File:Krauss fig1.jpg

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Revision as of 13:53, 18 January 2016 by ManuelaTemmer (Talk | contribs)
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current13:54, 18 January 2016Thumbnail for version as of 13:54, 18 January 2016691×536 (63 KB)ManuelaTemmer (Talk | contribs) (Illustration of the thermospheric temperature response to high solar/stellar EUV flux. Enhanced ionization (IN) and photochemical processes like photo-dissociation (PD) and dissociative recombination (DR) eventually lead to heating and subsequent expansio)
13:53, 18 January 2016Thumbnail for version as of 13:53, 18 January 2016691×536 (63 KB)ManuelaTemmer (Talk | contribs)

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