Zobrazeno 1 - 10
of 30
pro vyhledávání: '"I. S. Petukhov"'
Autor:
P. Yu. Gololobov, S. A. Starodubtsev, G. F. Krymsky, S. I. Petukhov, V. G. Grigoryev, I. S. Petukhov, A. S. Petukhova, S. K. Gerasimova, S. N. Taneev, V. I. Kozlov, A. S. Zverev
Publikováno v:
Physics of Atomic Nuclei. 84:1087-1097
Publikováno v:
Spravochnik. Inzhenernyi zhurnal. :20-26
An algorithm for determining the quality level of gas forming technology in the superplasticity mode of the material at the debugging stage is Developed. Proposed management measures to improve the new technology, which can help reduce the percentage
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:19-31
Publikováno v:
Space Weather. 18
Publikováno v:
E3S Web of Conferences, Vol 127, p 02007 (2019)
Geomagnetic storms are initiated by organized magnetic structures of the solar wind. The intensity of magnetic storms is determined by the product of the southward component of the magnetic field and the time interval, during which the structure is l
Publikováno v:
Journal of Physics: Conference Series. 1690:012016
Magnetic clouds affect the intensity of galactic cosmic rays. The diffusion mechanism is usually used as the formation mechanism for Forbush decrease (FD) in a magnetic cloud (MC). An FD is an observed decrease in the cosmic ray intensity. There is a
Publikováno v:
JETP Letters. 102:697-700
The time dynamics of the particle distribution function in a magnetic cloud with the shape of a toroidal segment with the characteristic (forceless) structure of a magnetic field has been calculated. The shape of the cloud at the subsequent propagati
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 81:532-534
The intensity of cosmic rays in a magnetic cloud is calculated. It is found that the duration of the Forbush decrease recovery is determined by the magnetic cloud orientation and the reduction in the magnetic field inside the magnetic cloud as it exp
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 81:529-531
The injection of solar cosmic rays with relativistic energies into interplanetary space is calculated within a new model of particle acceleration by shock waves in the solar atmosphere. A comparison of the calculation results and the particle injecti
Autor:
S. I. Petukhov, I. S. Petukhov
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 79:588-591
A model for the injection of flare solar energetic particles (SEP) from the solar atmosphere is proposed. SEP propagation in interplanetary space is calculated using the Krimigis model. The calculation results are compared to data on events recorded