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UV Radiation from the Night‐Time Atmosphere seen from the “Universitetsky‐Tatiana” Satelliteстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Дата последнего поиска статьи во внешних источниках: 16 февраля 2016 г.
- Авторы: Dmitriev A.V., Garipov G.K., Grigoryan O.R., Khrenov B.A., Klimov P.A., Lazutin L.L., Myagkova I.N., Petrov A.N., Petrov V.L., Panasyuk M.I., Tulupov V.I., Shahparonov V.M., Shirokov A.V., Vedenkin N.N., Yashin I.V., Jeon J.A., Jeong S.M., Jung A., Kim J.E., Kim W.S., Lee J., Lee H.Y., Na G.W., Nam S.W., Oh S.J., Park I.H., Park J.H., Jin J.Y., Kim M., Kim Y.K., Yoo B.W., Park Y.‐S, Yoo H.J., Lee C.H., Salazar H.I., Martinez O.B., Ponce and Cotsomi E.L.J.P
- Сборник: Coupling of Thunderstorms and Lightning Discharges to Near‐Earth Space: Proceedings of the Workshop
- Том: 1118
- Год издания: 2009
- Место издания: AIP Publishing USA
- Первая страница: 116
- Последняя страница: 123
- DOI: 10.1063/1.3137703
- Аннотация: Detectors on the “Universitetsky‐Tatiana” satellite measured a smoothly varying intensity of UV radiation from the night‐time atmosphere in the nadir direction and the intensity of the energetic electron flux at the orbit. At high latitudes the UV intensity in the auroral oval is interpreted as being due to electrons penetrating into the atmosphere. At middle latitudes the UV intensity is an order of magnitude less and more data are needed to reveal the origin of this radiation. Millisecond flashes of UV radiation were observed. The flashes’ energy, temporal profile and global distribution are similar to these parameters for Transient Luminous Events (TLEs). These studies will be continued aboard the next satellite “Tatiana‐2”.
- Добавил в систему: Шахпаронов Владимир Михайлович