Manifestation of solar wind corotating interaction regions in GCR intensity variations-Reference-Cited by-同舟云学术

Manifestation of solar wind corotating interaction regions in GCR intensity variations

Published:2023-03-28 Issue:1 Volume:9 Page:10-21
ISSN:2712-9640
Container-title:Solnechno-Zemnaya Fizika
language:en
Short-container-title:

Author:

Krainev Mikhail¹²,Kalinin Mikhail³,Bazilevskaya Galina³,Svirzhevskaya Albina³,Svirzhevsky Nikolay³,Luo Xi²,Aslam O.P.M.²,Shen F.⁴,Ngobeni M.D.⁵⁶,Potgieter M.S.²⁷

Affiliation:

1. Lebedev Physical Institute, RAS

2. Shandong Institute of Advanced Technology

3. P.N. Lebedev Physical Institute of RAS

4. National Space Science Center

5. North-West University, Centre for Space Research

6. School of Physical and Chemical Sciences, North-West University

7. nstitute for Experimental and Applied Physics, Christian Albrechts University

Abstract

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 results of 3D MHD modeling of corotating interaction regions, and Monte Carlo simulation of recurrent GCR variations, we analyze the importance of the corotating interaction regions for longitude-averaged characteristics of the heliosphere and GCR propagation, and possible ways for simulating long-term GCR intensity variations with respect to the corotating interaction regions.

Publisher

Infra-M Academic Publishing House

Subject

General Medicine

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