Retrieving the solar EUV spectrum from a reduced set of spectral lines
The solar EUV irradiance is a key input for thermospheric and ionospheric models. Difficulties in continuously measuring the calibrated spectrum has prompted the use of various surrogate quantities. Although most proxies correlate quite well with the spectral variability, their use for modelling...
Main Authors: | T. D. de Wit, J. Lilensten, J. Aboudarham, P.-O. Amblard, M. Kretzschmar |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2005-11-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/23/3055/2005/angeo-23-3055-2005.pdf |
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