Can the EUV spectrum and its variability be reconstructed from a small set of spectral lines ?

Thierry Dudok de Wit (1) , Jean Lilensten (2) , J. Aboudarham (3) , Pierre-Olivier Amblard (4) , F. Auchère (5) , Matthieu Kretzschmar (6)

1 LPCE - Laboratoire de physique et chimie de l'environnement
2 LPG - Laboratoire de Planétologie de Grenoble
3 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
4 LIS - Laboratoire des images et des signaux
5 IAS - Institut d'astrophysique spatiale
6 ROB - Royal Observatory of Belgium [Brussels]

The severe lack of continuously measured and spectrally resolved solar EUV spectra is a major obstacle towards modelling the impact of the solar irradiance on the ionosphere The usual solution involves the measurement of various proxies We consider a different approach in which the EUV spectrum and its variability are reconstructed from the linear combination of a few spectral lines Using three years of spectra from TIMED and a statistical classification technique we demonstrate that 5 to 8 lines only are needed and in addition show which lines are the best candidates These results are valuable for instrument specification and also provide new insight into the comparison of solar proxies against the EUV irradiance

Thierry Dudok de Wit, Jean Lilensten, J. Aboudarham, Pierre-Olivier Amblard, F. Auchère, et al.. Can the EUV spectrum and its variability be reconstructed from a small set of spectral lines ?. 36th COSPAR Scientific Assembly, 2006, Beijing, China. ⟨insu-00358865⟩