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The structure of the magnetospheric boundary layers and the magnetospheric turbulenceстатья
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: 9 апреля 2015 г.
- Автор: Antonova E.E.
- Журнал: Planetary and Space Science
- Том: 53
- Номер: 1-3
- Год издания: 2005
- Издательство: Elsevier BV
- Местоположение издательства: Netherlands
- Первая страница: 1
- Последняя страница: 3
- DOI: 10.1016/j.pss.2004.09.041
- Аннотация: The concept of the formation of the turbulent wake under the obstacle gives the possibility to explain many features of the plasma dynamics in the magnetosphere of the Earth. The formation of the plasma sheet and tail lobes in accordance with this concept is explained as the result of the interactions of large-scale (the dawn-dusk electric field) and medium-scale modes of magnetospheric turbulence. The application of the developed approach to the problem of the boundary layer formation gives the possibility to explain the low latitude boundary layer (LLBL) thickness during southward and northward interplanetary magnetic field orientations and the dawn-dusk LLBL asymmetry. Theory predictions are compared with the results of experimental observations.
- Добавил в систему: Антонова Елизавета Евгеньевна