Differences in the response to CME and CIR drivers of geomagnetic disturbances

Differences in the response to CME and CIR drivers of geomagnetic disturbances

Utilizing 1-minute resolution data on the geomagnetic indices SYM-H, AE, solar wind parameters (velocity Vsw and density Np), and z-component Bz of the interplanetary magnetic field (IMF) during solar cycles 23 and 24, we have statistically analyzed the correlations between geomagnetic activity (sto...

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Bibliographic Details
Main Authors: Namuun B., Tsegmed B., Li L., Leghari G.
Format: Article
Language:English
Published: INFRA-M 2023-06-01
Series:Solar-Terrestrial Physics
Subjects:
solar wind
coronal mass ejections
corotating interaction regions
geomagnetic storms
magnetospheric substorms
correlations
Online Access:https://naukaru.ru/en/nauka/article/54805/view

Internet

https://naukaru.ru/en/nauka/article/54805/view

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