Manifestation of solar wind corotating interaction regions in GCR intensity variations

Manifestation of solar wind corotating interaction regions in GCR intensity variations

The regions of interaction between solar wind streams of different speed, known as corotating interaction regions, form an almost constantly existing structure of the inner heliosphere. Using observational data on the main characteristics of the heliosphere, important for GCR modulation, and the res...

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Bibliographic Details
Main Authors: Krainev M. B., Kalinin M. S., Bazilevskaya G. A., Svirzhevskaya A. K., Svirzhevsky N. S., Luo X., Aslam O., Shen F., Ngobeni M., Potgieter M.
Format: Article
Language:English
Published: INFRA-M 2023-03-01
Series:Solar-Terrestrial Physics
Subjects:
heliosphere
corotating interaction regions
galactic cosmic rays
gcr modulation
long-term gcr variations
27-day gcr intensity variation
mhd approximation
monte carlo method
Online Access:https://naukaru.ru/en/nauka/article/55377/view

Internet

https://naukaru.ru/en/nauka/article/55377/view

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