• Aucun résultat trouvé

DETERMINATION OF STANDARDS FOR AN UV MONITORING NETWORK

N/A
N/A
Protected

Academic year: 2021

Partager "DETERMINATION OF STANDARDS FOR AN UV MONITORING NETWORK "

Copied!
3
0
0

Texte intégral

(1)

IGAC

DETERMINATION OF STANDARDS FOR AN UV MONITORING NETWORK

Project leader: Dr. Didier GILWTAY, lnstitut d'Aeronomie Spatiale de Belgique, 3, Avenue Circulaire, B-1180 Bruxelles, Tel: +322373.03.50 - Fax: +32 2 374.84.23 - E-mail: (Bitnet) dgill@aero.oma.be

Participants: Prof. Paul C. SIMON, Mr. William PEETERMANS, Mr. David BOLSEE, lnstitut d'Ael'onomie Spatiale de Belgique, 3, Avenue Circulaire, B-1 180 Bruxelles, Belgique, Tel : +322375.15.79 - Fax: +322374.84.23 - E-mail: (Bitnet) pauls@aero.oma.be

[n collaboration with:

Dr. Ann R. WEBB (coordinator), University of Reading, United Kingdom Dr. Mario BLUMTHALER, University of Innsbruck, Austria

Dr. Inge DIRMHIRN, University of Agriculture, Vienna, Austria

Prof. Jacqueline LENOBLE, Universite des Sciences et Techniques de Lille-Flandres- Artois, France

Dr. Gunther SECKMEYER, Fraunhofer Institute, Garmisch-Partenkirchen, Germany Dr. Jtirgen ROS, University of Karlsruhe, Germany

Dr. Brian G. GARDINER, Natural Environment Research Council, United Kingdom Prof. Christ os S. ZEREFOS, Aristotelian University of Thessaloniki, Greece

Dr. Henk REINEN, National Insitute for Public Health, The Netherlands Dr. Foeke KUIK, Royal Netherlands Meteorological Institute, The Netherlands Dr. Trond SVEN0E, University of Troms0, Norway

Natural and anthropogenic changes of the stratosphere have two important consequences on the biosphere. First, stratospheric ozone is the major absorber of UV-B radiation (280-320 nm) in the Earth's atmosphere and it is known to have damaging effects on biological systems. Processes, either natural or anthropogenic, that cause decreases in stratospheric ozone and therefore cause increases of UV-B radiation are of great concern. Second, biospheric processes are known to affect the concentrations of radiatively active trace gases in the atmosphere. Therefore, consideration must be given to the possibility of indirect effects of the stratosphere on climate that might result from UV-B-produced biospheric effects that could modulate the flux of greenhouse gases into the atmosphere.

The overall objective of this project is to produce practical recommen- dations for the deployment of an integrated UV-B network throughout Europe.

The recommendations will be based on comparison of different methods of

\04

(2)

measurement both between and within instrument categories. Three 'European Intercomparison Campaign of UV Spectrometers' were carried out since July 1991 in different European countries. Suitability of instruments and the criteria for a network will be judged by their ability to meet the requirements of the data users : atmospheric modellers, photobiologists, photochemists, ...

Recommendations will also be produced for the absolute calibration and the maintenance procedures of the instruments involved in the future network.

In achieving this major aim two other independent objectives need to be met to allow a network based on a number of different instruments. One is the development of a transportable calibration system that can be used for all instruments. The 'Transportable Lamp System' (TLS) has been designed and developed by IASB to meet this goal. The TLS, which is for the moment used as a relative reference, is presently in a final development and evaluation phase. The second is a computational means of normalising the results from instruments with different optical geometry.

A side product of the project will be a data base of UV-B measurements made throughout Europe during the duration of the project. In this field, IASB has build a full automatic U V -B monitoring station which is operational since March 1993, providing UV-B and UV-A measurements every 15 minutes for solar zenith angles lower than 100. While not a unified network, the investigation of measurement techniques and instruments in the project will

UV-B INTEGRATED IRRADIANCE in UCCLE from 1/1 to 31/12/1993

r::i' 4

<

Ei 3.5

Julian day 1 --> 365

~ '--'

U.l 3

U

~

2.5

- ~

c.:::

c.::: 2

-

Cl

U.l 1.5

~ c.:::

d U.l 1 E-<

~ 0.5

CO

>-

:J 0

0 50

DAY OF THE YEAR

Fig. I. - UV-B Climatology in Uccle during 1993.

105

(3)

UV-B INTEGRATED IRRADIANCE in UCCLE from 1/1 to 31/12/1994 N

<

8

4, , - - - ---, - - -- -- -, - - - - -- - - , - --- , - -- -- - - ,- ---, -- -- -- -, - - -,

~ '-"

fJ.l U

~

~ ~

Cl fJ.l

~ 0:::

~

r::o

>-

~

3.5 3 2.5

2 1.5

0.5

o

0 50

Julian day 1 --> 365

100 150 200 250 300 350

DAY OF THE YEAR

Fig. 2. - UV-B Climatology in Uccle during 1994.

provide compatibility limits between different locations, and allow data from other networks to be used with an acknowledged degree of uncertainty in absolute spectral measurements. The other networks can also provide infor- mation on the level of various atmospheric constituents which together with the measured UV-B irradiances should aid the understanding of UV radiative transfer.

References

Gardiner B.G., Webb A.R., Bais A.F., Blumthaler M., Dirmhirn 1., Foster P., Gillotay D., Henrilsen K., Huber M., Kirsch P.l., Simon P.c., Sven0e T., Weihs P. and Zerefos C.S. 1993. European lntercomparison of ultraviolet spectro-radiometers.

Environ. Techno!. 14: 25-43.

106

Références

Documents relatifs

However, (B 2 BN ) and Benes networks can permute more than one frame in parallel having different length and different circular-shift rotation. In [13] the authors propose to prune

For instance, the authors in [18] suggested a high throughput 5G LDPC encoder based on a Barrel Shifter, but without the capability to deal with different frame lengths and

While not a unified network, the investigation of measurement techniques and instruments in the project will provide compatibility limits between different locations,

If we do not have the surface vessels, we can calculate the Relative Localization (i.e., the configuration of the swarm) by solving the distance equations, and create a constellation

Ozone Monitoring Instrument (OMI) is a nadirview- ing spectrometer designed to monitor ozone and other atmo- spheric species (Levelt et al., 2006). The OMI surface UV algo- rithm

With this symbolic-numeric implemen- tation we can compute the exact absolute factorization of a bivariate polynomial with total degree 200 having 10 absolute irreducible factors

Health organizalions should alsobeaware thatdifferenl genres of music may have differenl potcntials for use in aneducalional

In the perspective of reusing EHR data to automate the monitoring of medical devices, we carried out a comparison of the main MD knowledge bases (MD-KDB) currently available