Studying the relationship of localization parameters of solar sources of magnetic clouds with their characteristics and substorm activity

We propose a method for determining location and orientation of extended solar sources of magnetic clouds, using coronagraph data and SOHO EIT/MDI images of the photosphere. To estimate the probability of formation of magnetic clouds, we use a simple cylindrical force-free model. We have established...

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Bibliographic Details
Main Authors: Barkhatov N.A., Revunova E.A., Romanov R.V., Barkhatova O.M., Revunov S.E.
Format: Article
Language:English
Published: INFRA-M 2019-09-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/30597/view