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SUMMARY:"The long-term oscillations in sunspots and related inter-sunspot 
 sources in microwave emission"
DTSTART;VALUE=DATE-TIME:20151008T113000Z
DTEND;VALUE=DATE-TIME:20151008T120000Z
DTSTAMP;VALUE=DATE-TIME:20260815T102449Z
UID:indico-contribution-39-452@cern.ch
DESCRIPTION:Speakers: Irina Bakunina (National Research University Higher 
 School of Economics)\nIrina A. Bakunina (1)\, Vladimir E. Abramov-Maximov 
 (2)\, Alexander A. Solov’ev  (2)\n(1) National Research University Highe
 r School of Economics\, 25/12 B. Pecherskaja ul.\, Nizhny Novgorod 603155\
 , Russia\nrinbak@mail.ru\n(2) Central Astronomical Observatory at Pulkovo\
 , Russian Academy of Sciences\, Pulkovskoe chaussee 65/1\, St Petersburg 1
 96140\, Russia\nbeam@gao.spb.ru\n\nThis work presents the microwave long-t
 erm oscillations with periods of a few tens of minutes obtained from Nobey
 ama radioheliograph (NoRH) at frequency 17 GHz. In number of active region
 s the fluctuations of  radio emission of different types of sources (spots
 \, compact and extended intersunspot sources (ISS)) were compared with the
  fluctuations in magnetic fields of sunspots. More significant correlation
  between the variations in magnetic field and radio emission was observed 
 for sunspots and compact ISS.\nWe adopt the cross-correlation analysis\, w
 avelet analysis\, and statistical tests to deduce the results. The model o
 f the shallow sunspot’s eigen oscillations is discussed  for explanation
  of the origin of quasi-periodic oscillations in sunspots and ISS.\n\nhttp
 s://indico.particle.mephi.ru/event/2/contributions/452/
LOCATION:Milan Hotel 4*
URL:https://indico.particle.mephi.ru/event/2/contributions/452/
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BEGIN:VEVENT
SUMMARY:Non-Radioactive fusion in $pd\\mu$ Muonic Molecule
DTSTART;VALUE=DATE-TIME:20151008T113000Z
DTEND;VALUE=DATE-TIME:20151008T120000Z
DTSTAMP;VALUE=DATE-TIME:20260815T102449Z
UID:indico-contribution-39-432@cern.ch
DESCRIPTION:https://indico.particle.mephi.ru/event/2/contributions/432/
LOCATION:Milan Hotel 4*
URL:https://indico.particle.mephi.ru/event/2/contributions/432/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Neutrino processes $\\nu \\bar\\nu \\to e^- e^+$ and $\\nu \\to \\
 nu e^- e^+$ in a strong magnetic field
DTSTART;VALUE=DATE-TIME:20151008T113000Z
DTEND;VALUE=DATE-TIME:20151008T120000Z
DTSTAMP;VALUE=DATE-TIME:20260815T102449Z
UID:indico-contribution-39-272@cern.ch
DESCRIPTION:Speakers: Vasiliy Savin (Yaroslavl Higher Military School of A
 ir Defence)\nThe processes of neutrino production of electron positron pai
 rs\, $\\nu \\bar\\nu \\to e^- e^+$ and $\\nu \\to \\nu e^- e^+$\, in a mag
 netic field of arbitrary strength\, where electrons and positrons can be c
 reated in the states corresponding to excited Landau levels\, are analysed
 . The mean values of the neutrino energy losses due to these processes are
  calculated. The results can be applied for calculating the efficiency of 
 the electron-positron plasma production by neutrinos in the conditions of 
 the Kerr black hole accretion disc considered by experts as the most possi
 ble source of a short cosmological gamma burst. The presented research can
  be also useful for further development of the calculation technic for an 
 analysis of quantum processes in external active medium\, and in part in t
 he conditions of moderately strong magnetic field\, when taking account of
  the ground Landau level appears to be insufficient.\n\nhttps://indico.par
 ticle.mephi.ru/event/2/contributions/272/
LOCATION:Milan Hotel 4*
URL:https://indico.particle.mephi.ru/event/2/contributions/272/
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