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Title:	CosRay (Draft Written Version of Talk)
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Handle:	Document-57647
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Tuesday, April 5, 2011 01:42:55 PM CDT
Modified Date:	Thursday, April 7, 2011 11:35:15 AM CDT
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Abstract:	CosRay � Neutron Monitors at the South Pole Submitted by Paul Evenson, University of Delaware In contrast to the investigations that seek to extend the range of IceCube to higher energy CosRay works with IceTop to extend the energy range to lower energy (1-10 GeV) primarily to study the acceleration and transport of solar energetic particles. Neutron monitors respond to primary energies of ~1 GeV for solar cosmic rays and ~10 GeV for Galactic cosmic rays. In the figure we use this spectrum and the response function of a neutron monitor to calculate the response of a neutron monitor, shown by the heavy points. Although the NM64 response function peaks at an energy similar energy to that...
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Preferred Version:	CosRay