Zobrazeno 1 - 10
of 150
pro vyhledávání: '"Kalinin, A S"'
Autor:
Krainev M. B., Kalinin M. S.
Publikováno v:
Solar-Terrestrial Physics, Vol 10, Iss 3, Pp 37-49 (2024)
Phenomena in the outer layer of the solar atmosphere, the heliosphere, including the supersonic solar wind, the heliospheric magnetic field (HMF) carried by it, and cosmic rays propagating in the heliosphere are important for many processes occurring
Externí odkaz:
https://doaj.org/article/313f758f41f44336aecee2f5987a683f
Autor:
Kalinin, Danil S., Mayorov, Sergey G., Zemskova, Marina Yu., Latypov, Oleg R., Shlyapnikov, Michael G., Gorshkova, Maria A., Titova, Eva N., Vlasova, Natalia N., Lipkin, Alexey V., Fedorov, Alexey N., Granovsky, Igor E.
Publikováno v:
In Journal of Virological Methods December 2024 330
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
Akademický článek
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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., Kalinin, M. S.
We consider the long-term behavior of the solar and heliospheric parameters and the GCR intensity in the periods of high solar activity and the inversions of heliospheric magnetic field (HMF). The classification of the HMF polarity structures and the
Externí odkaz:
http://arxiv.org/abs/1411.7532
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:
Kalinin, R. S.1 (AUTHOR) Roman.Kalinin.93@yandex.ru, Shipunova, V. O.1 (AUTHOR), Rubtsov, Y. P.1 (AUTHOR), Ukrainskay, V. M.1,2 (AUTHOR), Schulga, A.1 (AUTHOR), Konovalova, E. V.1 (AUTHOR), Volkov, D. V.1 (AUTHOR), Yaroshevich, I. A.3 (AUTHOR), Moysenovich, A. M.3 (AUTHOR), Belogurov, A. A.1,3 (AUTHOR), Telegin, G. B.1 (AUTHOR), Chernov, A. S.1 (AUTHOR), Maschan, M. A.2 (AUTHOR), Terekhov, S. S.1,3 (AUTHOR), Knorre, V. D.1 (AUTHOR), Khurs, E.4 (AUTHOR), Gnuchev, N. V.4 (AUTHOR), Gabibov, A. G.1,3 (AUTHOR), Deyev, S. M.1,5 (AUTHOR)
Publikováno v:
Doklady Biochemistry & Biophysics. Feb2023, Vol. 508 Issue 1, p17-20. 4p.