Empirical model of variations in the continuum emission in the upper atmosphere. 1. Intensity |
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| Authors: | A. I. Semenov N. N. Shefov I. V. Medvedeva |
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| Affiliation: | 1. Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences, Pyzhevskii per. 3, Moscow, 119017, Russia
2. Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, ul. Lermontova 126A, Irkutsk, 664033, Russia
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| Abstract: | The ground-based and satellite measurements of the upper-atmosphere continuum (continuous emission) intensity in the visible and near IR spectral regions have been analyzed. The data were obtained at the geophysical stations, located in different regions of the globe, and at Mir Space Station. The regularities in the spectral distribution of the continuum emission intensity and emission variations have been revealed for different heliogeophysical conditions. |
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