Characteristic Features of Solar Cosmic Rays in the 21st–24th Solar-Activity Cycles According to Data from Catalogs of Solar Proton Events     

Bazilevskaya  G. A.  Daibog  E. I.  Logachev  Yu. I.  Vlasova  N. A.  Ginzburg  E. A.  Ishkov  V. N.  Lazutin  L. L.  Nguyen  M. D.  Surova  G. M.  Yakovchouk  O. S. 《Geomagnetism and Aeronomy》2021,61(1):6-13

Geomagnetism and Aeronomy - 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...  相似文献   

A 27-Day Period in the Flux of Jovian Electrons at the Earth’s Orbit     

E. I. Daibog  K. Kecskeméty  L. L. Lazutin  Yu. I. Logachev  G. M. Surova 《Astronomy Reports》2017,61(12):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 solar rotations; electrons were observed by SOHO during 14 solar rotations during the 2007–2008 cycle. The fluxes of these electrons in each solar revolution experienced variations with a characteristic time scale of ~27 ^d , with the maximum flux near the middle of the rotation. The mean period of the variations does not coincide with the synodic period for the Sun–Earth system, equal to 27.3 ^d . The mean variation periods for the electron fluxes were 26.8 ^d in 1974–1975 and 26.1 ^d in 2007–2008. The detected variations are interpreted as reflecting variations in the structure of the solar wind speed and associated magnetic traps, the confinement time of the electrons in thesemagnetic traps, and the influence of the relative positions of the Earth and Jupiter in space.  相似文献   

Statistical Links between Solar Cosmic Rays,Type-II Radio Emission,and Coronal Mass Ejections     

Bazilevskaya  G. A.  Logachev  Yu. I.  Daibog  E. I.  Vlasova  N. A.  Ginzburg  E. A.  Ishkov  V. N.  Lazutin  L. L.  Nguyen  M. D.  Surova  G. M.  Yakovchuk  O. S. 《Geomagnetism and Aeronomy》2021,61(5):773-779

Geomagnetism and Aeronomy - 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...  相似文献   

Solar energetic particle events from solar flares with weak impulsive phases of microwave emission     

E. I. Daibog  V. F. Mel'nikov  V. G. Stolpovskii 《Solar physics》1993,144(2):361-372

In some solar energetic particle events relatively intense proton fluxes are accompanied by disproportionately weak intensity of-burst. A possible reason for such a situation is discussed in this paper. We use the idea that the dynamics of particles in flare loops strongly influences the efficiency of their escape into interplanetary space. It is proposed that in events with weak impulsive phase flare loops are large sized and stretched high into the corona, the magnetic field is weak, and the level of excited turbulence is rather low. All this leads to the weak diffusion of protons into the loss cone, a large lifetime of a particle in the loop ( 10³ s) and, hence, to the relatively high efficiency of their escape into interplanetary space.  相似文献