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<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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 <title>The possible acceleration source of solar relativistic particles on 13 December 2006</title>
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   <name first="Chuan" middle="" last="Li"></name>
   <organization>Department of Astronomy, Nanjing University and IAS, batiment 121, Paris XI University</organization>
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   <name first="Chuan" middle="" last="Li"></name>
   <organization>Department of Astronomy, Nanjing University and IAS, batiment 121, Paris XI University</organization>
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 <abstract>In large solar energetic particle (SEP) event, the acceleration source of 
relativistic particles remains enigmatic. The main controversy focuses on 
acceleration occurring at shock driven by coronal mass ejections (CMEs) or in 
the active region producing flares. The ground level enhancement (GLE) event 
of 2006 December 13 offers excellent opportunity to extend our knowledge 
about the acceleration and transport process of solar energetic particles. From 
analysis of imaging data from TRACE, SOHO, and RHESSI, along with the data 
from neutron monitors, we find good correlation between the flare's eruptions 
and relativistic particles count rate. Moreover, the flare occurred almost at the 
well-connected region, it suggests that the main acceleration process probably 
occurred in the flare active region.</abstract>
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