Zobrazeno 1 - 10
of 2 433
pro vyhledávání: '"Gololobov"'
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 2, Pp 78-85 (2023)
During large-scale solar wind disturbances, variations in galactic cosmic rays with periods from several minutes to 2–3 hours, which are called cosmic ray fluctuations in the scientific literature, often occur. Such fluctuations are not observed in
Externí odkaz:
https://doaj.org/article/aa03669342d1435f85b3341ee99c3474
Autor:
Bobrowskii Alexander V., Zotov Alexey V., Bobrowskii Dmitry A., Gololobov Mikhail P., Chizhatkina Ekaterina D.
Publikováno v:
E3S Web of Conferences, Vol 471, p 04002 (2024)
The study is focused on presenting an assessment of additive manufacturing usage in modern technological processes, including the manufacturing of parts of the racing car participating in Formula Student project. It shows the necessity of simulating
Externí odkaz:
https://doaj.org/article/0fd3aed5a53e451eb130d5bf9713d978
Publikováno v:
Solar-Terrestrial Physics, Vol 6, Iss 1, Pp 24-28 (2020)
The work studies the cumulative modulating effect of the geometry of the interplanetary magnetic field's neutral current sheet and solar activity on propagation of galactic cosmic rays in the heliosphere. The role of each factor on the modulation of
Externí odkaz:
https://doaj.org/article/27fbdbb784234f72a1e7b269c0b6a7d9
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:
Gololobov A.Yu., Golikov I.A.
Publikováno v:
Solar-Terrestrial Physics, Vol 5, Iss 1, Pp 62-68 (2019)
The electron temperature enhancement is known to occur in the main ionospheric trough during geomagnetic disturbances. In this paper, we study fea-tures of the formation of the electron temperature (Te) enhancement in the subauroral ionosphere by com
Externí odkaz:
https://doaj.org/article/d701a9bf0944446fadb5b9c8824b1a96
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 4, Pp 70-80 (2016)
Using the three-dimensional model of the high-latitude ionosphere in Euler variables, which takes into account the mismatch between geographic and geomagnetic poles, we study the behavior of the electron temperature Te in the F2 region as a function
Externí odkaz:
https://doaj.org/article/70b3f4f5ca524f45a951ef51af0afcd0
Publikováno v:
Solar-Terrestrial Physics, Vol 3, Iss 2, Pp 51-53 (2017)
We present results of modeling of the electron temperature distribution in the F region of the subauroral ionosphere for different helio-geomagnetic conditions with consideration for magnetospheric heat fluxes. It is shown that under quiet geomagneti
Externí odkaz:
https://doaj.org/article/3d4a76548eee4d89abbd6e4632d1b227