BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Detection of High-Energy Solar Neutrons and Protons by Ground Leve
 l Detectors on April 15\, 2001
DTSTART;VALUE=DATE-TIME:20070704T153000Z
DTEND;VALUE=DATE-TIME:20070704T154200Z
DTSTAMP;VALUE=DATE-TIME:20260614T222920Z
UID:indico-contribution-99@cern.ch
DESCRIPTION:Speakers: Prof. MURAKI\, Yasushi (Nagoya University)\nIn assoc
 iation with the large solar flare of April 15th 2001\, the Chacaltaya \nne
 utron monitor observed an 8.2 sigma enhancement of the counting rate \nbet
 ween 13:51 and 14:24 UT.  Since the enhancement was observed from 11 \nmin
 utes before the GLE\, solar neutrons must be involved in this enhancement.
  \n  Comparing with the Yohkoh Soft X-ray Telescope images with the observ
 ed \nparticle time profiles\, we can draw a picture on the particle accele
 ration \nmechanism as follows.   By the loop-loop collisions\, high speed 
 plasma wind is\ngenerated.  When the high speed plasma hits at another mag
 netic loop\,\nparticles inside the loop may be accelerated by the collisio
 n process within a \nfew minutes.  This may be an origin of solar cosmic r
 ays.\n\nhttps://indico.nucleares.unam.mx/event/4/session/72/contribution/9
 9
LOCATION:Merida\, Mexico Yucatan I (Fiesta Americana)
URL:https://indico.nucleares.unam.mx/event/4/session/72/contribution/99
END:VEVENT
END:VCALENDAR