Speaker
Dr.
Yuri Kopysov
(INR RAS)
Description
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 zone, which is a resonator for 160-minute *g*-mode oscillations.
2. In addition to thermal branch of *pp*-reaction of hydrogen chain, which gives the main contribution into solar luminocity, there is a side nuclear-molecular catalytic brunch of *pp*-reaction, which gives a small contribution into solar luminocity, but controls solar activity and supplies energy to processes of dynamical solar interiors self-organization which are responsible for vigorous solar activity.
This new model can justify the necessity of further searches and investigations of non-stationary solar neutrino fluxes.
Primary author
Dr.
Yuri Kopysov
(INR RAS)
