Possible difference in the formation of coronal mass ejections of two types

Possible difference in the formation of coronal mass ejections of two types

Analysis of seven near-limb coronal mass ejections (CMEs) has shown that at distances R<1.4R from the center of the Sun CMEs according to their formation can be divided into two types: type 1 CMEs and type 2 CMEs. In the case of type 1 CMEs, the frontal structure (FS) is formed by processes occu...

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Bibliographic Details
Main Authors: Eselevich V. G., Eselevich M. V., Zimovets I. V.
Format: Article
Language:English
Published: INFRA-M 2022-06-01
Series:Solar-Terrestrial Physics
Subjects:
coronal mass ejection
magnetic flux rope
coronal arched structures
flare
eruptive prominence
Online Access:https://naukaru.ru/en/nauka/article/47753/view

Internet

https://naukaru.ru/en/nauka/article/47753/view

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