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SUMMARY:Method of solar neutron exploring with PAMELA neutron detector
DTSTART;VALUE=DATE-TIME:20161011T121500Z
DTEND;VALUE=DATE-TIME:20161011T124500Z
DTSTAMP;VALUE=DATE-TIME:20260714T044551Z
UID:indico-contribution-528@cern.ch
DESCRIPTION:Speakers: Victoria Goryacheva (NRNU MEPHI)\nThis work is devot
 ed to methodology of solar neutrons search during solar \nevents by using 
 a neutron detector of the PAMELA the magnetic \nspectrometer on-board RESU
 RS-DK1 satellite. Analysis of counts rates showed that in the geomagnetic 
 equator region the detector performance is nominal and \nbackground condit
 ions are stable. Maps of background fluxes were constructed and then 27 so
 lar events were examined in the period from December 2006\n to September 2
 014. In some events\, there are evidence \n of neutrons count rate increas
 ing during solar events. To make conclusion about the nature of these neut
 rons statistics and monitoring intervals need to be increased\, that requi
 res the analysis of background conditions in the Polar Regions\n\nhttps://
 indico.particle.mephi.ru/event/4/contributions/528/
LOCATION:Milan Hotel Hall of the 2nd floor
URL:https://indico.particle.mephi.ru/event/4/contributions/528/
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