 (Version 4.2 - February 1998)

Version 5 - April-August 1998 (Version 5.1 - January 1999)

 

 

 

Foreword

 

This document describes the World Ultraviolet Radiation Data Centre (WUDC) and is intended as a guide for data originators and clients.  The World Wide Web (WWW) will be used to update information and serve as a bulletin board.  As the WUDC is further developed, this guide will be enhanced and updated accordingly.

 

The current version, Version 5.1, incorporates suggestions made by members of the WMO/GAW  Scientific Advisory Group on Ultraviolet Radiation (SAG_UV)  up to April 1998.

 

The use of terminology throughout this text will interchange between the World Ozone and Ultraviolet Radiation Data Centre (WOUDC) and the acronym WUDC.  Issues that refer to the general aspects of the Data Centre such as data reception or access, will use  the acronym WOUDC.  Issues specific to ultraviolet radiation such as form and content, will use the WUDC acronym.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

D.I. Wardle*, E.W. Hare*, E.J. Carty++ and V.E. Fioletov*


Table of Contents

 

Foreword..............................................................................................................................................................................................

1 Introduction...............................................................................................................................

1.1 Origin..............................................................................................................................................................................................

1.2 Purpose..........................................................................................................................................................................................

1.3 Development.................................................................................................................................................................................

1.4 Guide...............................................................................................................................................................................................

2 Current Status...........................................................................................................................

2.1 Submission of Data  (see section 5 for current procedure)....................................................................................................

2.2 Current Data  Availability............................................................................................................................................................

2.3 Current Data Output Products....................................................................................................................................................

3 Data Types....................................................................................................................................

3.1 Basic Data......................................................................................................................................................................................

3.2 Ancillary data................................................................................................................................................................................

3.3 Auxiliary Data................................................................................................................................................................................

3.4 Meta Data (File Identification)....................................................................................................................................................

4 Data Levels and Versions......................................................................................................

4.1 Level 0  Raw data..........................................................................................................................................................................

4.2 Level 1   Processed Data..............................................................................................................................................................

4.3 Level 2   Spectrally Gridded Data...............................................................................................................................................

5 Data Submission........................................................................................................................

5.1 Step 1: The Scientific Sponsorship Statement.......................................................................................................................

5.2 Data Identification......................................................................................................................................................................

5.2.1 Step 2: The Agency Profile.....................................................................................................

5.2.2 Step 3a: Special Agreements...................................................................................................

5.3 Step 3b: Submission File Format..............................................................................................................................................

5.3.1 Rationale of The WOUDC File Format....................................................................................

5.3.2 The Extended Comma Separated File Format for Data Submission............................................

5.3.3 The WUDC Metadata Content: Class and Category: FORM 1..................................................

5.3.4 Examples...............................................................................................................................

5.3.5 Representation of Time...........................................................................................................

5.4 Step 4: Assignment of Personal Data submission account.................................................................................................

6 Identification of Data Quality.........................................................................................

6.1 General principles of the WUDC Identification of Data Quality.........................................................................................

6.2 The Data Passport or SSS.........................................................................................................................................................

6.3 Examination by the WOUDC....................................................................................................................................................

6.3.1 Additional Data Quality Identification Procedures.....................................................................

6.4 Examination by Others...............................................................................................................................................................

6.5 Role of WMO and AES Advisory Committees......................................................................................................................

7 Access and Data Retrieval.................................................................................................

7.1 Addresses....................................................................................................................................................................................

7.2 General Access...........................................................................................................................................................................

7.3 Restricted Access and Protocol...............................................................................................................................................

7.4 Data Archive Structure..............................................................................................................................................................

8 Acknowledgments..................................................................................................................

9 References..................................................................................................................................

Appendix A    Scientific Sponsorship Statements...........................................................

Appendix B   The Agency Profile...........................................................................................

Appendix C   ISO 3166 Country Codes.....................................................................................

Appendix D   WOUDC Security protocol documents....................................................

Appendix E    WUDC Data Flags...............................................................................................

Appendix F    List of Acronyms...............................................................................................

Appendix G    List of Defined Instrument Types and Names.......................................

 


1        Introduction

 

1.1       Origin

 

The World Ozone Data Centre (WODC) in Toronto was established as a WMO data centre in 1961.  It is operated by Environment Canada as part of the WMO Global Atmospheric Watch (GAW) program.  In 1992, a WMO sponsored Experts meeting on UV data took place in Toronto and in early 1993 the World Ultraviolet Data Centre (WUDC) was formed and began collecting spectral ultraviolet data by the end of the year.  The WODC and WUDC components now constitute the one data centre which is called the World Ozone and Ultraviolet Radiation Data Centre (WOUDC).  Although matters relevant to the WOUDC will be discussed, the primary focus of this document is WUDC related topics.

 

1.2       Purpose

 

The purpose of the WOUDC was identified in the 1992 agreement between Environment Canada and the WMO as to facilitate research on ozone and ultraviolet radiation and the effects of the latter.  As with other WMO Data Centres the basic activities are the collection, archiving and distribution of geophysical data and information.  The early examination of measurements by researchers in addition to those responsible for the measurements is a valuable form of quality control that can lead to improvements in measurement and analysis techniques.  This is a particularly valid process for atmospheric UV radiation because the measurement technique and theory are not yet fully developed in many aspects.  The WUDC, therefore, encourages originators to make their data so available.  Research is also facilitated by providing uniform sets of ultraviolet radiation data which can be easily used by the scientific community.  This is done by maintaining an up-to-date, well-qualified archive which involves applying simple quality control procedures, organising the data logically and providing value added output products such as data gridded on wavelengths and bandwidths, or time series analysis. The WUDC also offers centralized secure archiving of raw data that may be of value in the long-term. 

 

1.3       Development

 

At present, there is little uniformity in ultraviolet radiation data.  UV instruments not only have different characteristics, but often make measurements which differ in both sampling and resolution, and in both time and wavelength.  Individual instrument types and data originators represent data in unique output formats.  These formats, in turn, become the easiest form in which to submit data.  Although desirable, it is not easy nor perhaps practical to establish a fixed spectral range and resolution for data submission.  Conversely, users like uniformity in data, and it is reasonable that a data centre provide clients with output products which are made more uniform, for example by being gridded to a standard set of wavelengths, and presented in the same format.  It may be stressed that the WUDC will not in any way process  submitted data without the specific consent of the originators. 

 

1.4       Guide

 

This Guide in general addresses questions about content, submission and conditions of access.  Data content and particularly submission procedure will change and the Guide will be revised when necessary.   The current content is described in Section 2.  Data types are defined in Section 3 and Data levels in Section 4.  The rules and rationale for data submission are discussed in Section 5  which will be of interest to data originators.  The data quality control procedures are then outlined in Section 6, which describes what procedures the WUDC uses to accept and flag data.  Finally in Section 7, data access is discussed with all the relevant Internet addresses for easy access to the data sets. This section will be of interest to data clients.


2        Current Status

 

The guide is currently on its fifth version issued in April, 1998.

 

2.1       Submission of Data  (see section 5 for current procedure)

 

·         Data have been accepted in the originator’s format if a detailed description of the format is provided.

·         The submitted data are used by the WUDC to create uniform output products.

·         The data can be submitted electronically (by e-mail, FTP) or on computer media (diskettes, CD‑ROMs).

·         The data have been processed by the submitting agencies, i.e. the data are not Level 0 (Refer to Section 4.0 Data Levels and Versions).

 

2.2       Current Data  Availability

 

·         At present, spectral UV data from three major sources have been submitted to the WUDC: the Brewer Database Management System (BDMS) of the Atmospheric Environment Service (AES) where raw data from the Canadian Brewer Network and some international Brewer sites are processed; the  Japan Meteorological Agency (JMA); and the National Science Foundation (NSF) Polar Programs UV Spectroradiometer Network.  UV irradiance values stored in the BDMS and JMA archives were measured by the Brewer spectrophotometer (single-monochromator) types MKII and MKIV. The NSF Polar Network uses double spectroradiometers developed by Biospherical Instruments Incorporated.

·         The archive also contains multi-band UV irradiance data for 1998 from the Colorado State University in conjunction with the of United States Department of Agriculture (USDA_CSU).

·         The total number of spectra available from WUDC is about 500,000. About 3/5 of the total number are from the BDMS, 1/5 from JMA and 1/5 from the NSF Polar Network. The total number of stations is 24. The time span is from 1989 1998.

·         All submitted data are available as WUDC output products (see below). JMA data in the originator’s format are available on the WUDC FTP server. NSF data in the ‘native’ format are available on CD‑ROM from the data originator (Biospherical Instruments Inc. [1]), or can be provided by WOUDC by special arrangement.

·         The data are organised as flat ASCII files in a directory structure based on location (station name) and time (year/day).

 

 

2.3       Current Data Output Products

 

·         The WUDC has converted the submitted processed spectral data to a uniform, gridded wavelengths set (from 290 to 325 nm with 0.5 nm increments).

·         The output files also contain calculated integrated (spectral and daily) UV characteristics and data quality flags (see section 6).

·         Separate summary files list daily statistics and monthly statistics of the spectral irradiance at a few wavelengths and of two  weighted integrals of the UV irradiance (CIE and ACGIH-NIOSH.)

·         Data are available through the Internet at the WUDC FTP site and on the first edition,  WOUDC CD‑ROM (Volume 1).

·         Data are now available in the prototype extended comma separated values format (refer to Section 5.0 Data Submission).


3        Data Types

 

The WUDC terminology for data types is as follows:

 

Basic data:        Spectrally resolved or weighted spectral integrals of UV radiation such as radiance, irradiance, irradiation as functions of time and wavelength or of time alone and possibly of direction (these data may be level 0, 1 or 2, refer to section 4).

Ancillary data:   Data describing atmospheric variables and variable site characteristics such as temperature, ozone, pressure, cloud conditions for example by a cloud index or by a sky image, albedo, pyranometer data.  Information on permanent characteristics of the measuring site. 

Auxiliary data:   Characteristics of the instrument that made the measurements, the way in which the instrument was operated, the algorithms that were used to compute the measured values from the instrument signals, etc.   Auxiliary data may be potentially of value to the user or absolutely necessary as when the basic data is raw (Level 0).

Meta data:        Information that uniquely describes sections (files) of basic data (‘data about the data’), such as instrument and agency identification, location and category of the measurements, etc.

 

 

3.1       Basic Data

 

The following types of ultraviolet radiation measurements are considered acceptable for submission to the WUDC archive.

·         Spectral global UV irradiance at the Earth surface expressed in Wm-2nm-1 by spectroradiometer-type instruments. The recommended spectral interval is 290‑400 nanometres (nm), with a minimum requirement 300‑315 nm.  Possible subsets are 290-360  nm and 290‑325 nm  The spectral resolution should be 1.0 nm full width at half maximum (FWHM) or better.

·         Spectral global UV irradiance at the Earth surface measured in Wm-2nm-1 at selected wavelengths in the UV part of the spectrum measured by Multi-band filter instruments.  The requirement is for measurements at two or more wavelengths.

·         Spectrally integrated global UV irradiance expressed in Wm-2 measured by a broadband filter instrument. The originator should provide information on the weighting function which should approximate one of the standard weighting functions (e.g. CIE).

·         If available, independent measurements of the direct and diffuse components of the global irradiance should also be submitted.

·         Actinometric (actinic) irradiance(flux), spectrally resolved or integrated, may also be submitted.

 

 

3.2       Ancillary data

 

·         Pyranometer global solar radiation data in the broadband spectral range from 280 to 3000 nm in Wm‑2.  The data file can include direct solar, downwelling and upwelling global solar irradiance for the same broadband spectral range from 280 to 3000 nm, albedo, and aerosol optical depth. Recommended temporal resolution is 1-10 minutes.  Pyranometer data is defined as a WOUDC UV Category.  Refer to Section 5 for details PAR (Photosynthetically Active Radiation) data are acceptable.

·         Meteorological data that includes: surface temperature (in °C), surface pressure (hPa), cloud amount (in tenths), snow on the ground (in cm), stratospheric temperatures at 100, 50, and 30 hPa (in °C). Recommended temporal resolution is 12-24 hours.

·         Atmospheric composition data such as total ozone, NO2 , SO2. Recommended temporal resolution 12-24 hours.

·         2D (e.g., sky images in UV part of the spectrum) and 3D (e.g., spectrally resolved sky images) data files also can be submitted to the WUDC and can be distributed by the WOUDC, although algorithms for their control and processing by the WUDC are not established yet.

·         Other types of UV-related data can be included in the WOUDC database. This may be negotiated between the data originator and the WOUDC.

 

 

3.3       Auxiliary Data

 

·         The originator of the data is encouraged to submit any auxiliary data that he or she may consider relevant.  The WUDC has defined required auxiliary data that will be discussed later in Section 5, Data Submission. 

·         Measurements of instrument characteristics are valuable regardless of whether the characteristics are described in text elsewhere.  Such measurements include scans of radiation from lasers or spectral lamps that characterise the spectral sampling function of the  measuring instrument and measurements of the directional sensitivity of any irradiance measuring instrument.    

·         The Agency Profile (which includes Station Information) and the Scientific Sponsorship Statement (see Section 5) are Auxiliary data.

·         For the special case when “raw” Brewer UV files are submitted, the instrument responsivity files are required.

 

 

3.4       Meta Data (File Identification)

 

·         Meta data (‘data about the data’) are those data used by the WOUDC for file identification.  Typically, the Agency Profile and the Station or Site information data are considered examples of ‘metadata’.  The requirements for meta data are given later in Section 5, Data Submission.

 


4        Data Levels and Versions

 

The WOUDC has attempted to maintain as much consistency as possible with usage in the satellite data community and with the Network for the Detection of Stratospheric Change (NDSC) in choosing the following definitions of Data Levels for UV radiation data [2].

 

Level 0    Raw data.  E.g. signals from radiation detectors in counts or converted voltage, signals from

                sensors or digital data that describe instrument configuration,  as functions of time.

Level 1    Radiometric data, i.e. irradiance vs. wavelength  (and time).  The spatial, temporal and spectral

                 characteristics of each datum are those of the original measurement.

Level 2    Spectrally gridded.

                2a  On a standard wavelength sampling interval such as (integer nm)/2 or (integer nm)/5. 

2b  With a standard passband e.g. trapeziod 1.0 nm full width at half intensity with 0.5 nm slope.  (Note: this implies a base width of 1.5 nm and a flat peak of width 0.5 nm.)

 Level 3   Spatially and/or temporally gridded and other high level products.  These are not yet being addressed by

               WUDC. 

 

In principle, Level 0 data are unchangeable.  In practice they might be changed to correct gross mistakes like an assignment of the wrong time or location to a file.  There are no versions of Level 0 data.

 

Versions and levels are entirely distinct.  The level refers to the product while the version specifies the procedure used to generate the product from the Level 0 data.  In the normal course of progress, research in measurement and modeling generates better algorithms and better instrument characterization.  The non-zero level data can then be upgraded and then given incremented Version numbers (c.f. TOMS Version 7) and/or version dates.  

 

Preliminary data are the result of processing that may be over-simple or lacking key information due to lack of time.  The WOUDC, in common with other data agencies, asks that Preliminary data be designated as Version 0. 

 

 

4.1       Level 0  Raw data

 

·         An instrument’s output in the numerical form which cannot in principle be altered or corrected, is known as “raw data”. Examples include photon counts, step counts, voltages and temperatures.  An example of a raw data file is the UV-file generated by the Brewer instrument. 

·         In some instruments the signals are internally processed to provide output voltages or digital signals that directly represent the measurement.  Also the internal processing may involve discarding some of the data.  In either event whether such data should be classed as Level 0 or Level 1 is debatable.

·         WOUDC encourages the submission of Level 0 data as an alternative or in addition to Level 1 data. For directions on submission of raw data to the WOUDC refer to Section 5, Data Submission.

 

 

4.2       Level 1   Processed Data

 

·         Level 1  data are the result of processing instrument signals to give numbers  describing physical quantities in standard units such as Wm-2nm-1. Examples include irradiance, total column ozone and airmass.  The processing may be simple or it may involve several stages including corrections for instrument stability and response, conversion of raw parameters to standard physical units or any other adjustment required to assure the data is of high quality.

·         The spatial, temporal and spectral characteristics of Level 1 data are the same as those of the Level zero data from which they are generated.  Thus gridded spectra and temporal or wavelength integrations of measured spectra are on higher levels.

·         The data originator is responsible for applying appropriate, documented corrections and quality control coding to raw data in order to obtain the required processed parameter such as irradiance.  If the output of an instrument is already the required processed parameter (i.e. irradiance calculated internally by the instrument), the quality control still remains the responsibility of the originator.

 

 

4.3       Level 2   Spectrally Gridded Data

 

·         It is expected that data will not usually be submitted in a “gridded’ form.  Gridding data may be done mostly by the WUDC, subject to approval by the originator, to produce UV data in a uniform format with the standard spectral range 290‑400 nm and with a sampling interval of 0.5 nm.  It is planned that data measured in restricted ranges (such as 290‑360 nm or 290‑325 nm) will be supplemented with simulated (and flagged) data in order to make a similar product for all spectra.  With the data represented in a uniform format,  there is an additional QA/QC step which provides value-added products such as quality flags and statistical summaries (e.g. daily means).

·         Processing algorithms will be described in the WUDC documentation.  If certain data transformations are required (e.g. re-calculation to a different wavelength grid), the WUDC will compute and distribute these data.

·         File formats for the output data products are easy-to-use and in-line with other WOUDC data formats.  Although some slight changes to the formats are possible, the WUDC expects that major changes will be infrequent.

·         The WOUDC would be glad to accept Level 2 or higher data provided that the data set is accompanied by the appropriate Level 1 version of the data.  In all cases format and quality control checks will be done by WUDC.


5        Data Submission

 

This section will present a step‑by‑step data submission procedure which is essential to the data originator, but may also be of use to data clients who are interested in understanding how ultraviolet data are forwarded to the WOUDC.

 

The logical development of data submission is as follows:

 

1.    Write a Scientific Sponsorship Statement (SSS) or “data passport” using the models given here (if appropriate).  Contact the WOUDC for assistance or clarification if needed.

2.    Submit to the WUDC a completed SSS along with an Agency (data originator) Profile.  A template for the Agency Profile is available on the Web.  If submission by means of the Web is not possible, data originators are requested to contact the WOUDC to arrange an alternative method of submission. Refer to section 5.2.1.

3.    Upon approval of the SSS and Agency Profile, a data submission agreement will be established whereby the details of the file format for submission may be negotiated between the data originator and the WUDC.  If special agreements, provisos, or security restrictions are required, they will be established at this point.

4.    The WUDC will assign an ftp account (with a personal username/password) to be used exclusively for data submission.  Data may also be submitted on computer media such as CD-ROM or diskettes.

5.    It is recommended that data submissions be made monthly.

 

 

5.1       Step 1: The Scientific Sponsorship Statement

 

The Scientific Sponsorship Statement (SSS) is a condensed scientific description of the origin, processing and quality of the data, including estimates of measurement uncertainty.  The writer would normally be the scientist responsible for making the measurements but might be some other scientist who could fully describe the data.  It is an ASCII file that is intended to be read by WUDC staff and data users, not by computers.  Thus, there are no format rules.

 

The SSS should include the following:

·         Instrument calibration information such as  sources, frequency, stability, etc.

·         Detailed data processing information about algorithms, data corrections, interpolation, and smoothing etc.

·         Estimation of measurement uncertainties.

·         References to publications that describe instruments, observation program, error estimations, results.  (The WUDC will be grateful for receiving reprints or copies of these publications.)

·         Conditions under which the originator permits use of the data.

A comprehensive list of sources of uncertainties and techniques for their estimation is provided in the WMO Guidelines for Site Quality Control of UV Monitoring [3].  The writer of the SSS is strongly encouraged to consult this QC document before starting his or her task.  Another document that may be worth consulting is the WMO Guidelines on Instruments to Measure Solar Ultraviolet Radiation [4], which describes characteristics and categories of UV instruments.  The SSS may include references to other ASCII files with data that are relevant to the SSS, e.g., instrument laser scans, instrument’s filter characteristics, directional sensitivity scans, etc.  These files will be stored in the same directory as the SSS file.

 

The QC document includes forms for the description of the site and the estimation of measurement uncertainty.  Submitting these forms is not a requirement for data to be accepted by the WUDC, but the forms can be very useful adjuncts to the SSS, even if only partially completed.  As stated in the preface of the QC document, “In all cases it is better to have a little information than none at all.  The WUDC will post all relevant QC information with the corresponding data so it is easily available to users.”

 

Typically, the SSS file would be named Agency.SSS.  For example, for AES  the SSS is named AES.SSS.  The agency name will typically be an acronym such as AES, JMA or NSF.  Three examples of SSS’s, for the AES, JMA and the USDA_CSU are given in Appendix A.

 

 

5.2       Data Identification

 

 

5.2.1    Step 2: The Agency Profile

 

The Agency Profile provides the necessary auxiliary and meta data required by the WOUDC to establish details about the measurement program, instruments, contact person(s) and address(es).  This information establishes the necessary link between the data originator and the WOUDC.  The profile will provide the following information:

 

·         Agency name, mailing and electronic address, phone/fax numbers, contact person(s).

·         A list of all stations from which the Agency plans to submit data.

·         The instruments in use by each Agency.  Each instrument must be specified by type, model and serial numbers and the main characteristics such as pass-band and spectral range must be provided.

·         Details about the observation program and schedule such as type and frequency of observations, along with sources of ancillary information.

 

A sample form of the Agency profile is provided in Appendix B.

 

Each agency will be represented by it’s known acronym or be assigned an acronym by the WUDC.  The country of origin must be expressed as the 3-character ISO-3166 standard [5].  Appendix C lists these codes.  This information must be included with each data file submission.  Table 5.2.1 illustrates several examples of each.

 

 

Table 5.2.1 Identification of Data Sources by Agency.

 

Agency Name (full)

Acronym

Country

ISO Code

 

 

 

 

Atmospheric Environment Service

AES

Canada

CAN

Finnish Meteorological Institute

FMI

Finland

FIN

Fraunhofer Institute for Env. Atmos. Research

IFU

Germany

DEU

Japanese Meteorological Agency

JMA

Japan

JPN

National Science Foundation

NSF

United States

USA

US Dept. of Agriculture-Colorado State Univ.

USDA_CSU

United States

USA

Univ. of Manchester Institute of Science Tech.

UMIST

United Kingdom

GBR

University of Thessalonki

AUTH

Greece

GRC

 

 

 

 

 

 


5.2.2    Step 3a: Special Agreements

 

The WUDC expects to receive quality controlled, Level 1 processed data.  However, data originators are encouraged to submit Level 0, raw data.  Currently, the data submission options are as follows:

 

 

Level 0 (Raw) Data - Submission

 

1.    Level 0 data submitted in it’s “native” format. 

2.    File format requirement - none.

 

Distribution options for the release of Level 0 data are presented in Table 5.2.2.

 

 

Table 5.2.2  Distribution Options  for release of Level 0 data by the WOUDC.

 

Option

Description

 

 

     1

Archive only. No distribution.

     2

Distribute the data as submitted with data originator’s permission.

          a. Restricted distribution for up to 24 months

          b. Unrestricted, public distribution

 

 

These options are discussed in more detail in the security/distribution protocol document (Appendix D).

 

The WUDC will archive and document the existence of these data.

 

 

Level 1 (Processed) Data - Submission

 

A basic requirement of the WUDC is to be a “processed data” archive and distribution centre.  Therefore, the usual method for sending data to the WUDC will involve the submission of Level 1 (processed) data.  The remaining sections of this chapter will examine the required format(s) and the minimum expected content for Level 1 data.

 

 

Level 2 (Spectrally Gridded) Data - Submission

 

Should a data originator decide to submit Level 2 (spectrally gridded ) data then the data originator is encouraged to contact the WUDC to negotiate the terms of a submission and distribution agreement.

 

 


5.3       Step 3b: Submission File Format

 

This section will discuss in detail the required data submission file format by first giving the rationale for the simple file format directives, followed by a description of the general format rules and finally the required data content.

 

 

The WUDC is aware that large volumes of UV “legacy” data exist in formats which are unique to an instrument or perhaps to an Agency.  The file format used for the data submission to the WUDC may be negotiated between the originator and the WUDC.  It should be clearly noted, that a certain minimum data requirement must be met for  data to be accepted.  

 

 

 

5.3.1    Rationale of The WOUDC File Format

 

The WOUDC Data Inventory, relational database uses the “metadata” (or data about the data) at the beginning of each file as an index for locating files based on search criteria such as location, time, data type etc.  A direct benefit of this approach is that the same metadata rules apply for complimentary data sets from the WODC such as total ozone and vertical profile data which in turn makes data extraction a relatively simple procedure.

 

The format for data submission to the WOUDC addresses the following design requirements:

 

1.    Ease of use by the submitting agency.

2.    Efficient processing, archiving and quality control of data by the WOUDC

3.    Providing  manageable, easily read and consistent output products.


 

5.3.2    The Extended Comma Separated File Format for Data Submission

 

Comma Separate Value (CSV) files are an accepted file format standard that can be directly imported into database, spreadsheet and analysis applications.  As they are written in ASCII, they are portable to differing computer platforms.  The WOUDC has extended these standard CSV syntax rules to support comments and multiple data content (tables) within individual files and this format has been given the name extended CSV or extCSV for short.  An extCSV file consists of two sections: a metadata header and data tables.  The metadata header has rigid format and content rules, but the data tables are designed to be more flexible.  Level 1 data submissions are expected in the extCSV format, however, Level 2 and 3 data may also be submitted using this format.

 

Extended CSV (extCSV) Syntax Rules

 

1.    Fields are separated by comma characters, and the field width is variable.

2.    Records end with some combination of carriage-return and/or line-feed.

3.    If a data field contains either comma or double-quote characters, the entire field must be enclosed within double-quote characters when written.  Note: These added characters are removed when read.

4.    double-quote characters within a field are doubled (two double-quote characters) when written.  Note: These added characters are removed when read.

5.    Null values are represented as empty fields.

6.    Blank lines are ignored.

7.    Lines beginning with an asterisk are comments.

8.    Lines beginning with a pound (#) symbol are table names.

9.    The first record following the #TABLENAME record specifies column (field) names.  Each data column (field) requires a name separated by a comma.

Example

* The following data are simulated...

#TABLENAME

X,Y,Comment

12,35.6,Clear sky.

12.5,,Thunderstorm (can’t measure Y).

13,55.5,“It’s raining, it’s pouring!”

13.5,70,“Better start ““The Ark””.”

 

WOUDC Content Rules

1.    Table names are written in uppercase.  Field names are case-sensitive.

2.    Trailing nulls are assumed for unspecified data attributes.

3.    Each file must contain only one instance of the following static metadata tables;

#CONTENT

#DATA_GENERATION

#INSTRUMENT

#PLATFORM

5.    Each file must contain at least one instance of the following dynamic metadata tables;

#LOCATION

#TIMESTAMP

6.    Static metadata (#content, #data_generation, #instrument and #platorm) apply to all data within the file.

7.    Dynamic metadata (#location and #timestamp) apply until they are re-stated.  Class content that use the fields of these tables can modify the attributes (i.e., time can be updated by individual samples).

 

Required Metadata in extCSV.

 

Styles:

 
Bold:

Required attributes.

Italic:

Optional attributes.

Courier:

Sample data.

 

Example

Description

#CONTENT

Class,Category,Level,Form

WOUDC,Spectral,1.0,1

 

Static metadata - one per file

·       WOUDC definitions required

·       Form refers to the current version of the data form and content of each Category

 

#DATA_GENERATION

Date,Agency,Version,ScientificAuthority

1997-05-21,AES,1.5,Jim Kerr

 

Static metadata - one per file

·       Version is specific to an Agency, referencing algorithm and instrument revisions. Refer to the Special Note below for details

·       Agency is coded by the Agency acronym.

·       The ScientificAuthority is the person(s) who either authored the SSS or is qualified to author the SSS and who has undertaken to adhere to the standards described in the SSS and thus be responsible for the data quality.

 

#INSTRUMENT

Name,Model,Number

Brewer,MKII,15

 

Static metadata - one per file

·       WOUDC definitions required (Refer to Appendix G)

#PLATFORM

Type,ID,Name,Country,GAW_ID

STN,065,Toronto,CAN,71638

 

Static metadata - one per file

·       Three letter Country code per ISO-3166 [5]

·       Station number (ID) assigned by WOUDC

·       STN-stationary, FLI-flight, SAT-satellite

#LOCATION

Latitude,Longitude,Height

43.78,-79.47,198

 

Dynamic metadata - at least one per file

·       Decimal-Degrees, (North/East are positive)

·       Height is in meters above sea-level

#TIMESTAMP

UTCOffset,Date, Time

-05:00:00,1996-17-29,12:50:00

 

Dynamic metadata - at least one per file

·       Date and Time per ISO-8601 [6]

·       UTCOffset is the amount of time SUBTRACTED from the local time in order to obtain UTC time (where east is positive).  Local time is defined by the user and is equivalent to UTC =Time-UTCOffset.  From the sample data given,

UTC=12:50:00-(-05:00:00)=17:50:00

Time given in UTC has an offset of +00:00:00.

 

Special Note for the table” #DATA_GENERATION” and Category, “Version”, the number conventions are as follows.

These version numbers have the form major.minor (i.e. 3.2) where;

 

·       Major values are incremented with changes to the  processing algorithm.

·       Minor values are incremented when the characterisation or calibration values are changed

·       Minor values are reset to zero with changes in the processing algorithm.

5.3.3    The WUDC Metadata Content: Class and Category: FORM 1

 

WUDC data is defined as the WOUDC Data CLASS - “WOUDC”.  Within the CLASS WOUDC, there are several categories of UV data: Spectral, Multi-band, Broad-band and Pyranometer.

 

Tables 5.3.1 through 5.3.4 contain definitions for table and field names, for WUDC data content.  Additional table and field types can be defined as required.  These table definitions constitute the data file format - Form 1.  Changes to the data file submission format are viewed as infrequent.  However, should a change be necessary to either file format (structure) or data content, then a Form 1+i would be defined.

 

The use of the following table names is required for submission to the WUDC database.  The tables provide the logical structure for separating (and organising) the different physical data types.

 

 

Required Table and Field Names for the WOUDC CLASS & Categories

 

 

Table 5.3.1  Required Table names based upon data content (i.e. Category) definitions.

 

CLASS

Category

Table Names

 

 

 

WOUDC

Spectral

GLOBAL, DIRECT, DIFFUSE, ACTINOMETRIC

WOUDC

Multi-band

GLOBAL, DIRECT, DIFFUSE, ACTINOMETRIC, SIMULTANEOUS

WOUDC

Broad-band

GLOBAL, DIRECT, DIFFUSE, ACTINOMETRIC, SIMULTANEOUS

WOUDC

Pyranometer

GLOBAL, DIRECT, DIFFUSE, SIMULTANEOUS

 

 

 

 

 

Content Rules for WOUDC Data Tables

 

A minimum set of physical parameters are defined  for each table.  The number of defined parameters for each table can vary, that is to say, many more fields can be added, but a minimum number is required. Table 5.3.2 gives the minimum set of required field names for the listed tables within the CLASS  WOUDC.  Table 5.3.3 gives a required set of table and field names for ancillary and auxiliary data.  Table 5.3.4 lists a set of defined field names representing physical parameters relevant to the WUDC.  The spelling of table and field names must be exactly as shown in Tables 5.3.2 through 5.3.4.

 

Ancillary and Auxiliary data are best submitted as separate files.  For example, pyranometer data have been defined as a separate category (refer to Table 5.3.1) and therefore, require storage in separate files.

 


Table 5.3.2  Required Category, Table and Field names for the data CLASS -WOUDC.  The following category, table and field names must be specified as shown. (Form 1).  Note: Column 3 (or field name) Time for the Spectral and Multi-band tables is denoted in italics to indicate that field position is reserved, but not required.

 

Category      

Table Name(s)           

Field names (in order)

 

 

 

Spectral        

GLOBAL  

Wavelength,S-Irradiance,Time

Spectral        

DIRECT 

Wavelength,S-Irradiance,Time

Spectral        

DIFFUSE  

Wavelength,S-Irradiance,Time

Spectral

ACTINOMETRIC

Wavelength,S-Irradiance,Time

 

 

 

Multi-band        

GLOBAL  

Wavelength,S-Irradiance,Time

Multi-band        

DIRECT 

Wavelength,S-Irradiance,Time

Multi-band        

DIFFUSE  

Wavelength,S-Irradiance,Time

Multi-band

ACTINOMETRIC

Wavelength,S-Irradiance,Time

Multi-band

SIMULTANEOUS

Wavelength,GLS-Irradiance,DFS-Irradiance,DRS-Irradiance,Time

 

 

 

Broad-band

GLOBAL  

Time,Irradiance

Broad-band

DIRECT 

Time,Irradiance

Broad-band

DIFFUSE  

Time,Irradiance

Broad-band

ACTINOMETRIC

Time,Irradiance

Broad-band

SIMULTANEOUS

Time,GL-Irradiance,DF-Irradiance,DR-Irradiance

 

 

 

Pyranometer

GLOBAL  

Time,Irradiance

Pyranometer

DIRECT 

Time,Irradiance

Pyranometer

DIFFUSE  

Time,Irradiance

Pyranometer

SIMULTANEOUS

Time,GL-Irradiance,DF-Irradiance,DR-Irradiance

 

 

 

 

Note: The table SIMULTANEOUS refers to a single detector whereby the measurements are made in a near-simultaneous mode, but reported on the same time scale.  For example, measurements are recorded in 15 second intervals, first for global then for diffuse and an integrated value is reported every 15 minutes.  This integrated value is considered “simultaneous” for inclusion in this table.  Simultaneous measurements made using two or more independent detectors, requires a data file for each detector.  GL/GLS refers to Global/Global spectral, DF/DFS refers to Diffuse/Diffuse spectral and  DR refers to Direct/Direct spectral.

 

 

General Table Names for Ancillary and Auxiliary Data

 

Table 5.3.3  General Table Names for Ancillary and Auxiliary Data.  Note: the tables are shown with sample fields  which may be included in any of the above Categories.

 

Table name

Suggested field names

 

 

CALIBRATION

Specified by the data originator (Scientific Authority)

METEOROLOGY

Temperature,Pressure,Relative Humidity

METEOROLOGY_SUMMARY

Time,Temperature,Pressure,Relative Humidity

SURFACE_CONDITIONS

Albedo,

IMAGE

Filename,Comments  (Example: sky97001.gif)

 

 


Table 5.3.4 lists all the required and optional field names.  Those field names specified in bold are required, while those in italics are optional. (Abbreviations of the units are given in brackets.)

 

 

Table 5.3.4.  Accepted Field Names  or WUDC data submissions [7].

 

Field Name

Physical Units

Comments

 

 

 

Albedo

Dimensionless

 

Cloud Amount

 

special codes

 

Date

yyyy-mm-dd

ISO-8601 standard[6]

DF-Irradiance

Wm-2

Diffuse Irradiance

DFS-Irradiance

Wm-2nm-1

Diffuse Spectral Irradiance

DR-Irradiance

Wm-2

Direct Irradiance

DRS-Irradiance

Wm-2nm-1

Direct Spectral Irradiance

GL-Irradiance

Wm-2

Global Irradiance

GLS-Irradiance

Wm-2nm-1

Global Spectral Irradiance

Height

Metres (m)

Above sea level

Image filename and -path

No units

*.bmp, *.gif, *.jpeg etc.

Irradiance

Wm-2

 

Irradiation

KJ m-2 nm-1

Daily integrated irradiance

Latitude

Decimal degrees

North is positive

Longitude

Decimal degrees

East is positive

Pressure

Hecto-Pascal (hPa)

 

RelativeHumidity

Dimensionless (%)

 

S-Irradiance

Wm-2nm-1

Spectral Irradiance

S-Irradiation

KJm-2

Spectral Irradiation

Time

hh:mm:ss

ISO-8601 standard [6]

Temperature

Degrees Celsius (°C)

 

Wavelength

Nanometres (nm)

 

WindSpeed

ms-1

 

WindDirection

Decimal degrees

 

 

 

 

 


5.3.4    Examples

 

Examples are given below of the use of the WUDC metadata to describe UV data in the extCSV file format. 

The examples of spectral UV data are provided by the NSF (USA) the University of Manchester -UMIST (GBR), and the AES (CAN) as shown in Figures 5.3.4a-c.

 

Figure 5.3.3a  NSF Data (USA) in extCSV

 

#CONTENT

Class,Category,Level,Form

WOUDC,Spectral,1.0,1

 

#DATA_GENERATION

Date,Agency,Version,ScientificAuthority

1995-08-12,NSF,2.3,R. Booth

 

#INSTRUMENT

Name,Model,Number

Biospherical,SUV-100,5

 

#PLATFORM

Type,ID,Name,Country,GAW_ID

STN,239,San Diego,USA

 

#LOCATION

Latitude,Longitude,Height

32.82,-117.13,124

 

#TIMESTAMP

UTCoffset Date,Time

+00:00:00,1995-08-12

 

*High resolution spectral scan between 280-315 nm with a total of 176 points

*Increment is 0.2 nm

*Zenith angle is 58.38 and the azimuth angle is 268.25

 

#GLOBAL

Wavelength,S-Irradiance,Time,TSI sensor

280.27,2.6E-6,0:01:24,1.9049

280.48,0.4E-5

280.68,-0.2E-6

280.88,1.2E-6

281.08,-1.5E-6

281.28,0.4E-5,,1.9049

314.93,7.58828E-2

315.13,7.62414E-2

315.33,7.38935E-2, 0:03:49,1.87805


Figure 5.3.3b  University of Manchester Data (GBR) in extCSV.  Note in this example, that this file represents a single a day and individual spectral steps are time stamped and concatenated into one large day file of many spectra..

 

 

Same UMIST sample data in extCSV

 

#CONTENT

Category,Category,Level,Form

WOUDC,Spectral,1.0,1

 

#DATA_GENERATION

Date,Agency,Version,ScientificAuthority

1994-01-28,UMIST,1.0,Ann Webb

 

#INSTRUMENT

Name,Model,Number

Optronic,742,89304061

 

*Although the serial number for this instrument is unavailable for this example, *it is required within the data file.  In the #PLATFORM table, the station *number for Reading is assigned by the WOUDC.  TBA means To Be Assigned.

 

#PLATFORM

Type,ID,Name,Country,GAW_ID

STN,353,Reading,GBR

 

#LOCATION

Latitude,Longitude,Height

51.45,-0.93,66

 

#TIMESTAMP

UTCoffset,Date,Time

+00:00:00,1994-01-27

 

#GLOBAL

Wavelength,S-Irradiance,Time,Undefined

280.00,2.06699E-07,10:00:00,0.29

281.00,1.02418E-08,10:00:02,0.31

282.00,0.00000E+00,10:00:04,0.32

399.00,,10:01:48,,

400.00,,10:01:50,,

280.00,2.06699E-07,11:00:00,0.29

281.00,1.02418E-08,11:00:02,0.31

282.00,0.00000E+00,11:00:04,0.32

 

#METEOROLGY_SUMMARY

Time,Temperature,Pressure,RelativeHumidity

10:00:00,19.2

11:00:00,21.0,

12:00:00,23.0,


Figure 5.3.3c.  Atmospheric Environment Service (CAN) data in extCSV.  In this example, Spectral data are given with supporting Ancillary data (pyranometer) for both Global and Diffuse radiation.  Note that these data are contained within three individual files since each data sets is supplied by a separate instrument.

 

*Data file 1: spectral

 

#CONTENT

Name,Category,Level,Form

WOUDC,Spectral,1.0,1

 

#DATA_GENERATION

Date,Agency,Version,ScientificAuthority

1997-07-02,AES,1.0,Bruce McArthur

 

#INSTRUMENT

Name,Model,Number

Brewer,MKII,71

 

#PLATFORM

Type,ID,Name,Country,GAW_ID

STN,338,Regina,CAN,72863

 

#LOCATION

Latitude,Longitude,Height

50.21,-104.71,592

 

#TIMESTAMP

UTCOffset,Date,Time

-06:59:08,1997-06-08,06:45:00

*The data are reported in solar (apparent) time.

#GLOBAL

Wavelength,Irradiance,Time

290.0,0.00,06:45:00

290.5,0.00,06:45:03

291.0,0.00,06:45:06

325.0,6.395E-02,06:48;00

 

#METEOROLOGY

Temperature,Pressure,RelativeHumidity

15,972

 

#INSTRUMENT_CONDITIONS

Temperature

16.2

 

* The sequence of a #TIMESTAMP, #GLOBAL spectral scan, site and instrument *conditions (#METEOROLOGY, INSTRUMENT_CONDITIONS) continues throughout the file

 

#TIMESTAMP

UTCOffset,Date,Time

-06:59:08,1997-06-08,21:45:00

 

#GLOBAL

Wavelength,Irradiance,Time

290.0,0.00,20:05:00

290.5,0.00,20:05:03

291.0,0.00,20:05:06

325.0,4.669E-01,20:08;00

 


#METEOROLOGY

Temperature,Pressure,RelativeHumidity

18,976

 

#INSTRUMENT_CONDITIONS

Temperature

19.4

 

 

 

----- Start of New data file -----

 

 

* Data file 2 Pyranometer Data (Global)

 

#CONTENT

Name,Category,Level,Form

WOUDC,Pyranometer,1.0,1

 

#DATA_GENERATION

Date,Agency,Version,ScientificAuthority

1997-07-02,AES,1.0,Bruce McArthur

 

#INSTRUMENT

Name,Model,Number

Kipp and Zonen,CM21,920065

 

#PLATFORM

Type,ID,Name,Country,GAW_ID

STN,338,Regina,CAN,72863

 

#LOCATION

Latitude,Longitude,Height

50.21,-104.71,592

 

#TIMESTAMP

UTCOffset,Date,Time

-06:59:08,1997-06-08

 

* In this example, the pyranometer data are concatenated into one table *(#GLOBAL), with a single #TIMESTAMP table. The #METEOROLOGY and *#INSTRUMENT_CONDITIONS_SUMMARY tables are a summary.

 

#GLOBAL

Time,Irradiance

06:45:00,201

07:00:00,212

07:15:00,243

22:00:00,244

 

#METEOROLOGY_SUMMARY

Time,Temperature,Pressure,RelativeHumidity

07:00:00,15,972

08:00:00,16,973

 

#INSTRUMENT_CONDITIONS_SUMMARY

Time,Temperature

06:45:00,15.8

07:00:00,16.0


----- Start of New data file -----

 

 

* Data file 3 Pyranometer Data (Diffuse)

 

#CONTENT

Name,Category,Level,Form

WOUDC,Pyranometer,1.0,1

 

#DATA_GENERATION

Date,Agency,Version,ScientificAuthority

1996-07-02,AES,1.0,Bruce McArthur

 

#INSTRUMENT

Name,Model,Number

Kipp and Zonen,CM21,920066

 

#PLATFORM

Type,ID,Name,Country,GAW_ID

STN,338,Regina,CAN,72863

 

#LOCATION

Latitude,Longitude,Height

50.21,-104.71,592

 

#TIMESTAMP

UTCOffset,Date,Time

-06:59:08,1997-06-08

 

* In this example, the pyranometer data are concatenated into one table *(#DIFFUSE), with a single #TIMESTAMP table. The #METEOROLOGY and *#INSTRUMENT_CONDITIONS_SUMMARY tables are a summary.

 

#DIFFUSE

Time,Irradiance

06:45:00,99

07:00:00,101

07:15:00,111

22:00:00,112

 

#METEOROLOGY_SUMMARY

Time,Temperature,Pressure,RelativeHumidity

07:00:00,15,972

08:00:00,16,973

 

#INSTRUMENT_CONDITIONS_SUMMARY

Time,Temperature

06:45:00,15.8

07:00:00,16.0

 

 


5.3.5    Representation of Time

 

Typically, spectral data (where each record is Wavelength,Irradiance,Time) are represented in a single file for each day, but how time is represented within the file may be decided by the data originator.  A single day may have one #TIMESTAMP table for every scan, especially if each spectral step does not have an associated time.  Or the file may have one #TIMESTAMP table for the entire file, in which case some form of a time stamp (i.e. a start time, midpoint time stamp, end time or a time stamp for each spectral step) is to be indicated in the data table (#GLOBAL, #DIFFUSE,#DIRECT etc.).  If a file represents a month of data, then typically, there would be a #TIMESTAMP table for each day that data are reported as well as the time stamp indicated within the data table itself as previously mentioned.  If the amount of monthly data is such that these data can be accommodated in a single file, this is recommended.  Otherwise, daily data are best submitted in a single file.

 

 

5.4       Step 4: Assignment of Personal Data submission account

 

This is the final step before data submission can proceed.  Data originators are assigned a unique account to access the WOUDC ftp site through either conventional ftp or the Web.  It is recommended that the time between data submissions should be between one week and several months.  The optimum frequency is either bi-weekly or monthly.  This allows adequate time to process the data.

 

File naming is at the discretion of the data originator.  The personal ftp accounts allow write permissions.  Data originators have the flexibility to re-submit and overwrite existing data for a period of one week.  The onus is on the data originator to maintain a record of data submissions for use in the WOUDC Data Inventory database.  Every Sunday at 00:00 UTC, all contents of the account are extracted, archived and then removed.


6        Identification of Data Quality

 

Data quality control and assurance is primarily the responsibility of the data originator.  The purpose of the SSS is to ensure and illustrate that the appropriate measures have been undertaken to provide high quality data for the inclusion into the WOUDC database.  Once a file has been submitted to the WOUDC, data quality is monitored at various stages during data processing.  Database quality control consists of checking for file format and metadata content, inspection of data value ranges and data redundancy checks.

 

Initially, a file will be tested for adherence to the file format specifications, but later, higher level statistical summaries may be generated, which identify anomalous values, calibration problems etc.  Although the later examples involve more detailed knowledge of the data, the archive already includes enough data to make some critical judgments and general assessments about the data.  As the volume and statistical knowledge increase, the scope of these assessments will be broadened.

 

This section will focus on the initial stages of the quality control path, how are the files checked, what happens to the original data and what sort of data flagging occurs.

 

 

6.1       General principles of the WUDC Identification of Data Quality

 

The are four basic elements in the quality control of WUDC data. 

 

Specifically the four QC elements are:

 

1.    Acceptance of the Data Passport or SSS.

2.    Examination by the WUDC.  Data are checked for file format, presence of required meta data and valid value ranges.

3.    Examination by External groups

4.    Additional QA/QC by the WMO and AES Advisory Committees.

 

The first is the joint responsibility of the originator and the WUDC while the second is an examination of the data solely by the WUDC.  The third and fourth elements are not strictly defined and are expected to evolve. Data that have passed through the first two elements are published on the WOUDC ftp server.

 

 

6.2       The Data Passport or SSS

 

The single most important step in the quality control process is the acceptance of the Data Passport or SSS.  Guidelines for quality control with regards to the SSS have been established and published by the WMO/GAW Scientific Advisory Group on Ultraviolet radiation (SAG_UV) [3].  In addition, examples of SSS documents can be examined on the WOUDC ftp server and Web site.  The subjects to be covered are, therefore, well established.  However, the writer of the SSS need not follow a rigid prescription.  The contents of the SSS are discussed in Section 5.1.

 


6.3       Examination by the WOUDC

 

Once a file arrives at the WOUDC, the data are first checked for adherence to the correct format and content rules established in Section 5.3.  Only those files that meet the metadata requirements are to be indexed in the WUDC database.  It is not necessary for all files to conform to the extCSV file format, provided that the required metadata can be extracted from the file.

 

Examination of data values includes the identification of obvious errors such as misprints or data transmission errors.  Data values are range checked and any anomalous values are further examined.  When the data have been processed through the initial stages, output files ready for posting on the ftp site may include an additional data index (flag) which is aimed at providing the data client with information about any unusual or anomalous values of the data itself or derived properties of the spectrum.

 

 

6.3.1    Additional Data Quality Identification Procedures

 

An additional data index (flag) has been established for WUDC output data products (Appendix D). The aim is to provide information about unusual or anomalous values or a more detailed description of other useful characteristics.  Each flag is a separate digit and can have values in the range 0-3 inclusive.  Code 0 indicates that the value of the relevant  property is in the usual range of values for  that property while the codes 1,2 and 3 indicate  increasingly unusual values. The interpretation is as follows: Code  0 means no problems or potential problems were found, Code 1 means that  there  may be a minor problem  with the data. Normally, 3-5% of all data have Code 1. Code 2 shows either unusual observing conditions  or  some problem  with  the  instrument.  The percentage depends on the criteria and is different for the various flags.  Code 3 shows a major disturbance in the data (property) that the "user" should  definitely know about. While Codes 1, 2 and 3 raise the possibility  of instrument malfunctions, it is important to note that spectra with known significant instrument problems have already been rejected. However, instrument problems cannot be considered to be eliminated from these data.

 

 

6.4       Examination by Others

 

The WOUDC has benefited considerably from research done by users of the data and expects to continue to do so.  The user may find aspects of the data and deficiencies that are entirely unexpected by the originator.  Notification of the WOUDC can produce better data processing and comments; references and/or papers by users can be included in the WOUDC.

 

 

6.5       Role of WMO and AES Advisory Committees                

 

Advisory Committees can help the WUDC in a number of ways.  The AES committee has special expertise in the management of related data centres.  The WMO/GAW SAG_UV has a wide base of experience in many aspects of UV radiation and has the task of coordinating UV measurement activities for the WMO.  The SAG_UV has a subcommittee on UV data archiving  which is intended to interface with the WUDC.  As well as providing advice on techniques and requirements, the people on these committees can assist WUDC by being model or test clients, that is originators and users of data, and by promoting the use of the centre.  Finally, the committees can ratify or not ratify critical scientific decisions made by WUDC staff or more generally to help WUDC make such decisions.  This might be particularly important with regard to decisions to accept or reject submitted data.


7        Access and Data Retrieval

 

Data access and retrieval are core functions of the WUDC. The primary search elements will be those fields defined in the metadata tables and content rules such as: the data CONTENT and Category, the instrument in use and it’s location, the Source Agency, Location and Time stamp.  The format for data outputs will generally appear the same.  The basic output format will be the extCSV which will provide data clients an easy means to search a broader set of data by using the CLASS and Category fields.  It is likely that enhancements to existing data sets will occur as well as the inclusion of value added data products such as statistical summaries.  Therefore, some variations in the representation of data output should be expected.

 

The WOUDC, on a point of principle , will provide access to all data in their native, as submitted, format, subject only to possible restriction required by the data originator.  The data will normally be on-line but, in the case of large volumes, special arrangement may be needed.

 

Regular updates and enhancements to data outputs will be posted at the WOUDC Web site.

 

The WOUDC data archive is available at an Internet ftp site and is accessible by means of conventional ftp or through the Web. The Internet site provides two levels of access to the posted data. 

 

1.       A generic username/password access that presently exists, and will be maintained.  This level permits access to all data output products posted by the WOUDC on the Internet.

2.       The second type of access is defined as “Restricted” and will be available to those data originators and clients who wish to negotiate special access agreements.

 

Both levels of data access are described in more detail later in this chapter. 

 

 

7.1       Addresses

 

Mail:                   World Ozone and Ultraviolet Radiation Data Centre (WOUDC)

   Atmospheric Environment Service

   4905 Dufferin Street

   North York, Ontario, CANADA

   M3H 5T4

E-Mail                woudc@ec.gc.ca

FTP Access       ftp.tor.ec.gc.ca

WWW Access    www.tor.ec.gc.ca/woudc

 

 

7.2       General Access

 

General access is a quasi-anonymous access to the entire suite of WOUDC data output products posted on the Internet.  The generic username: woudc and password: woudc* will continue to be used.  There are no restrictions imposed on the reading or viewing of data other than the use of the generic username and password.  This access is essentially universal and conforms to what WOUDC staff believe to be the intent of WMO data agreements and to certain provisions in the Vienna Convention of 1985 [8], [9].  Nevertheless, users are asked to read relevant SSS files and to abide by any specified  restrictions.

 

At present, the WOUDC Data Inventory will not allow searches to “drill down” to individual file attributes that are related to data content such as Temperature, Irradiance or Total ozone value.  Instead, a selection of files will be returned which meet the metadata query and it is the task of the data client to develop higher order relational database searches based upon individual requirements.  These files allow relatively easy parsing out of elements to load conventional relational databases because the form is the same for all output files, only the data content varies.

 

 

Key Elements of the WOUDC Inventory Database

 

·       The archive is organised as an ASCII flat-file system using a hierarchical directory structure of raw, processed or gridded data files based on the metadata.

·       Instrument and site information are stored at the beginning of each file as part of the metadata.

·       No formal requirements for file formats, with respect to data submission, aside from the required metadata.  ExtCSV is suggested since data output files will be represented using this format.

·       Database queries are based on metadata (what files are available, from when and where, etc.).

·       Files from the same CLASS, in this case WOUDC, “belong together”, but have different “contents”; spectral, Multi-band, broad-band or pyranometer.

 

 

7.3       Restricted Access and Protocol

 

The second level of data access is defined as “restricted” and will be available to those data originators and clients who wish to negotiate special access agreements.  Data originators and clients must apply to the WOUDC to view the restricted data archive. 

 

 

 

Although  believing strongly that the merits of fast universal distribution of data far outweigh any advantage in not distributing data, the  WUDC respects the positions of individual data originators and agencies and has attempted to accommodate them as recommended by the WMO/GAW Scientific Advisory Group on UV Radiation in May, 1995.

 

 

 

WOUDC continues to offer data originators the flexibility to generate a second volume of data that can only be accessed by special users who have signed a protocol agreement, which is posted on the WOUDC ftp server, and who would be issued with personal passwords of limited duration.  

 

The Scientific Sponsorship Statement can be used to prescribe certain uses of the data.  Someone who violated that prescription could be censured by the WUDC as well as by the originator.  In such an instance his or her password could be canceled in addition to the censure.  


 

7.4       Data Archive Structure

 

The present form of the WUDC ftp site, directory structure is outlined below.  Updates or information about changes to WUDC procedures or data formats will be posted on the WOUDC Web site.

 

 

FTP Server Directory & File Structure

 

[wudc]

   |--- readme.1st

   |--- stations.wudc

   |

   |--- [archive]

   |        |--- process.txt

   |        |

   |        |--- [Level_0]

   |        |

   |        |--- [Level_1]

   |        |     

   |        |--- [Level_2]

   |        |         |

   |        |         |--- [Station Name 1] (Example: Edmonton)

   |        |                    |

   |        |                    |--- help files & site specific documentation

   |        |                    |

   |        |                    |--- [year] --- UVBdddyy.iii

   |        |

   |        |                    Where: ddd is Julian day

   |        |                            yy is year

   |        |                           iii is instrument id (serial #)

   |        |--- [Ancillar]

   |        |       |

   |        |       |--- [Station name]  (Example: Toronto)

   |        |       |        |--- [Type of Ancillary Data]  (Example: pyranom)

   |        |

   |        |--- [Agency]

   |                |

   |                |--- [AES]

   |                |      |--- profile.aes

   |                |      |--- AES.SSS

   |                |--- [JMA]

   |                |--- [NSF]

   |

   |--- [document]

   |        |--- overview.wudc

   |        |--- fmtout02.txt

   |        |--- flwudc2.txt

   |

   |--- [software]

 

 

The “readme.1st" file is a general guide to WUDC subdirectories.  The "stations.wudc" contains all pertinent information related to each station and is useful for referencing station numbers

 

Within the subdirectory [archive] are WUDC sanctioned data (for retrieval), along with any accompanying support documentation provided by the data originator(s) from the sponsoring agency.  Typically, this information is included as a text file, part of the Scientific Sponsorship Statement (SSS) or in addition to the SSS.  Information about the observation programs, agency profiles and SSS files are also found in the [agency] subdirectory

 

The: Agency.SSS is the Scientific Sponsorship Statement file and is provided by a qualified sponsor from the submitting organisation.  Each data originator must provide an SSS in the form of a text file.  The Scientific Sponsorship Statement files may represent one station or many stations under the sponsorship of the single agency.  SSS files are named in UPPERCASE.  Data clients are strongly urged to consult these files.

 

The file "process.txt" describes the data processing procedures the WOUDC has followed to provide the data output products found in the [archive] directory.

 

The subdirectory [woudc/temp/wudc] contains data which has been submitted to the WUDC in some format which does not currently conform to the standard documented format for data presentation.  These data represent the “native” format as received by the WOUDC.

 

[woudc]

     |

     |--- [temp]

            |

            |--- [wudc]

                    |

                    |--- [Agency acronym]

                                |

                                |--- [year]

 

In some instances (example, large volume of data) these data files may not be kept on line, however, these data will be made available if requested.  Also, if the WOUDC or the data originator(s) reformats these data files into the standard, extCSV format, then the original data files (in non-standard format) may be removed from the on-line archive, but would always be made available on request.


8        Acknowledgments

 

The authors would like to acknowledge the contributions of the following individuals: C.T. McElroy, J.B. Kerr, L.J.B. McArthur, and D.V. Barton from the Atmospheric Environment Service, Canada, G. Blair from Vision Works, Canada, Ann Webb of the University of Manchester Institute of Science and Technology, England and Arve Kylling (formerly of Norut It) NILU, Norway.

 

 

9        References

 

[1]        NSF Polar Programs UV Spectroradiometer Network 1994-1995 Operations Report.  C.R. Booth et

al., Biospherical Instruments, Inc., 5340 Riley Street., San Diego, CA.., USA.

 

[2]        Network for the Detection of Stratospheric Change, A Status and Implementation Report, Prepared by M.J. Kurylo and S. Solomon, NASA Upper Atmosphere Research Program and NOAA Climate and Global Change Program, January, 1990.

 

[3]        WMO, Ann Webb ed.: "Guidelines for Site Quality Control of UV Radiation Measurements", Global Atmospheric Watch, WMO/GAW Report 126, 1998.

 

[4]        WMO, Gunther Seckmeyer ed.:, "Guidelines for Instruments to Measure Solar Ultraviolet Radiation" Global Atmospheric Watch, to be published, WMO/GAW Report 1998.

 

[5]        ISO 3166 Country and Currency Codes, International Standards Organization (ISO), Switzerland, (1995).   http://www.iso.ch/infoe/otherpub.html and ftp://ftp.ripe.net/iso3166-countrycodes.

 

[6]        ISO 8601 Numeric presentations of Date and Time, International Standards Organization (ISO), Switzerland, (1997).  http://www.iso.ch/infoe/otherpub.html and http://www.iso.ch/cate/d15903.html for information on how to obtain an official version of this publication.  http://www.mcs.vuw.ac.nz/technical/SGML/doc/iso8601/ISO8601.html or http://www.ft.uni-erlanger.de/~mskuhn/iso-time.html for abbreviated versions of this document.

 

[7]        R. Dogniaux, et al., "Solar Meteorology: Units and Symbols": Int. J. Solar Energy, 1984, 2,

p249‑255.

 

[8]        United Nations Environment Programme, Vienna Convention of the Protection of the Ozone Layer, Final Act., United Nations Environment Programme, (1985).

 

[9]        World Meteorological Organization, Twelfth World Meteorological Congress, Abridged Final report with Resolutions, WMO-No.827, Resolution 40, Secretariat of the WMO, Geneva, Switzerland, 30-May-21 June, 1995.

 

 

 


Appendix A    Scientific Sponsorship Statements

 

 

Scientific Sponsorship Statement - (AES.SSS)

 

Brewer spectral data from Canadian Stations

 

Toronto  1989-              Resolute  1991-             Montreal 1993-

Edmonton 1992-            Churchill 1992-              Regina 1994-

Winnipeg 1992- Saturna   1991-

Halifax  1992-               Saskatoon 1990-

 

 

General Methodology.

 

The data are from UV-B scans of the Brewer instrument [1]. 

 

The calibration source comprises calibrated DHX 1000 watt lamps that are traceable to the US National Institute of Standards and Technology (NIST).   These lamps were either calibrated by Optronics Inc., based on NIST standards, or directly by NIST.

 

Daily stability checks are done on the Brewer by reading the signals from an internal 20 watt quartz halogen lamp.  Prior to 1990, a 200 watt external lamp was used roughly every month. These stability checks are done primarily to detect malfunctions and for ozone measurements rather than to establish UV responsivities

 

The Toronto Brewer #014, and two traveling standard Brewers #017 & #039 have been calibrated roughly six times per year with 1000 watt lamps at Toronto.

 

The field stations (Halifax, Edmonton and Winnipeg) have been calibrated at approximately each year by bringing two 1000 watt lamps and one traveling Brewer instrument to the site.

 

Laboratory tests have shown that there is a wavelength-dependent temperature effect on responsivity of up to 4% over the operating range of temperature. The measurements (at this time)  have not been corrected for any temperature effect.

 

The wavelength on the Brewer is checked several times per day by reference to a mercury discharge lamp.  Although the control of the wavelength setting is in steps of about 0.007nm and the finding can be reproduced to 0.002nm, changes in the lamp and the accuracy of the dispersion equation limit the wavelength accuracy.

 

The pass-band is approximately triangular with a 0.55 nm full width at half intensity.( See note 1).

 

The spectra are corrected for instrumental stray light which affects the measurements at wavelengths less than 305 nm where the light intensity is very small. The method of stray light correction was revised in August, 1996 from the "5 wavelength" correction which subtracts the signal measured between 290 and 292 nm from the rest of the spectra (ref. 3) to the "laser scan" correction which uses a scan of the HeCd laser (325.03 nm) to define the stray light characteristics of the single monochromator Brewer instrument. The Toronto data are corrected using a laser scan measured on the Toronto instrument (#14). As of August 1996, because laser scans from the other field instruments are not yet available, the data are derived using estimated laser scans with parameterized characteristics specific to each instrument.

 

Results

 

The Toronto instrument and the traveling Brewers show a month-to-month reproducibility of about 2% over the five years period. 

 

The Toronto Brewer shows long-term spectral responsivity drifts ranging from -0.3% per year to +1.0% per year based on 1000 watt lamp readings.

 

On field visits results from the lamps are usually within 2% of the result derived from side-by-side  measurement with the traveling standard Brewer.

 

Uncertainty estimates (2 sigma):

Wavelength                 0.05nm

Intensity                       Field stations   7%

                                    Central station 6%.

 

 

Notes

 

1.    A scan of the Helium-Cadmium laser emission at 325 nm has been submitted to WOUDC as L3250141.DAT.

2.    New 1000 watt lamps and lamp housings are now being used.  This will enable more frequent calibrations at all sites.

3.    Various new methods of quality control and checking calibrations are being developed.  These include correlation with satellite measurements and with local measurements of spectrally integrated downward irradiance.

4.    The variability in the Brewer readings on the 1000 watt lamps is currently treated as entirely due to the instrument.  However, there is clear evidence of changes in the lamps and of change in results due to small differences in procedures.  It is hoped that a more sophisticated treatment, based on a larger number of lamp calibrations, can be developed.

5.    It is expected that the uncertainty of new and existing data can be reduced in future.

 

D.I. Wardle and J.B. Kerr 95 04 28, revised 96 04 02, revised again 96 08 30)

 

 

References

 

J.B. Kerr, C.T. McElroy, D.I. Wardle, R.A. Olafson and W.F.J. Evans:1984 The automated Brewer spectrophotometer.  Atmospheric Ozone: Proceedings of the Quadrennial Ozone Symposium held in Halkidiki, Greece, 3-7 September 1984.  D. Reidel Publishing Company.

 

D.I. Wardle, J.B. Kerr and C.T. McElroy:  Operational ozone and spectral UV-B monitoring in Canada:  13th UOEH International Symposium on the Impact of Increased UV-B Exposure on Human Health and Ecosystems. 13-15 October 1993, Kitakyushu, Japan.

 

J.B. Kerr and C.T. McElroy:  Evidence for Large Upward Trends of Ultraviolet-B Radiation linked to Ozone Depletion. Science 262, 1032-1034, 12 November 1993


Scientific Sponsorship Statement - (JMA.SSS)

 

Preliminary Scientific Sponsorship Statement for the data from the UV-B monitoring network of the Japan Meteorological Agency,  JMA.SSS.

 

 

This document describes the deployment of instruments and the responsivity calibration procedures that are used in the JMA network.  A more extensive sponsorship statement which deals with other aspects of the data will be provided later.

 

The instruments in the network are Brewer MK-II spectrophotometers located as shown in Table 1.

 

Table 1         JMA Network for UV monitoring.

[Station]                       [location]    [Instrument]              [purpose]

 Sapporo                                43:03N  141:20E     #058                       Routine Observation [from 1991]

 Tsukuba                               36:03N  140:08E     #052                       Routine Observation [from 1990]

 Tsukuba                               36:03N  140:08E     #113                       Standard use

 Kagoshima                           31:38N  130:36E     #059                       Routine Observation [from 1991]

 Naha                                      26:12N  127:42E     #060                       Routine Observation [from 1991]

 Syowa (Antarctica)             69:00S     39:35E     #091                       Routine Obs.[from 1991] (1991-94: #034)

Routine observations are made at every hour from sunrise to sunset.

 

QC (calibration) system in the network.

The responsivity of each Brewer is obtained by measuring the irradiance from NIST lamps supplied with 7.900 or 8.000A constant current just before being sent to observation site (we define it calibration).

We use two other kinds of lamp:-  internal lamp which is installed already in spectrometer and the external one.  The time change of the responsivity is corrected by comparison between external and internal lamp(we call stability check).  There are 5 external lamps at each site which are checked against themselves in the dark, once a week for two lamps, once a month for three lamps, and once each half year for five lamps.  Simultaneously the responsivity of each spectrometer is also checked.  The internal lamp is used three times a day, sunrise, noon and sunset times in order to monitor the responsivity of each spectrometer.

 

An international intercomparison was carried out at Table Mountain near Boulder (USA) in September 1994.  From Japan,  spectrometer #113 of Brewer was brought as a Japanese standard, and according to the results we revised the responsivity of all other Brewers used in UV-B network in Japan.  These were based on the intercomparisons between standard #113 and the others for routine observation use at each station.

 

The latest international intercomparison of the standard spectrometer between Japan and Canada was carried out during the period February through March 1997 at AES in Toronto, Canada.  Calibration activities are summarized in tables 2,3 and 4

 

Definition of terms:

Intercomparison.  The comparison between JMA's standard instrument and the instruments in routine use

and between the JMA standard and standard instruments of other agencies ( i.e. AES).

Calibration.            The source of calibration is a 1000W lamp that is traceable to NIST.

Stability check.     Monitoring for the time change of responsivity using lamps that are not calibrated.

 

.
Table 2  Types and frequency of calibration activities in the JMA UV network.

[Spectral interval] [Frequency.]                         [Scans]

Intercomparison                   0.25nm                    every 3 years                        see 3.(1)

Calibration                             0.50nm                    every 3 years                        see 3.(2)

Stability checks:

External 50W lamp               0.50nm                    2 lamps: every week             3 double scans

3 lamps: every month          3 double scans

5 lamps: every half year      3 double scans

Internal 20W lamp                variable                  3 times a day                         5 scans

 

note1: external lamps are checked simultaneously

note2: the responsivity of instrument for every month are calculated by this stability check

note3: external lamp is not necessary to be traceable to NIST lamp

note4: spectral interval for internal lamp depends on wavelength being scanned

note5: The intercomparison and the calibration specifics do not apply to the observation at Syowa.

 

Table 3 The most recent intercomparisons for of JMA spectrometers

[Instrument]          [Frequency]          [Date of latest]                      [Site]                       [standard instrument]

#113 Standard       every 2 years        Feb. - Mar., 1997                   Toronto                 AES #013.

#058 Sapporo        every 3 years        Jul.,1997                 Sapporo                 #113

#052 Tsukuba       every  year            Jun.,1997                                Tsukuba                                #113

#034 Tsukuba       every  year            Jun.,1997                                Tsukuba                                #113

#059 Kagoshima   every 3 years        Sept.-Oct.,1995                     Kagoshima            #113

#060 Naha             every 3 years        Oct.,1996                                Naha                       #113

#091 Syowa(Antarc.)  Temporal        Sept.-Oct.,1993                     Tsukuba                                #113

 

Table 4.  Details of calibration procedures

(1) Intercomparison for each are done by comparing with the standard measuring solar radiation.

            sky condition            clear sky

            frequency                  every 30 minutes from sunrise to sunset (several days)

            range                          290-325nm per 0.25nm

            error in timing           < 1.0 s

(2) Calibration by NIST lamp

           NIST lamp  DXW type 1000 W lamps (Eppley,inc. and Optronic,inc.)

           distance                      50.0 cm

           lamp housing             manufactured Takasho,inc., Japan

           power supply             manufactured Takasago,inc., Japan

           error of ampere          < 0.0005 A

           range                           290-325nm per 0.5nm double-scans

           scans                           15 times      (It takes about 3 hours to complete a lamp test)

(3) Check of responsivity by external lamp after (1) and (2)

          lamp and holder          5 halogen 50 W lamps (SCI-TEC,inc.)

          distance                       5 cm

          power supply and lamp housing          : SCI-TEC,inc.

          Range                           290-325nm per 0.5nm double-scan

          scans                            3 times    (It takes about 40 minutes to complete a lamp test)

 

 

Masaatsu  Miyauchi

97/09/15:    for the

Japan Meteorological Agency

 


Scientific Sponsorship Statement - (USDA_CSU.SSS)

 

 

Scientific Sponsorship Statement:

USDA Ultraviolet Radiation Monitoring Program

File Date: 6 March 1998

 

UV-MFRSRs

 

The UV-MFRSR is a seven channel ultraviolet version of the Multi-Filter Shadowband Radiometer described by Harrison et al. (1994). This new shadowbanded instrument contains separate solid-state detectors which utilize Barr Associates, Inc. ion-assisted-deposition filters, each with a nominal 2 nm full-width at half-maximum (FWHM) bandwidth. The seven filters have nominal center wavelengths at each of 300, 305, 311, 317, 325, 332 and 368 nm.  Each detector shares a common diffuser, thereby allowing total horizontal (no blocking) and diffuse horizontal (direct beam blocked) irradiance to be measured simultaneously at each passband. Direct normal irradiance is derived in near-real time by firmware included within the data logging component of the instrument. All three measurements are returned for each 3-minute interval.

 

The Lambertian response of MFRSR instruments has been described by Harrison et al. (1994) and Michalsky et al. (1995).  Precise angular corrections are applied to the direct-beam measurement (but not the diffuse) based upon an independent radiometric characterization of individual detectors made through the diffuser along two orthogonal planes (Michalsky et al. 1995).

 

The relative spectral response function (SRF) of the detector is determined by focusing a 150 Watt Xenon arc lamp onto the entrance slit of an Acton Spectra-Pro 275 monochromator equipped with a 1200 grooves per mm grating.  The monochromatic beam passes through the exit slits and strikes a beam-splitter which directs half of the light to a reference NIST-traceable photodiode and the other half to the detector (the diffuser/ filter/photodiode combination). The irradiance determined by the reference photodiode is used to adjust the signal for the spectral characteristics of the lamp in order to yield the detector's relative spectral response at that wavelength. It is assumed that the differences between the spectral response of the two photodiodes is negligible over the narrow passband being measured. The measurement is repeated over the passband by scanning the wavelength of the monochromator in 0.1 nm steps in the UV and 1.0 nm steps in the visible.

 

Calibration of the UV-MFRSR is established through the use of a standard lamp. The SFR of a detector is measured as described in the previous paragraph. Next the voltage of the detector (diffuser/filter/photodiode combination) is recorded with the detector exactly 50 cm from a 1000 Watt NIST-traceable FEL lamp spectral irradiance standard. The SRF is convolved with the known absolute lamp spectral irradiance to give the effective power incident on the detector. Dividing the measured voltage by the effective power produces the spectral responsivity for each individual channel of the detector in Volts/Watts per meter-squared per nanometer (YES, 1994).  Langley analysis of each detector is also pursued as a means of calibrating instruments but is not currently being applied routinely to network data.

 

Only preliminary estimates of instrument stability, precision and bias are available for the instrument due to the short network measurement history.  Bigelow et al. (1998) have reported precision of < 3% within a single passband based upon side-by-side comparisons of two prototype UV-MFRSR instruments. However, biases between the same two instruments from -10% to +3% depending upon the passband being investigated. Comparisons to a Brewer on a single clear day have yielded biases of 1 to 20%. Comparisons of Langley to NIST standard lamp calibrations for the same UV-MFRSR on 4 occasions have yielded agreements to within 3%, again depending upon the specific passband being measured. It should be reiterated that these results are not considered definitive and more work needs to be done to establish the true accuracy of these instruments.

 

The following references document the techniques used by the USDA UVB Monitoring Program to obtain calibrations of network instrumentation.

 

                Bigelow, D.S., J.R. Slusser, A.F. Beaubien and J.H. Gibson, 1998,

                The USDA Ultraviolet Radiation Monitoring Program, Bull. Amer. Meteor. Soc. (In press)

 

                Yankee Environmental Systems, Inc., 1994. Yankee Environmental

                Systems Optical Calibration Facilities. YES Turners Falls, MA. p16

 

 

UV-MFRSR instrumentation is calibrated at least annually. The instruments have been calibrated primarily by the instrument manufacturer but calibrations on some instruments have additionally been conducted by the NOAA Central UV Calibration Facility (CUCF) at Boulder, Colorado. Some instruments have participated in the NOAA/NIST sponsored North American Interagency Spectroradiometer Intercomparisons. Routine annual calibrations include a cosine response characterization, spectral response function characterization, and calibration against a standard lamp.

 

REFERENCES

 

Harrison, L., J. Michalsky and J. Berndt, 1994. Automated multi-filter rotating shadowband radiometer: an instrument for optical depth and radiation measurements. Applied Optics, 32, 343-349.

 

Long,C.S., A.J. Miller, H. Lee, J.D. Wild, R.C. Przywarty and D. Hufford, 1996. Ultraviolet Index Forecasts Issued by the National Weather Service. Bull, Amer. Meteor. Soc., 77,729-748.

 

Michalsky, J.J., L.C. Harrison and W.E. Berkheiser, 1995. Cosine response characteristics of some radiometric and photometric sensors, Solar Energy, 54, 397-402.

 

 

 

Dave Bigelow

US Department of Agriculture at Colorado State University

March 1998


 

Appendix B   The Agency Profile

 

 

WUDC Agency Profile

                                                                                                 

Agency Name

 

Agency Acronym

 

 

 

Mailing Address

 

 

 

 

 

E-mail

 

Phone Number

 

Fax Number

 

 

Contact Person(s)

 

 

 

 

Each individual station should be submitted on a separate form with a description of all instruments there.

 

 

Sample WUDC Agency Profile

                                                                                                 

Agency Name

Atmospheric Environment Service

Agency Acronym

AES

 

 

Mailing Address

 

4905 Dufferin Street

Downsview, Ontario

CANADA   M3H 5T4

 

E-mail

Jim.Kerr@ec.gc.ca

Phone Number

1-416-739-4635

Fax Number

1-416-739-4281

 

Contact Person(s)

 

James B. Kerr or David I. Wardle

 

 


Station Information

 

Station Name

 

 

 

Latitude

 

Longitude

 

Elevation

 

Mean Pressure

 

 

 

Instrument Description

 

 

 

Instrument type

 

Model and serial numbers

 

 

Instrument Description

(include spectral range or wavelengths and pass-band(s))

 

 

Observation Program and Schedule   

 

 

 

Type of Measurement

 

Frequency of Measurement

 

 

 

 

 

Instrument Description

 

 

 

Instrument type

 

Model and serial numbers

 

 

Instrument Description

(include spectral range or wavelengths and pass-band(s))

 

 

Observation Program and Schedule   

 

 

 

Type of Measurement

 

Frequency of Measurement

 

 

 

 

 


Sample Station Information

 

Station Name

Toronto

 

 

Latitude

43.78

Longitude

79.47

Elevation

198 m

Mean Pressure

1004 hPa

 

 

Instrument Description

 

 

 

Instrument type

Brewer

Model and serial numbers

Mark II, 14

 

Instrument Description

(include spectral range or wavelengths and pass-band(s))

 

Single monochromator

Special range 290-325 nm

Resolution 0.55 nm   FWHI

Observation Program and Schedule   

 

 

 

Type of Measurement

Spectral GLOBAL, Spectral Direct

Frequency of Measurement

c  2hr-1

 

 

 

 

Instrument Description

 

 

 

Instrument type

Solar Light

Model and serial numbers

401- 0909

 

Instrument Description

(include spectral range or wavelengths and pass-band(s))

 

Broadband erythemal

 

Observation Program and Schedule   

 

 

 

Type of Measurement

Global erythemal (meds h-1)

Frequency of Measurement

Every minute

 

 


Appendix C   ISO 3166 Country Codes

 

 

ISO 3166 Country Codes [5]

 

Updated by the RIPE Network Coordination Centre.

 

Source: ISO 3166 Maintenance Agency

 

Latest change: Tue Jan  7 15:57:16 MET 1997

 

COUNTRY

A 2

A 3

No.

 

 

 

 

AFGHANISTAN

AF

AFG

4

ALBANIA

AL

ALB

8

ALGERIA

DZ

DZA

12

AMERICAN SAMOA

AS

ASM

16

ANDORRA

AD

AND

20

ANGOLA

AO

AGO

24

ANGUILLA

AI

AIA

660

ANTARCTICA

AQ

ATA

10

ANTIGUA AND BARBUDA

AG

ATG

28

ARGENTINA

AR

ARG

32

ARMENIA

AM

ARM

51

ARUBA

AW

ABW

533

AUSTRALIA

AU

AUS

36

AUSTRIA

AT

AUT

40

AZERBAIJAN

AZ

AZE

31

BAHAMAS

BS

BHS

44

BAHRAIN

BH

BHR

48

BANGLADESH

BD

BGD

50

BARBADOS

BB

BRB

52

BELARUS

BY

BLR

112

BELGIUM

BE

BEL

56

BELIZE

BZ

BLZ

84

BENIN

BJ

BEN

204

BERMUDA

BM

BMU

60

BHUTAN

BT

BTN

64

BOLIVIA

BO

BOL

68

BOSNIA AND HERZEGOWINA

BA

BIH

70

BOTSWANA

BW

BWA

72

BOUVET ISLAND

BV

BVT

74

BRAZIL

BR

BRA

76

BRITISH INDIAN OCEAN TERRITORY

IO

IOT

86

BRUNEI DARUSSALAM

BN

BRN

96

BULGARIA

BG

BGR

100

BURKINA FASO

BF

BFA

854

BURUNDI

BI

BDI

108

CAMBODIA

KH

KHM

116

CAMEROON

CM

CMR

120

CANADA

CA

CAN

124

CAPE VERDE

CV

CPV

132

CAYMAN ISLANDS

KY

CYM

136

CENTRAL AFRICAN REPUBLIC

CF

CAF

140

CHAD

TD

TCD

148

CHILE

CL

CHL

152

CHINA

CN

CHN

156

CHRISTMAS ISLAND

CX

CXR

162

COCOS (KEELING) ISLANDS

CC

CCK

166

COLOMBIA

CO

COL

170

COMOROS

KM

COM

174

CONGO

CG

COG

178

COOK ISLANDS

CK

COK

184

COSTA RICA

CR

CRI

188

COTE D'IVOIRE

CI

CIV

384

CROATIA (local name Hrvatska)

 HR

HRV

191

CUBA

CU

CUB

192

CYPRUS

CY

CYP

196

CZECH REPUBLIC

CZ

CZE

203

DENMARK

DK

DNK

208

DJIBOUTI

DJ

DJI

262

DOMINICA

DM

DMA

212

DOMINICAN REPUBLIC

DO

DOM

214

EAST TIMOR

TP

TMP

626

ECUADOR

EC

ECU

218

EGYPT

EG

EGY

818

EL SALVADOR

SV

SLV

222

EQUATORIAL GUINEA

GQ

GNQ

226

ERITREA

ER_

ERI    

223

ESTONIA

EE

EST

233

ETHIOPIA

ET

ETH

231

FALKLAND ISLANDS (MALVINAS)

FK

FLK

238

FAROE ISLANDS

FO

FRO

234

FIJI

FJ

FJI

242

FINLAND

FI

FIN

246

FRANCE

FR

FRA

250

FRANCE, METROPOLITAN

FX

FXX

249

FRENCH GUIANA

GF

GUF

254

FRENCH POLYNESIA

PF

PYF

258

FRENCH SOUTHERN TER RITORIES

TF

ATF

260

GABON

GA

GAB

266

GAMBIA

GM

GMB

270

GEORGIA

GE

GEO

268

GERMANY

DE

DEU

276

GHANA

GH

GHA

288

GIBRALTAR

GI

GIB

292

GREECE

GR

GRC

300

GREENLAND

GL

GRL

304

GRENADA

GD

GRD

308

GUADELOUPE

GP

GLP

312

GUAM

GU

GUM

316

GUATEMALA

GT

GTM

320

GUINEA

GN

GIN

324

GUINEA-BISSAU

GW

GNB

624

GUYANA

GY

GUY

328

HAITI

HT

HTI

332

HEARD AND MC DONALD ISLANDS

HM

HMD

334

HOLY SEE (VATICAN CITY STATE)

VA

VAT

336

HONDURAS

HN

HND

340

HONG KONG

HK

HKG

344

HUNGARY

HU

HUN

348

ICELAND

IS

ISL

352

INDIA

IN

IND

356

INDONESIA

ID

IDN

360

IRAN (ISLAMIC REPUPLIC OF)

IR

IRN

364

IRAQ

IQ

IRQ

368

IRELAND

IE

IRL

372

ISRAEL

IL

ISR

376

ITALY

IT

ITA

380

JAMAICA

JM

JAM

388

JAPAN

JP

JPN

392

JORDAN

JO

JOR

400

KAZAKHSTAN

KZ

KAZ

398

KENYA

KE

KEN

404

KIRIBATI

KI

KIR

296

KOREA, DEMOCRATIC PEOPLE'S REPUBLIC OF

KP

PRK

408

KOREA, REPUBLIC OF

KR

KOR

410

KUWAIT

KW

KWT

414

KYRGYZSTAN

KG

KGZ

417

LAO PEOPLE'S DEMOCR ATIC REPUBLIC

LA

LAO

418

LATVIA

LV

LVA

428

LEBANON

LB

LBN

422

LESOTHO

LS

LSO

426

LIBERIA

LR

LBR

430

LIBYAN ARAB JAMAHIRIYA

LY

LBY

434

LIECHTENSTEIN

LI

LIE

438

LITHUANIA

LT

LTU

440

LUXEMBOURG

LU

LUX

442

MACAU

MO

MAC

446

MACEDONIA, THE FORMER YUGOSLAV REPUBLIC OF

MK

MKD

807

MADAGASCAR

MG

MDG

450

MALAWI

MW

MWI

454

MALAYSIA

MY

MYS

458

MALDIVES

MV

MDV

462

MALI

ML

MLI

466

MALTA

MT

MLT

470

MARSHALL ISLANDS

MH

MHL

584

MARTINIQUE

MQ

MTQ

474

MAURITANIA

MR

MRT

478

MAURITIUS

MU

MUS

480

MAYOTTE

YT

MYT

175

MEXICO

MX

MEX

484

MICRONESIA, FEDERATED STATES OF

FM

FSM

583

MOLDOVA, REPUBLIC OF

MD

MDA

498

MONACO

MC

MCO

492

MONGOLIA

MN

MNG

496

MONTSERRAT

MS

MSR

500

MOROCCO

MA

MAR

504

MOZAMBIQUE

MZ

MOZ

508

MYANMAR

MM

MMR

104

NAMIBIA

NA

NAM

516

NAURU

NR

NRU

520

NEPAL

NP

NPL

524

NETHERLANDS

NL

NLD

528

NETHERLANDS ANTILLES

AN

ANT

530

NEW CALEDONIA

NC

NCL

540

NEW ZEALAND

NZ

NZL

554

NICARAGUA

NI

NIC

558

NIGER

NE

NER

562

NIGERIA

NG

NGA

566

NIUE

NU

NIU

570

NORFOLK ISLAND

NF

NFK

574

NORTHERN MARIANA ISLANDS

MP

MNP

580

NORWAY

NO

NOR

578

OMAN

OM

OMN

512

PAKISTAN

PK

PAK

586

PALAU

PW

PLW

585

PANAMA

PA

PAN

591

PAPUA NEW GUINEA

PG

PNG

598

PARAGUAY

PY

PRY

600

PERU

PE

PER

604

PHILIPPINES

PH

PHL

608

PITCAIRN

PN

PCN

612

POLAND

PL

POL

616

PORTUGAL

PT

PRT

620

PUERTO RICO

PR

PRI

630

QATAR

QA

QAT

634

REUNION

RE

REU

638

ROMANIA

RO

ROM

642

RUSSIAN FEDERATION

RU

RUS

643

RWANDA

RW

RWA

646

SAINT KITTS AND NEVIS

KN

KNA

659

SAINT LUCIA

LC

LCA

662

SAINT VINCENT AND THE GRENADINES

VC

VCT

670

SAMOA

WS

WSM

882

SAN MARINO

SM

SMR

674

SAO TOME AND PRINCIPE

ST

STP

678

SAUDI ARABIA

SA

SAU

682

SENEGAL

SN

SEN

686

SEYCHELLES

SC

SYC

690

SIERRA LEONE

SL

SLE

694

SINGAPORE

SG

SGP

702

SLOVAKIA (Slovak Republic)

SK

SVK

703

SLOVENIA

SI

SVN

705

SOLOMON ISLANDS

SB

SLB

90

SOMALIA

SO

SOM

706

SOUTH AFRICA

ZA

ZAF

710

SOUTH GEORGIA AND THE SOUTH SANDWICH ISLANDS

GS

SGS

239

SPAIN

ES

ESP

724

SRI LANKA

LK

LKA

144

ST. HELENA

SH

SHN

654

ST. PIERRE AND MIQUELON

PM

SPM

666

SUDAN

SD

SDN

736

SURINAME

SR

SUR

740

SVALBARD AND JAN MAYEN ISLANDS

SJ

SJM

744

SWAZILAND

SZ

SWZ

748

SWEDEN

SE

SWE

752

SWITZERLAND

CH

CHE

756

SYRIAN ARAB REPUBLC I

SY

SYR

760

TAIWAN, PROVINCE OF CHINA

TW

TWN

158

TAJIKISTAN

TJ

TJK

762

TANZANIA, UNITED REPUBLIC OF

TZ

TZA

834

THAILAND

TH

THA

764

TOGO

TG

TGO

768

TOKELAU

TK

TKL

772

TONGA

TO

TON

776

TRINIDAD AND TOBAGO

TT

TTO

780

TUNISIA

TN

TUN

788

TURKEY

TR

TUR

792

TURKMENISTAN

TM

TKM

795

TURKS AND CAICOS ISLANDS

TC

TCA

796

TUVALU

TV

TUV

798

UGANDA

UG

UGA

800

UKRAINE

UA

UKR

804

UNITED ARAB EMIRATES

AE

ARE

784

UNITED KINGDOM

GB

GBR

826

UNITED STATES

US

USA

840

UNITED STATES MINOR OUTLYING ISLANDS

UM

UMI

581

URUGUAY

UY

URY

858

UZBEKISTAN

UZ

UZB

860

VANUATU

VU

VUT

548

VENEZUELA

VE

VEN

862

VIET NAM

VN

VNM

704

VIRGIN ISLANDS (BRITISH)

VG

VGB

92

VIRGIN ISLANDS (U.S)

VI

VIR

850

WALLIS AND FUTUNA ISLANDS

WF

WLF

876

WESTERN SAHARA

EH

ESH

732

YEMEN

YE

YEM

887

YUGOSLAVIA

YU

YUG

891

ZAIRE

ZR

ZAR

180

ZAMBIA

ZM

ZMB

894

ZIMBABWE

ZW

ZWE

716


Additional notes on the ISO-3166 Country Codes

 

The fifth edition will consist of three parts:

1.  3166-1 country codes / DIS published April 96 / IS expected summer|fall 97  "The list of country names remains basically unchanged."

2.  3166-2 country subdivision code / DIS published November 1996

3.  3166-3 Code for formerly used names of countries / DIS expected spring 97

 

Quote: “We are delighted to notice that the acceptance of ISO3166 among users of country codes is growing.  However, the use of ISO3166 e.g. in the Internet confronts ISO3166/MA with formerly unknown problems.  One among these problems is that more and more "non-country-entities" as e.g. organisations, interest groups or groupings of countries request ISO3166 code elements.  The scope of the standard does not allow for allocation of code elements to such "groups".

 


Appendix D   WOUDC Security protocol documents

 

 

World Ozone and Ultraviolet Data Centre (WOUDC) Data Users' Protocol

 

Introduction

 

The World Ozone and Ultraviolet Radiation Data Centre (WOUDC) provides data sets to the scientific and educational communities free of charge.  The WOUDC is one of several World Data Centres (WDC) operating under the auspices of the World Meteorological Organization - Global Atmosphere Watch (WMO-GAW).

 

Resolution 40 (Cg-XII) of the Twelfth World Meteorological Congress of the WMO states that data and products within the WMO networks be made available "... on a free and unrestricted basis." [1] to the scientific and education community.  However, depending on the needs and wishes of the data originators, the WOUDC will post data so that access is restricted for an agreed limited duration (up to 2 years), after which, the restriction would be removed and the data would be made available through general access.

 

The conditions that a user must agree to before being allowed access to WOUDC "restricted" data are the subject of this document.

 

Access to WOUDC "restricted" data will be made available by means of a special ftp account upon receipt of this signed users protocol by the party(ies) wishing to use the data.

 

The WOUDC data archive contains the following data sets which are freely accessible:

 

1. Total column ozone

2. Ozonesonde profiles

3. Umkehr retrievals

4. Lidar profiles   

5. Surface ozone data

6. Ultraviolet radiation data

 

Data sets that require a signed copy of this protocol include Level 0 (primary or "raw" data), processed data (Level 1) awaiting publication by the data originator or data products that are used as input data for Level 2 output generated by the WOUDC in a standard grid or an accepted algorithm.  An example of the latter is the Umkehr retrievals which use a standard algorithm.

 

(The WOUDC deals primarily with Level 1 processed data. However, Level 1 Umkehr data are used as input into a standard algorithm to produce Level 2 retrievals.  The Level 1 Umkehr are not available unless this protocol is signed.

 

Any further inquiries may be directed to the WOUDC by:

 

Phone: 1-416-739-4635

Fax:   1-416-739-4281

Email: woudc@ec.gc.ca

 

References

 

[1]        World Meteorological Organization, Twelfth World Meteorological Congress, Abridged Final report with Resolutions, WMO-No.827, Resolution 40, Secretariat of the WMO, Geneva, Switzerland, 30-May-21 June, 1995.

 

- Original WOUDC document created September 27, 1995. Revised October 1997.

Terms and Agreements of the Data Users Protocol

 

 

Completion of this form is required for access to the WOUDC "restricted" data sets which are not publicly available.  Before submitting it, ensure that you have read the wodc/readme.wodc, wudc/readme.wudc and secure.txt documentation files.

 

In signing this form the data user(s) agrees to all elements of both the Security and Data Use sections.

 

 

Security

 

Þ  She/He will use the user identifier for their own personal use and will not make it available to another person.

 

Þ  She/He will keep the password known only to herself/himself.

 

Þ  She/He will inform the WOUDC administrators if it is suspected that someone else has logged into the WOUDC system using her/his identifier.

 

 

Data Use

 

¨    The ownership of every data file is as specified by the WOUDC.

 

¨    All WOUDC registered users have equal and complete access to the restricted data.

 

¨    Originators of data endeavour to notify the WOUDC as soon as possible of data which is considered suspect and to submit revised and/or corrected data.

 

¨    Any kind of publication scientific or otherwise must have the written consent of the originator.

 

¨    For data younger than one year joint authorship must be offered.

 

¨    Any originator/owner of some WOUDC data has the right to refuse the use of

his/her data in any publication by someone else.

 

¨    Data are to be used for scientific and/or educational purposes.

 

¨    The user will abide by any special stipulations that might be posted by WOUDC with the data to which they apply.

 

 

 

 

 

Signature:___________________________________   Date: __________________________________


 

WOUDC "Restricted" Access Data Archive User Registration Form

 

 

 

Last Name: _________________________ Given Name(s): _______________________________

 

 

Institute: ________________________________________________________________________

 

 

Address:___________________________________________

 

               ___________________________________________

 

               ___________________________________________

 

 

Telephone: _________________________________   Fax: _______________________________

 

 

E-mail address: __________________________________________________________________

 

 


World Ozone and Ultraviolet Data Centre (WOUDC) Data Submission Agreement

 

 

Introduction

 

The World Ozone and Ultraviolet Radiation Data Centre (WOUDC) provides data sets to the scientific and educational communities free of charge.  The WOUDC is one of several World Data Centres (WDC) operating under the auspices of the World Meteorological Organization - Global Atmosphere Watch (WMO-GAW).

 

Resolution 40 (Cg-XII) of the Twelfth World Meteorological Congress of the WMO states that data and products within the WMO networks be made available "... on a free and unrestricted basis." [1] to the scientific and education community.  However, depending on the needs and wishes of the data originators, the WOUDC will post data so that access is restricted for an agreed limited duration (up to 2 years), after which, the restriction would be removed and the data would be made available through general access.

 

This agreement outlines the terms to be established between the WOUDC and the data originator(s) with respect to the limited or "restricted" access to the submitted data.

 

 

WOUDC data designated as "restricted" will be made available by means of a special restricted access ftp account to only those individuals who submit a signed copy of the WOUDC data users protocol (protocol.txt).

 

 

Any further inquiries may be directed to the WOUDC by:

 

Phone: 1-416-739-4635

Fax:   1-416-739-4281

Email: woudc@ec.gc.ca

 

 

References

 

[1] World Meteorological Organization, Twelfth World Meteorological Congress, Abridged Final report with Resolutions, WMO-No.827, Resolution 40, Secretariat of the WMO, Geneva, Switzerland, 30-May-21 June, 1995.

 

 

- World Ozone and Ultraviolet Radiation Data Centre, Toronto, CANADA

 

  October 1997

 


Terms of the Data Submission Agreement

 

The WUDC expects to receive Level 0 primary or "raw" data, Level 1 quality assured processed data and in some instances, Level 2 data which are gridded to standard parameters based on accepted algorithms.

 

For the purposes of data distribution, the data originator(s) is required to indicate the option of choice for the release of his/her data.

 

NOTE: "General Distribution" requires a generic username/password to access the WOUDC data archive.  However, no data usage agreements are specified or required in order to obtain access.

 

 

Data Distribution Options

 

Indicate only one.

 

Level 0 - Primary or "Raw" Data

 

Option

Condition(s)

 

 

__ 1.

Data will be archived only. No distribution.

 

 

__ 2.

Restricted distribution for __ months (up to 24 months), after which, the restriction would be removed and the data would be made available through general access.

 

 

__ 3.

Unrestricted access, with general distribution.

 

 

Level 1 - Processed Data

 

Option

Conditions(s)

 

 

__ 4.

Restricted distribution for __ months (up to 24 months),after which, the restriction would be removed and the data would be made available through general access.

 

 

__ 5.

Unrestricted access, with general distribution.

 

 

Special Data Processing Agreement

 

A data originator may choose to allow the staff at the WOUDC to process Level 0 data using standard data processing procedures and algorithms, specifically developed for the output and distribution of Level 1 data, by the WOUDC.

 

Option

Conditions(s)

 

 

__ 6.

Restricted distribution for ___ months (up to 24 months),after which, the restriction would be removed and the data would be made available through general access.

 

 

__ 7.

Unrestricted access, with general distribution.

Level 2 - Gridded Data

 

Should a data originator decide to submit Level 2 gridded data then he/she is encouraged to contact the WUDC to discuss the terms of a data submission and distribution agreement.

 

 

INSTRUCTIONS

 

Complete the data originator(s) information (please print) and sign below.  Then forward the entire document by fax to:

 

The World Ozone and Ultraviolet Radiation Data Centre (WOUDC)  Fax: +1-416-739-4635

 

 

 

Last Name: _________________________ Given Name(s): ________________________________

 

 

Institute: _________________________________________________________________________

 

 

Address:   _______________________________________

 

                 _______________________________________

 

                 _______________________________________

 

 

Telephone: __________________________________   Fax: _______________________________

 

 

E-mail address: ___________________________________________________________________

 

 

 

 

I hereby acknowledge and consent to the above indicated option and conditions.

 

 

 

 

 

Signature: ___________________________________   Date: ______________________________

 


SECURE.TXT

 

The WOUDC data output is normally freely available for public use and all files are write protected with read only access. There are special circumstances, however, which require a single user or group of users to have the ability to freely exchange data at a level of security which permits both read and write access to that specified group.

 

In response to this need for a higher level of security, special "secure" directories and user access through a specified username/password will be made available to interested individuals or groups. The general procedure to access these new directories by means of the Internet file transfer protocol (ftp) will remain the same, just the username and password will be different. Files and documentation may then be freely exchanged within this second level and be protected from "public" viewing.

 

The submission of data either to the "secure" or public directories is acceptable, the latter being preferred. Originators should note that users of public data are advised by the WOUDC to abide at all times by whatever stipulations the originator has written in the sponsorship file. Refer to the readme.wudc file for further details of the sponsorship file format.  Data originators may choose the level of security and access by indicating the option and signing the OPTIONS.TXT form.

 

To get special directory access, the data client will have to complete the information and sign that the security and protocol undertaking in PROTOCOL.TXT will be accepted. After mailing the signed PROTOCOL.TXT form to the WOUDC the data client (user) can contact woudc@ec.gc.ca to obtain a password.

 

 

 

Although  believing strongly that the merits of fast universal distribution of data far outweigh any advantage in not distributing data, the  WODC respects the positions of individual data originators and agencies and has attempted to accommodate them as recommended by the WMO Scientific Advisory Group on UV Radiation in May, 1995.

 

 

 


Appendix E         WUDC Data Flags

 

 

For the spectral UV irradiance data properties associated with the six flags are as follows:

 

1.     The irradiance  at  324nm which is  not  significantly  affected by ozone and which is compared with the "clear-sky"  value  for  the  same solar elevation.   In  this context,  the "clear-sky" value is defined as the  95th   percentile of all measurements except those  made  when there was snow on the ground.  (The actual value is not very  sensitive  to  the  percentile  level,  the  99th  percentile being ~1.08 of the adopted value.).

2.     An estimate of total ozone derived from the  spectrum  and solar elevation (Ref. ).

3.     The standard error in the total ozone estimate (Ref. ).

4.     An estimate of sulfur dioxide from the spectrum  (Ref.).

5.     The ratio of irradiances at individual wavelengths to those in an average UV spectrum for the given solar zenith angle and derived ozone amount.

6.     The difference between the raw spectra  recorded  with increasing and decreasing wavelength. (Each spectrum in  the processed Version 1 and 2 data is the average of an upward and a downward scan.)

Reference: Fioletov, V.E., J.B. Kerr and D.I. Wardle, The relationship between total ozone and spectral UV irradiance from Brewer spectrophotometer observations and its use for derivation of total ozone from UV measurements, Geophys. Res. Lett., 24, 2997-3000, 1997.

The  formal criteria are shown in Table  AD.1.

Table AD.1. The formal criteria used for error flag determination.

 

Digit

Code

Criterion

Comment

1

1

UV324 is either less than the 5th percentile (i.e. <13% of “clear sky” conditions) or 1.5 times higher than “clear sky” conditions

Rare but possible cases: low UV324 indicates heavy clouds. High UV324 can be related to clear sky and fresh snow.

 

2

UV324 is either less than the 1st percentile (i.e. <6% of clear sky conditions) or 2 times higher than “clear sky” conditions

Low UV324 indicate very heavy clouds, rain, or snow. Very high UV324 can be observed in high latitudes at low sun conditions.

 

3

UV324 is either at least 10 times less than the 1st percentile (<0.6% of clear sky conditions) or 2.5 times higher than “clear sky” conditions

It is still possible to observe these low UV324 in the case of a very heavy rain. Otherwise it may be caused by snow covering the instrument.


2

1

Total ozone derived from UV is less than 210 DU or more than 550 DU with small errors

Rare but possible total ozone amounts.

 

2

Total ozone derived from UV is less than 150 DU or more than 650 DU with high errors

Very rare total ozone amounts. High errors may indicate variable cloud conditions during the measurements

 

3

Total ozone derived from UV is less than 100 DU or more than 750 DU

Unusual total ozone may be an indicator of variable cloud conditions. For example, O3 will be low if clouds covered the Sun only during the measurements of UV at 320-325 nm, i.e. in the middle of the measurement cycle. Very high ozone can also be observed with heavy clouds

3

1

The error in total ozone retrieved from the spectrum is above the 99th percentile of all such errors at the given solar elevation

Indicates variable conditions during the measurement

 

2

The error in total ozone retrieval is twice that specified for Code 1

Indicates highly variable conditions during the measurement

 

3

The error in total ozone retrieval is six times that specified for Code 1

Very high variations of the conditions during the measurement, the data probably cannot be used for O3 or SO2 estimations

4

1

SO2 derived from UV is 5-10 DU

Traces of SO2.

 

2

SO2 derived from UV is 10-20 DU

SO2 component is seen in UV spectrum

 

3

SO2 derived from UV is more than  20 DU

High total amount of SO2. (It has to be accounted for when ozone - UV relationship is studied).

 

5

1

At  1 or 2 wavelengths the irradiance is outside  the +/-6 sigma envelope

Can be a random error. The appearance of that code in a large number of spectra may indicate, a wavelength shift.

 

2

As for Code 1 but at 3 or 4 wavelengths

Indicates variable conditions during the measurement or an wavelength shift

 

3

As for Code 1 but at 5 or more wavelengths

Indicates highly variable conditions during the measurement. Total ozone and SO2 probably cannot be estimated correctly

 

6

1

At  1 or 2 wavelengths the ratio between the irradiance measurements on the upward and downward scans exceeds the factor 2.

Another criterion that indicates variable conditions during the measurement.  Applies to Brewer type double scans.

 

2

As for Code 1 but at 3 or 4 wavelengths

 

 

3

As for Code 1 but at 5 or more wavelengths

Indicates highly variable conditions during the measurement. Total ozone and SO2 probably cannot be estimated correctly. The data may be useful only for calculation of integrated UV characteristics.

 

Appendix F         List of Acronyms

 

 

Acronym

Name

 

 

AES

Atmospheric Environment Service of Environment Canada

ACGIH

American Conference of Governmental Industrial Hygienists

ASCII

American Standard Code for Information Interchange

BDMS

Brewer Data Management System

CIE

Commission Internationale de L’Eclairage (Int’l Com. of Illumination)

CSV

Comma Separated Value

extCSV

extended Comma Separated Value

FTP

File Transfer Protocol

FWHM

Full Width at Half Maximum

ISO

International Organization for Standardization

JMA

Japanese Meteorological Agency

NASA

National Aeronautical and Space Administration (USA)

NDSC

Network for Detection of Stratospheric Change

NIOSH

National Institute of Occupational Safety and Health

NIST

National Institute of Standards and Technology (USA)

NSF

National Science Foundation (USA)

PAR

Photosynthetically Active Radiation

SAG_UV

WMO/GAW Scientific Advisory Group on Ultraviolet radiation

(formerly the Scientific Steering Committee on Ultraviolet radiation or SSC_UV)

SSS

Scientific Sponsorship Statement

TOMS

Total Ozone Mapping Spectrometer

UTC

Coordinated Universal Time

WMO/GAW

World Meteorological Organization - Global Atmosphere Watch

WOUDC

World Ozone and Ultraviolet Radiation Data Centre

WODC

World Ozone Data Centre

WUDC

World Ultraviolet Radiation Data Centre

 

 

 


Appendix G        List of Defined Instrument Types and Names

 

 

Manufacturer

Actual Name

Category

Defined Name

Model(s)

 

 

 

 

 

Bentham Instruments Ltd.

Bentham monochromator

Spectral

Bentham

DM-150, DM-300

 

 

 

 

 

Biospherical Instruments Inc.

Ground-based Scanning UV Spectroradiometer

Spectral

Biospherical

SUV-100, SUV-150

 

Ground-based UV Radiometer

Multi-band

Biospherical

GUV-511, GUV-541

 

Profiling UV Radiometer

Multi-band

Biospherical

PUV-500B, PUV-510

 

 

 

 

 

Eko Instruments Trading Co. Ltd.

Eko Pyranometer

Pyranometer

Eko

SBP-801, NP-62,

MS-42

 

Eko UV-B Pyranometer

Broad-band

Eko

MS-210W

 

 

 

 

 

Eppley Laboratory, Inc.

Precision Spectral pyranometer

Pyranometer

Eppley

PSP

 

Black and White pyranometer

Pyranometer

Eppley

8-48

 

Total Ultrviolet radiometer

Broad-band

Eppley

TUVR

 

 

 

 

 

Geminali, A.S.

UV-Irradiance meter

Multi-band

NILU

NILU-UV

 

 

 

 

 

Middleton

Middleton EP07

Pyranometer

Middleton

EP07

 

 

 

 

 

Optronics Laboratoies, Inc.

Optronics Spectroradiometer

Spectral

Optronics

OL742, OL750, OL752, OL754

 

 

 

 

 

Scintec Atmospharen messtechnik GMBH

Scintec UV-S

Broad-band

Scintec

UV-S-290-T

 

 

 

 

 

Sci-Tec/Kipp and Zonen Instruments Ltd.

Pyranometer (Visible Radiation)

Pyranometer

Kipp and Zonen

CM3, CM5, CM6/6B, CM10/11, CM21, CM31

 

Narrowband Scientific UV Radiometer (Global)

Broad-band

Kipp and Zonen

CUVA1, CUVB1

 

Narrowband Scientific UV Radiometer (Direct)

Broad-band

Kipp and Zonen

CUVA2, CUVB2

 

Broadband UV Radiometer

Pyranometer

Kipp and Zonen

CUV3

 

 

 

 

 

Sci-Tec Instruments Ltd.

Brewer spectrophotometer

Spectral

Brewer

MKII, MKIII and MKIV

 

 

 

 

 

Schenk

Schenk Star

Pyranometer

Schenk

Star

 

 

 

 

 

Solar Light Co. Inc.

UV-Biometer

Broad-band

UV-Biometer

500, 501, 501A

 

 

 

 

 

Swissteco

Swissteco SS25

Pyranometer

Swissteco

SS25

 

 

 

 

 

Vaisala

Vaisala pyranometer

Pyranometer

Vaisala

CM6B, CM11

 

 

 

 

 

Vital Technologies Corporation

Vital BW series

Broad-band

Vital

BW-20, BW100

 

 

 

 

 

Yankee Environmental Systems, Inc.

Yankee Ultraviolet Sun Photometer

Multi-band

Yankee

SPUV-6, SPUV-10

 

Yankee Ultraviolet Multi-filter radiometer

Multi-band

Yankee

UVMFR-7

 

Yankee UV Multifilter Rotating Shadow Band Radiometer

Multi-band

Yankee

UVMFR-1

 

Yankee Multifilter Rotating Shadow Band Radiometer

Multi-band

Yankee

MFRSR-1

 

Yankee Ultraviolet Pyranometer

Broad-band

Yankee

UVB-1

 

Yankee Total Solar Pyranometer

Pyranometer

Yankee

TSP-100, 400,700

 

 

 

 

 

 

 

**The WOUDC will continue to update this table.  Refer to the WOUDC web site for a current listing.



* Atmospheric Environment Service, Toronto, Canada

++ Ph.D. Associates Incorporated, Toronto, Canada