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The influence of effects of the heliospheric interface on parameters of backscattered solar L alpha radiation measured at the Earth's orbitстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 18 июля 2013 г.
- Авторы: Katushkina O.A., Izmodenov V.V.
- Журнал: Cosmic Research (English translation of Kosimicheskie Issledovaniya)
- Том: 50
- Номер: 2
- Год издания: 2012
- Издательство: Pleiades Publishing, Inc.
- Местоположение издательства: New York, USA
- Первая страница: 141
- Последняя страница: 151
- DOI: 10.1134/S0010952512010030
- Аннотация: A new kinetic model of distribution of interstellar hydrogen atoms in the heliosphere is suggested in this paper. It takes into account global effects associated with charge exchange of interstellar atoms near the heliospheric boundary. The constructed model allows one to find efficiently the detailed distribution of hydrogen atoms over space and velocities. For the axisymmetric steady-state case a comparison is made of the parameters of interstellar hydrogen atoms that were obtained using the classical hot model, two modifications of the improved hot model, and a global self-consistent kinetic gas-dynamic model of the heliospheric interface. The results of calculations of the spectral moments of scattered solar L alpha radiation are presented. They were derived on the basis of different models of distribution of hydrogen atoms in the heliosphere.
- Добавил в систему: Измоденов Владислав Валерьевич