Zobrazeno 1 - 10
of 92
pro vyhledávání: '"Grigoryev V.G."'
Publikováno v:
In Astroparticle Physics September 2021 131
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 3, Pp 93-97 (2019)
A method for forecasting geomagnetic storms using the realization of the global survey method in real time is presented. The method is based on data from the worldwide network of neutron monitors NMDB. Using this method, we analyze the behavior of co
Externí odkaz:
https://doaj.org/article/67fbd08f857b48b28aef827a7c226b19
Autor:
Starodubtsev S.A., Baishev D.G., Grigoryev V.G., Karimov R.R., Kozlov V.I., Korsakov A.A., Makarov G.A., Moiseev A.V.
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 1, Pp 14-27 (2019)
We report the results of monitoring of cosmic rays and geomagnetic field along 210 magnetic meridians in Yakutia in the first half of September 2017. The energy spectrum of solar cosmic rays during Ground Level Enhancement in September 10, 2017 is es
Externí odkaz:
https://doaj.org/article/214dfbccc6864aaca8fcc2196dd6a97f
Publikováno v:
Solar-Terrestrial Physics, Vol 3, Iss 2, Pp 20-24 (2017)
The observable anisotropy of cosmic rays has first been decomposed into zonal harmonics and components of vector and tensor anisotropy. We examine Forbush decreases in cosmic rays that occurred in November 2001 and November 2004. It is shown that at
Externí odkaz:
https://doaj.org/article/8433cea362d94d9297260dd99f9bf903
Publikováno v:
Solar-Terrestrial Physics, Vol 3, Iss 2, Pp 16-19 (2017)
We analyze time profiles of isotropic intensity, components of vector and tensor anisotropies of cos-mic rays (CR) when Earth crosses the neutral sheet of the interplanetary magnetic field (IMF) in solar activity cycles 23–24. The moments of the cr
Externí odkaz:
https://doaj.org/article/3ebd0394376845a197d8d09bf40eb262
Autor:
Gerasimova S.K., Gololobov P.Yu., Grigoryev V.G., Krivoshapkin P.A., Krymsky G.F., Starodubtsev S.A.
Publikováno v:
Solar-Terrestrial Physics, Vol 3, Iss 1, Pp 72-102 (2017)
This paper presents the basic model of cosmic ray modulation in the heliosphere, developed in Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences. The model has only one free modulat
Externí odkaz:
https://doaj.org/article/2abad8b20f7f4397818d83a8cf2224c4
Publikováno v:
Solar-Terrestrial Physics, Vol 2, Iss 1, Pp 103-119 (2016)
The method of receiving vectors allows us to determine cosmic ray anisotropy at every moment of time. Also, the method makes it possible to study fast anisotropy fluctuations related to the interplanetary medium dynamics. Receiving vectors have been
Externí odkaz:
https://doaj.org/article/3f59f1f96a8b4484915d52d225c19296
Akademický článek
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Autor:
Chuprova, V.P., Gerasimova, S.K., Grigoryev, V.G., Krivoshapkin, P.A., Krymsky, G.F., Mamrukova, V.P., Migunov, V.M., Prikhodko, A.N., Shafer, G.V., Skripin, G.V., Sorokin, Ye.Ye., Starodubtsev, S.A., Timofeev, V.E.
Publikováno v:
In Advances in Space Research 2009 44(10):1200-1206
Publikováno v:
In Advances in Space Research 2009 43(4):515-517