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...

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Bibliographic Details
Main Authors: T. D. de Wit, J. Lilensten, J. Aboudarham, P.-O. Amblard, M. Kretzschmar
Format: Article
Language:English
Published: Copernicus Publications 2005-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/23/3055/2005/angeo-23-3055-2005.pdf