Zobrazeno 1 - 10
of 41
pro vyhledávání: '"E. I. Daibog"'
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
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
Autor:
Yu. I. Logachev, E. I. Daibog
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 85:1032-1035
A combination of two power laws is used to present spectra of electrons in the MeV range of energies, measured during the solar activity minimum in 2007−2008 by the Electron Proton Helium Instrument (EPHIN) on board the Solar and Heliospheric Obser
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 502:2541-2548
This work studies the influence of the structure of inner heliospheric magnetic field on the propagation of Jovian electrons from Jupiter to the Earth orbit. Beginning from 1974, 13-month variations of relativistic Jovian electron fluxes were recorde
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,
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
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
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 81:136-139
The results from observing Jovian electrons in the vicinity of the Earth are discussed. Variations in Jovian electron flows are observed during 14 rotations of the Sun in 2007–2008. The results are analyzed by assuming the existence of magnetic tra
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