MANIFESTATION OF SOLAR WIND COROTATING INTERACTION REGIONS IN GCR INTENSITY VARIATIONS

被引：4

作者：

Krainev, M. B. ^{[1
,2
]}

Kalinin, M. S. ^{[1
]}

Bazilevskaya, G. A. ^{[1
]}

Svirzhevskaya, A. K. ^{[1
]}

Svirzhevsky, N. S. ^{[1
]}

Luo, Xi ^{[2
]}

Aslam, O. P. M. ^{[2
]}

Shen, Fang ^{[3
]}

Ngobeni, M. D. ^{[4
,5
]}

Potgieter, M. S. ^{[2
,6
]}

机构：

[1] RAS, PN Lebedev Phys Inst, Moscow, Russia

[2] Shandong Inst Adv Technol, Jinan, Shandong, Peoples R China

[3] Natl Space Sci Ctr, Beijing, Peoples R China

[4] North West Univ, Ctr Space Res, Potchefstroom, South Africa

[5] North West Univ, Sch Phys & Chem Sci, Mmabatho, South Africa

[6] Univ Kiel, Inst Expt & Appl Phys, Kiel, Germany

来源：

SOLAR-TERRESTRIAL PHYSICS | 2023年 / 9卷 / 01期

基金：

美国国家科学基金会;

关键词：

heliosphere; corotating interaction regions; galactic cosmic rays; GCR modulation; long-term GCR variations; 27-day GCR intensity variation; MHD approx-imation; Monte Carlo method; GALACTIC COSMIC-RAYS; MAGNETIC-FIELD; MODULATION; TRANSPORT; DRIFT;

D O I：

10.12737/stp-91202302

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

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, im-portant for GCR modulation , the results of 3D MHD modeling of corotating interaction regions, , 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.

引用

页码：9 / 20

页数：12

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