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SUMMARY:Nuclear-Molecular Version of Processes of Dynamical Self-organizat
 ion of Solar Interiors and their Possible Role in Formation of Solar Activ
 ity
DTSTART;VALUE=DATE-TIME:20161011T124500Z
DTEND;VALUE=DATE-TIME:20161011T130000Z
DTSTAMP;VALUE=DATE-TIME:20260714T031430Z
UID:indico-contribution-767@cern.ch
DESCRIPTION:Speakers: Yuri Kopysov (INR RAS)\nThe new model of solar inter
 ior structure is discussed. It is consistent with results of years INR RAS
  measurements of solar neutrino fluxes and with the multi-year observation
 s of 160-minute solar atmosphere oscillations in the Crimean astrophysical
  observatory. The model is based on two hypotheses:\n\n 1. There is a slig
 htly subadiabatic solar troposphere under the superadiabatic convective zo
 ne\, which is a resonator for 160-minute *g*-mode oscillations.\n 2.  In a
 ddition to thermal branch of *pp*-reaction of hydrogen chain\, which gives
  the main contribution into solar luminocity\, there is a side nuclear-mol
 ecular catalytic brunch of *pp*-reaction\, which gives a small contributio
 n into solar luminocity\, but controls solar activity and supplies energy 
 to processes of dynamical solar interiors self-organization which are resp
 onsible for vigorous solar activity.\n\nThis new model can justify the nec
 essity of further searches and investigations of non-stationary solar neut
 rino fluxes.\n\nhttps://indico.particle.mephi.ru/event/4/contributions/767
 /
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/767/
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