Guide to the WMO/GAW
World Ultraviolet
Radiation Data Centre
Version 5.1

Atmospheric Environment Service
Environment Canada
1998
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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)
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.......................................
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.
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.
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.
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.
The guide is currently on its fifth version issued in April, 1998.
·
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).
·
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).
·
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).
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.
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.
·
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.
·
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.
·
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.
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.
·
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.
·
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.
·
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.
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.
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.
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 |
|
|
|
|
|
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.
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. |
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.
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: |
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.
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 |
|
||
|
|
|
|
||
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
…
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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
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.
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.
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.
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.
[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.
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
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 |
|
|
|
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".
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. |
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. |
|
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 |
|
|
|
|
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.