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Spectral Bands from Measurements Carried out during ATLAS-1 and E U R E C A - 1

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Irradiance Observations in Near-UV, Visible and Near Infrared

Spectral Bands from Measurements Carried out during ATLAS-1 and E U R E C A - 1

Missions

B y G E R A R D T H U I L L I E R1, M I C H E L H E R S E1, D I E T R I C H L A B S2, P A U L C. S I M O N3, D I D I E R G I L L O T A Y3 AND H O L G E R M A N D E L2

Service d'Aeronomie du CNRS, BP3, F91371 Verrieres le Buisson, France

2Landessternwarte, Konigstul, D-69117 Heidelberg 1, Germany

3Institut d'Aeronomie Spatiale de Belgique, 3 avenue Circulaire B-1180 Bruxelles, Belgium

1. Introduction

For the ATLAS and EURECA missions, we have used two identical instruments to measure the absolute solar spectral irradiance from 180 to 3200 nm. These instruments are calibrated by use of a blackbody and a set of lamp standards. The measurements are carried out with 1 nm bandpass up to 800 nm and 20 nm above. The instruments and calibration procedures are described by Thuillier et al. (1981). The platform capability of instruments retrieval after measurements allows a post-flight calibration which is essential for accurate measurements. The main results obtained up to now are:

- In the UV, the ATLAS-1 and EURECA-1 solar spectral irradiance are consistent with the SpaceLab 1 data obtained in 1983 (Labs et al. 1987). Figure 1 shows the ATLAS 1 and SL 1 spectra. The origin of the existing differences is presently under investigation.

- In the visible domain, our measurements agree with the solar spectrum from Neckel

& Labs (1984) within a few percent difference at certain wavelength.

- In the IR domain, the preliminary processing shows a spectrum close to the one obtained by Thekaekara (1974).

This instrument calibrated against the same standard and operated in space has mea- sured the solar irradiance spectrum from 200 to 3000 nm. This instrument has partici- pated in the ATLAS 2 mission and will continue to monitor the solar spectral irradiance as a function of time.

REFERENCES

LABS, D., NECKEL, H., SIMON, P. & THUILLIER, G. 1987 Ultraviolet solar irradiance measurement from 200 to 358 nm during the SpaceLab 1 mission. Solar Phys. 107, 203-219.

NECKEL, H. & LABS, D. 1984 The solar radiation between 3300 and 12500 A. Solar Phys.

90, 205-258.

THEKAEKARA, M. P. 1974 Extraterrestrial solar spectrum, 3000-6100 A at 1 A intervals Appl. Opt. 13, 518-521.

THUILLIER, G., SIMON, P.C., LABS, D., PASTIELS, R. & NECKEL, H. 1981 An instrument to measure the solar spectrum from 170 to 3200 nm. Solar Phys. 74, 531-537.

70

available at https:/www.cambridge.org/core/terms. https://doi.org/10.1017/S0252921100024556

Downloaded from https:/www.cambridge.org/core. Konin Meteor Instit, on 31 May 2017 at 09:59:25, subject to the Cambridge Core terms of use,

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G. Thuillier et al.: Near-UV, Visible, and Near-IR Irradiance Observations 71

(L-uju-2-LU*MUJ)33NViavyyi

FIGURE 1. UV Solar irradiance from ATLASl mission.

available at https:/www.cambridge.org/core/terms. https://doi.org/10.1017/S0252921100024556

Downloaded from https:/www.cambridge.org/core. Konin Meteor Instit, on 31 May 2017 at 09:59:25, subject to the Cambridge Core terms of use,

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