Zobrazeno 1 - 10
of 18
pro vyhledávání: '"G. M. Surova"'
Autor:
N. A. Vlasova, Yu. I. Logachev, G. A. Bazilevskaya, E. A. Ginzburg, E. I. Daibog, V. N. Ishkov, V. V. Kalegaev, L. L. Lazutin, M. D. Nguyen, G. M. Surova, O. S. Yakovchuk
Publikováno v:
Cosmic Research. 60:151-164
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cefc0df400f240862229539b397ad4bd
https://doi.org/10.1134/s001095252203008x
https://doi.org/10.1134/s001095252203008x
Autor:
E. I. Daibog, E. A. Ginzburg, V. N. Ishkov, Yu. I. Logachev, Minh-Duc Nguyen, Natalia Vlasova, Leonid Lazutin, G. A. Bazilevskaya, O. S. Yakovchuk, G. M. Surova
Publikováno v:
Geomagnetism and Aeronomy. 61:773-779
Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the accelera
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e649e43f7257c663086ec41b3cfa24d
https://doi.org/10.1134/s0016793221050030
https://doi.org/10.1134/s0016793221050030
Autor:
O. S. Yakovchouk, V. N. Ishkov, Minh-Duc Nguyen, Leonid Lazutin, E. I. Daibog, G. M. Surova, E. A. Ginzburg, Natalia Vlasova, G. A. Bazilevskaya, Yu. I. Logachev
Publikováno v:
Geomagnetism and Aeronomy. 61:6-13
Homogeneous series of solar cosmic-ray events for four solar-activity cycles against the background of decreased activity in cycles 23 and 24 are considered. The number of solar cosmic-ray events with energies above 10 MeV decreased insignificantly,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7085d38cef2d6c2da7295ba1b2ffaab6
https://doi.org/10.1134/s0016793221010023
https://doi.org/10.1134/s0016793221010023
Autor:
V. N. Ishkov, G. M. Surova, Yu. I. Logachev, G. A. Bazilevskaya, Leonid Lazutin, E. I. Daibog
Publikováno v:
Physics of Atomic Nuclei. 81:384-389
Solar proton events possess a wide variety of features that reflect the conditions of solar proton acceleration and propagation. Relevant investigations rely on statistical methods that make it possible to classify events with the aim of obtaining de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d09423eb1f100029d0f3c8bd100c718e
https://doi.org/10.1134/s106377881803016x
https://doi.org/10.1134/s106377881803016x
Publikováno v:
Astronomy Reports. 61:1073-1081
Variations in the flux of Jovian electrons near the Earth in two synodic cycles of the Earth–Jupiter system, in 1974–1975 and 2007–2008, are considered. In the 1974–1975 cycle, Jovian electrons were observed by IMP-8 during 13 successive sola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e20cbc0e0744bc4e791593bf09bd204b
https://doi.org/10.1134/s1063772917120010
https://doi.org/10.1134/s1063772917120010
Autor:
Natalia Vlasova, E. A. Ginzburg, Minh-Duc Nguyen, E. I. Daibog, G. A. Bazilevskaya, Leonid Lazutin, V. N. Ishkov, Yu. I. Logachev, G. M. Surova, O. S. Yakovchouk
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4d1d2e2cd89397f353c50e767253a1ce
https://doi.org/10.31401/ws.2019.proc
https://doi.org/10.31401/ws.2019.proc
Publikováno v:
Cosmic Research. 54:416-422
A comparative analysis has been carried out of the parameters of energetic electrons in the tail of the Earth’s magnetosphere that belong to three sources, i.e., electrons of solar origin, electrons generated in the magnetosphere of Jupiter, and el
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5e3a4b99a763b765d06ddbc0714921c3
https://doi.org/10.1134/s0010952516060022
https://doi.org/10.1134/s0010952516060022
Publikováno v:
Astronomy Reports. 60:687-693
The energy spectra and relative abundances of 3He, 4He, C, O, and Fe ions with energies of ~0.04–2 MeV/nucleon are studied using data from the ULEIS instrument on board the ACE spacecraft obtained during quiescent periods in 2006–2012. During the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::864c6537adeca278fa8fead1161b1ad7
https://doi.org/10.1134/s1063772916070106
https://doi.org/10.1134/s1063772916070106
Autor:
Yu. I. Logachev, E. I. Daibog, O. S. Yakovchouk, Leonid Lazutin, V. N. Ishkov, G. M. Surova, I. E. Petrenko, G. A. Bazilevskaya, Leonty I. Miroshnichenko, E. V. Vashenyuk, M. N. Nazarova
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 79:573-576
It is shown that the number of solar proton events (SPEs) with proton energies (E) higher than 10 and 100 MeV in the current solar cycle (cycle 24) differs slightly from the number of the same events in earlier cycles (cycles 21–23), even though so
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e331aaebaf9bf62d03b695d252fb69f8
https://doi.org/10.3103/s1062873815050135
https://doi.org/10.3103/s1062873815050135
Autor:
M. N. Nazarova, G. A. Bazilevskaya, Yu. I. Logachev, V. N. Ishkov, Leonid Lazutin, O. S. Yakovchouk, Leonty I. Miroshnichenko, E. I. Daibog, E. V. Vashenyuk, I. E. Petrenko, A. G. Stupishin, G. M. Surova
Publikováno v:
Geomagnetism and Aeronomy. 55:277-286
The solar proton singularities in cycles 20–23 were compared. For such a comparison, it is of special importance to present information about solar proton events (SPEs) uniformly. The Katalog working group, including representatives of different in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d39b3dcbd51ef6647c470bc079814b78
https://doi.org/10.1134/s0016793215030135
https://doi.org/10.1134/s0016793215030135