Atmospheric ultraviolet light and comparison of its intensity with the variation of electron flux with energies higher than 70 KeV in satellite orbit (according to Universitetskii-Tatiana satellite data)

N. N. Veden'kin, A. V. Dmitriev, G. K. Garipov, P. A. Klimov, V. S. Morozenko, I. N. Myagkova, M. I. Panasyuk, S. N. Petrova, I. A. Rubinshtein, U. Salazar, S. I. Svertilov, V. I. Tulupov, B. A. Khrenov, V. M. Shakhparonov, A. V. Shirokov, I. V. Yashin

研究成果: 雜誌貢獻期刊論文同行評審

4 引文 斯高帕斯(Scopus)

摘要

The ultraviolet radiation of the night atmosphere and electron fluxes with energies higher than 70 keV are measured simultaneously onboard the satellite Universitetskii-Tatiana. It has been revealed that the mean intensity of ultra-violet radiation increases and this could be due to electron acceleration in atmospheric electric discharges with further capture by the geomagnetic field and electron precipitation in conjugated points of the geomagnetic field.

原文???core.languages.en_GB???
頁(從 - 到)450-454
頁數5
期刊Moscow University Physics Bulletin
64
發行號4
DOIs
出版狀態已出版 - 8月 2009

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