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

共 50 条

[1] Effect of Corotating Interaction Regions of Solar Wind on GCR Intensity in 2D Modulation Problems
Kalinin, M. S.
Krainev, M. B.
Luo, X.
Podgieter, M. S.
GEOMAGNETISM AND AERONOMY, 2024, 64 (07) : 1098 - 1108
[2] The Influence of Corotating Regions of Interaction of the Solar Wind on Long-Term Variations in the Intensity of Galactic Cosmic Rays
Kalinin, M. S.
Krainev, M. B.
Luo, X.
Potgieter, M. S.
GEOMAGNETISM AND AERONOMY, 2023, 63 (05) : 536 - 546
[3] Energetic particles and corotating interaction regions in the solar wind
Richardson, IG
SPACE SCIENCE REVIEWS, 2004, 111 (3-4) : 267 - 376
[4] Energetic Particles and Corotating Interaction Regions in the Solar Wind
Ian G. Richardson
Space Science Reviews, 2004, 111 : 267 - 376
[5] MANIFESTATIONS OF TWO BRANCHES OF SOLAR ACTIVITY IN THE HELIOSPHERE AND GCR INTENSITY
Krainev, M. B.
SOLAR-TERRESTRIAL PHYSICS, 2019, 5 (04): : 10 - 20
[6] Simulation of Solar Wind Turbulence near Corotating Interaction Regions: Superposed Epoch Analysis of Simulations and Observations
Ghanbari, Keyvan
Florinski, Vladimir
ASTROPHYSICAL JOURNAL, 2023, 943 (02):
[7] Solar wind stream interaction regions throughout the heliosphere
Richardson, Ian G.
LIVING REVIEWS IN SOLAR PHYSICS, 2018, 15
[8] Corotating interaction regions during the recent solar minimum: The power and limitations of global MHD modeling
Riley, Pete
Linker, Jon A.
Lionello, R.
Mikic, Z.
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2012, 83 : 1 - 10
[9] Analytic modeling of recurrent Forbush decreases caused by corotating interaction regions
Vrsnak, B.
Dumbovic, M.
Heber, B.
Kirin, A.
ASTRONOMY & ASTROPHYSICS, 2022, 658
[10] ELEMENTAL ABUNDANCES IN COROTATING INTERACTION REGIONS AT HIGH SOLAR LATITUDES
MACLENNAN, CG
LANZEROTTI, LJ
SPACE SCIENCE REVIEWS, 1995, 72 (1-2) : 297 - 302

← 1 2 3 4 5 →