Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Mikhail Krainev"'
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
Publikováno v:
Advances in Space Research. 68:2953-2962
Effects on galactic cosmic rays (GCRs) of several heliospheric factors during the minimum phases of the sunspot cycles are studied. Times of maximum GCR intensity are determined for the last five sunspot minima, including the present one, together wi
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:1179-1182
A study is performed of phases of solar cycle minima in sunspots, the heliosphere, and the intensity of Galactic cosmic rays (GCRs). Times of maximum GCR intensity in the minima of the last five cycles (including the current one), corresponding main
Autor:
V. S. Makhmutov, Mikhail Krainev, A. K. Svirzhevskaya, Yu. I. Stozhkov, M. S. Kalinin, N. S. Svirzhevsky, G. A. Bazilevskaya
Publikováno v:
Geomagnetism and Aeronomy. 61:299-311
In the Parker model of the heliospheric magnetic field, the ratio of the azimuthal field component $${{B}_{{{\varphi }}}}$$ to the radial component $${{B}_{r}}$$ depends only on the radial speed V of the solar wind and coordinates of the observation
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:1176-1178
The effect the three-component heliospheric magnetic field has on the modulation of galactic cosmic rays is considered. Radial and longitudinal components of the model are associated by the familiar Parker ratio. The latitudinal component is proporti
Autor:
A. S. Dyusembekova, A. K. Svirzhevskaya, G. A. Bazilevskaya, M. S. Kalinin, Yu. I. Stozhkov, E. A. Tulekov, Mikhail Krainev, V. S. Makhmutov, N. S. Svirzhevsky
Publikováno v:
Cosmic Research. 59:24-29
Energetic electron precipitation (EEP) into the atmosphere is one of the mechanisms of depleting the Earth’s outer radiation belt. Precipitating electrons generate bremsstrahlung that penetrates the stratosphere and is recorded by detectors on ball
Autor:
Donald Ngobeni, Mikhail Krainev, Mikhail Kalinin, Marius Potgieter, O. P. M. Aslam, Boris Gvozdevsky
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The conditions in the heliosphere are considered during the minimum phase of the sunspot cycle when the intensity of galactic cosmic rays (GCRs) attains its maximum at the Earth. These times of maximum GCR intensity are determined for the last five s
Autor:
Mikhail Krainev
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 4, Pp 10-20 (2019)
This paper provides insight into heliospheric processes and galactic cosmic ray (GCR) modulation occurring due to the presence of two branches of solar activity in this solar layer. According to the topology of solar magnetic fields, these branches a
Autor:
Yu. I. Stozhkov, Mikhail Krainev, V. S. Makhmutov, A. K. Svirzhevskaya, B. B. Gvozdevsky, N. S. Svirzhevsky, G. A. Bazilevskaya, M. S. Kalinin
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 83:584-587
Ionizing radiation fluxes in the Earth’s atmosphere have been measured at the Lebedev Physical Institute since 1957. They allow the recording of X-ray radiation generated in the atmosphere by precipitating magnetospheric electrons with energies abo
Autor:
M. S. Kalinin, Mikhail Krainev
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 83:555-558
The influence of the global heliospheric current sheet on the heliospheric characteristics important for GCR propagation is considered, particularly the strong dependence of the solar wind velocity on the distance from the current sheet. A simple mod