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Solar EUV/FUV irradiance variations: analysis and observational strategy

Wybrane pełne teksty z tego czasopisma
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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The knowledge of solar extreme and far ultraviolet (EUV) irradiance variations is essential for the characterization of the Earth’s upper atmosphere. For a long time, this knowledge has been based on empirical models, which are themselves based on proxies of the solar activity. However, the accurate modeling and prediction of the Earth’s upper atmosphere necessitate to improve the precision on the irradiance and its variations below about 200 nm. Here, we present a review of recent works made by the authors that aim at quantifying the irradiance variability at these wavelengths, and that lead to new way of monitoring the solar EUV/FUV irradiance spectrum. In more details, it is shown that the quantification of the high level of redundancy in the solar spectrum variability allows to envisage measuring only a small portion of the spectrum without losing essential knowledge. Finally, we discuss what should and could be measured in order to retrieve the solar extreme and far ultraviolet spectrum.
Słowa kluczowe
Czasopismo
Rocznik
Strony
42--51
Opis fizyczny
Bibliogr. 19 poz.
Twórcy
Bibliografia
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  • Dudok de Wit, T., M. Kretzschmar, J. Aboudarham, P.-O. Amblard, F. Auchere, and . Lilensten (2008), Which solar EUV indices are best for reconstructing the olar EUV irradiance?, Adv. Space Res. 42, 5, 903-911,
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  • Lilensten, J., T. Dudok de Wit, P.-O. Amblard, J. Aboudarham, F. Auchere, and M. Kretzschmar (2007), Recommendation for a set of solar EUV lines to be monitored for aeronomy applications, Ann. Geophys. 25, 6, 1299-1310.
  • Lilensten, J., T. Dudok de Wit, M. Kretzschmar, P.-O. Amblard, S. Moussaoui,J. Aboudarham, and F. Auchere (2008), Review on the solar variability spectrum for space weather purposes, Ann. Geophys. 26, 269-279.
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-BSL8-0025-0023
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