File:Krauss fig1.jpg
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Revision as of 13:53, 18 January 2016 by ManuelaTemmer (Talk | contribs)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 13:54, 18 January 2016 | 691×536 (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 2016 | 691×536 (63 KB) | ManuelaTemmer (Talk | contribs) |
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