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

Reference49 articles.

1. Калинин М.С., Крайнев М.Б. Двумерное транспортное уравнение для галактических космических лучей как следствие редукции трехмерного уравнения. Геомагнетизм и аэрономия. 2014. Т. 54, № 4. С. 463–469. DOI: 10.7868/ S0016794014040051., Adriani O., Barbarino G.C., Bazilevskaya G.A., Bellotti R., Boezio M., Bogomolov E.A., et al. Time dependence of the proton flux measured by PAMELA during the 2006 July – 2009 December solar minimum. Astrophys. J. 2013, vol. 765:91, no. 2. DOI: 10.1088/0004-637X/765/2/91.

2. Крайнев М.Б. Проявления в гелиосфере и в интенсивности ГКЛ двух ветвей солнечной активности. Солнечно-земная физика. 2019. Т. 5, № 4. С. 12–25. DOI: 10.12737/ szf-54201902., Aslam O.P.M., Bisschoff D., Potgieter M.S., Boezio M., Munini R. Modeling of heliospheric modulation of cosmic-ray positrons in a very quiet heliosphere. Astrophys. J. 2019, vol. 8736: 70, no. 1. DOI: 10.3847/1538-4357/ab05e6.

3. Крайнев М.Б., Базилевская Г.А., Боркут И.К. и др. О связи долготного распределения гелиосферных характеристик и интенсивности ГКЛ в 2007–2008 и 2014–2015 гг. Ядерная физика и инжиниринг. 2017. Т. 8, № 4. С. 373–379. DOI: 10.1134/S2079562917040157., Belcher J.W., Davis L. Large-amplitude Alfvén waves in the interplanetary medium, 2. J. Geophys. Res. 1971, vol. 76, iss. 16, p. 3534. DOI: 10.1029/JA076i016p03534.

4. Крымский Г.Ф. Диффузионный механизм суточных вариаций космических лучей. Геомагнетизм и аэрономия. 1964. Т. 4. С. 977., Burlaga L.F., Ness N.F., Wang J.-M., Sheeley N.R. Heliospheric magnetic field strength and polarity from 1 to 81 AU during the ascending phase of solar cycle 23. J. Geophys. Res. 2002, vol. 107, no. A11, p. 1410. DOI: 10.1029/2001JA009217.

5. Свиржевский Н.С., Базилевская Г.А., Калинин М.С. и др. Моделирование интенсивности галактических космических лучей с учетом пространственной и временной зависимости спектра флуктуаций гелиосферного магнитного поля. Известия РАН. Сер. физ. 2015. Т. 79, № 5. С. 663–666. DOI: 10.7868/S0367676515050415., Gosling J.T., Pizzo V. Formation and evolution of corotating interaction regions and their three dimensional structure. Space Sci. Rev. 1999, vol. 89, pp. 21–52. DOI: 10.1023/A:100 5291711900.

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The Influence of Corotating Regions of Interaction of the Solar Wind on Long-Term Variations in the Intensity of Galactic Cosmic Rays;Геомагнетизм и аэрономия;2023-09-01