Features of the impact of the solar wind diamagnetic structure on Earth’s magnetosphere

In Earth’s orbit on June 28, 1999, there was a diamagnetic structure (DS) representing a filament with a uniquely high speed (about 900 km/s). We show that the filament is a part of the specific sporadic solar wind (SW) stream, which is characterized as a small interplanetary transient. We report th...

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Autors principals:	Parkhomov V.A., Borodkova N.L., Eselevich V.G., Eselevich M.V., Dmitriev A.V., Chilikin V.E.
Format:	Artigo
Idioma:	Inglês
Publicat:	INFRA-M 2017-12-01
Col·lecció:	Solar-Terrestrial Physics
Matèries:	streamer filament diamagnetic structure; dayside auroras shock aurora substorm-like magnetospheric disturbance
Accés en línia:	https://naukaru.ru/ru/nauka/article/19710/view
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