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Autor:
Krainev M. B., Bazilevskaya G. A., Kalinin M. S., Mihaylov V. V., Svirzhevskaya A. K., Svirzhevsky N. S.
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 4, Pp 3-16 (2023)
The effects of the 22-year variation of solar magnetic fields in the galactic cosmic ray (GCR) intensity were first observed and interpreted as manifestations of inversion of the high-latitude solar magnetic field in properties of heliospheric magnet
Externí odkaz:
https://doaj.org/article/4a75dabc690042598fb71e43091ad39c
Autor:
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.
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 1, Pp 9-20 (2023)
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 heli
Externí odkaz:
https://doaj.org/article/e0ad6182c05248e3ac506e6608167633
Quasi-biennial oscillation (QBO) is a well-known quasi-periodical variation with characteristic time 0.5-4 years in different solar, heliospheric and cosmic ray characteristics. In this paper a hypothesis is checked on the causes of the apparent lack
Externí odkaz:
http://arxiv.org/abs/1509.00625
The maximum phase of the solar cycle is characterized by several interesting features in the solar activity, heliospheric characteristics and the galactic cosmic ray (GCR) intensity. Recently the maximum phase of the current solar cycle (SC) 24, in m
Externí odkaz:
http://arxiv.org/abs/1509.00613
Autor:
Kalinin, M. S., Bazilevskaya, G. A., Krainev, M. B., Svirzhevskaya, A. K., Svirzhevsky, N. S.
We discuss the main characteristic features in the heliospheric parameters important for the GCR intensity modulation for the last three solar minima (1986--1987, 1996--1997 and 2008--2009). The model for the GCR intensity modulation is considered an
Externí odkaz:
http://arxiv.org/abs/1411.7519
Autor:
Bazilevskaya, G. A., Kalinin, M. S., Krainev, M. B., Makhmutov, V. S., Svirzhevskaya, A. K., Svirzhevsky, N. S.
Modulation of galactic cosmic ray intensity is governed by several mechanisms including diffusion, convection, adiabatic energy losses and drift. Relative roles of these factors change in the course of an 11-year solar cycle. That can result in the c
Externí odkaz:
http://arxiv.org/abs/1411.7534
Autor:
Krainev, M. B., Bazilevskaya, G. A., Kalinin, M. S., Svirzhevskaya, A. K., Svirzhevsky, N. S.
Using the simple model for the description of the GCR modulation in the heliosphere and the sets of parameters discussed in the accompanying paper we model some features of the time and energy behavior of the GCR intensity near the Earth observed dur
Externí odkaz:
http://arxiv.org/abs/1411.7526
Autor:
Sloan, T., Bazilevskaya, G. A., Makhmutov, V. S., Stozhkov, Y. I., Svirzhevskaya, A. K., Svirzhevsky, N. S.
A survey of the data on measured particle fluxes and the rate of ionization in the atmosphere is presented. Measurements as a function of altitude, time and cut-off rigidity are compared with simulations of particle production from cosmic rays. The s
Externí odkaz:
http://arxiv.org/abs/1012.0250
Autor:
Mikhail Krainev, Mikhail Kalinin, Galina Bazilevskaya, Albina Svirzhevskaya, Nikolay Svirzhevsky, Xi Luo, O.P.M. Aslam, F. Shen, M.D. Ngobeni, M.S. Potgieter
Publikováno v:
Solnechno-Zemnaya Fizika. 9:10-21
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 heli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::608e213d4a24846ea17f67708e67ab56
https://doi.org/10.12737/szf-91202302
https://doi.org/10.12737/szf-91202302