Dr.
Yuri Kopysov
(INR RAS)
11/10/2016, 15:45
The new model of solar interior structure is discussed. It is consistent with results of years INR RAS measurements of solar neutrino fluxes and with the multi-year observations of 160-minute solar atmosphere oscillations in the Crimean astrophysical observatory. The model is based on two hypotheses:
1. There is a slightly subadiabatic solar troposphere under the superadiabatic convective...
Mr.
Alexander Byzykchi
(Ulyanovsk State University)
11/10/2016, 16:00
We solve the inverse problem of parameter determination for the generalized compound diffusion model from the simulation results [Pucci F. et al. Monthly Notices of the Royal Astron. Soc. (2016) 459, 3, 3395] for particle transport in the turbulent magnetic field (TMF). We find the distribution density p(x) of the parallel free path along a regular TMF component and the parameters of the...
Prof.
Igor Podgorny
(Institute of Astronomy of the Russian Academy of Sciences)
11/10/2016, 16:15
The analysis of GOES spacecraft measurements confirms the data of worldwide network of neutron monitors about solar cosmic ray generation in the solar flares above of an active region with the complex magnetic field distribution. The proton acceleration in a particular flare is beyond doubt. The so-called prompt proton component arrives to the Earth from western flares with a sharp (~5 min)...
Andrey Mayorov
(National Research Nuclear University MEPhI)
11/10/2016, 16:30
Solar modulation of galactic protons and helium with energies from ~50 MeV up to dozens of GeV during July ‘06 - January ‘16 studied based on a data of the magnetic spectrometer PAMELA and scintillation spectrometer ARINA. This period is interesting because it covers the end of 23rd and current 24th cycles of solar activity, including the abnormally long transient period and change of the...
Mr.
Sergey Koldobskiy
(NRNU MEPhI)
11/10/2016, 16:45
First results of cosmic ray deuteron spectra modulation are presented in this work. The data from the international space-born PAMELA experiment was analyzed. Deuterons were selected by multiparameter correlation technique in the energy range from 100 to 600 MeV/nucleon and the differential energy spectra were reconstructed for last solar minimum.
