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SUMMARY:Upper limits on high-energy solar neutrons from satellite-detected
  flares with the Yangbajing neutron monitor
DTSTART;VALUE=DATE-TIME:20070704T194500Z
DTEND;VALUE=DATE-TIME:20070704T194500Z
DTSTAMP;VALUE=DATE-TIME:20260418T161955Z
UID:indico-contribution-664@cern.ch
DESCRIPTION:Speakers: Dr. TSUCHIYA\, HARUFUMI (RIKEN\, 2-1\, Wako\, Saitam
 a 351-0198\,  Japan)\nThe Yangbajing neutron monitor is suitable for obser
 ving solar neutrons in\nassociation with solar flares due to a location wi
 th an altitude of 4\,300 m above sea\nlevel. \nUsing data of the Yangbajin
 g neutron monitor obtained during 1998 and 2001\, \nwe searched for solar 
 neutrons from individual solar flares detected by BATSE and\nYohkoh. No si
 gnal due to solar neutrons was found in coincidence with those solar\nflar
 es. \nThe 95 \\% confidence level upper limits on the integral flux of sol
 ar neutrons above \n100 MeV were obtained\, assuming a power-law index of 
  the energy spectrum is\n-3\,-4 and -5. The derived upper limits are compa
 red with integral fluxes of solar\nneutrons obtained by past observations 
 using other neutron monitors as well as\nsatellites.\n\nhttps://indico.nuc
 leares.unam.mx/event/4/session/8/contribution/664
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/8/contribution/664
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