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

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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Bibliographic Details
Main Authors: Parkhomov V.A., Borodkova N.L., Eselevich V.G., Eselevich M.V., Dmitriev A.V., Chilikin V.E.
Format: Article
Language:English
Published: INFRA-M 2017-12-01
Series:Solar-Terrestrial Physics
Subjects:
streamer
filament
diamagnetic structure; dayside auroras
shock aurora
substorm-like magnetospheric disturbance
Online Access:https://naukaru.ru/ru/nauka/article/19710/view

Internet

https://naukaru.ru/ru/nauka/article/19710/view

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