3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Contribution Poster (WITHDRAWN)

What did the relativistic solar neutrons occurrence in 2003 October 28 GLE event mean?

Speakers

  • Prof. Gui-Ming LE

Primary authors

  • Prof. Gui-Ming LE (National Center for Spaceweather, China Meteorological Administration,Beijing, 100081,China)
  • Prof. Yu-Hua TANG (Department of Astronomy, Nanjing University, 210093, P R China)
  • Ms. Yun-Qiu TANG (National Center for Spaceweather, China Meteorological Administration,Beijing, 100081,China)

Abstract content

In this paper we make an analysis of when relativistic neutrons escaped from the sun and where the relativistic neutrons in interplanetary space decayed into relativistic protons which were observed by several neutron monitors on the ground. The occurrence of relativistic neutrons seemly supports the conclusion obtained by Miroshnichenko et al. (2005) that relativistic solar protons (RSPs) were accelerated by solar flare and the path length traveled by RSPs was about 2.2AU.