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Title:	Search for neutrino induced cascades with the AMANDA detector
Abstract:	Physical review D 67, 012003 (2003)
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Handle:	Document-17251
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Friday, October 14, 2005 02:34:04 PM CDT
Modified Date:	Tuesday, April 3, 2007 05:49:17 PM CDT
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Abstract:	Hadronic cascades have a light yield about 20% lower @12#. These procedures are described in more detail elsewhere @17,18#. This procedure is quite similar to the algorithms used for muon fitting @17#. This background has been simulated with the CORSIKA program @22# using the average winter air density profile at the South Pole and the QGSJET hadronic model @23# option. The cosmic-ray composition is taken from @24#. The propagation of muons through ice is simulated with the program MUDEDX @25,26#.
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Appears In:	2004
Preferred Version:	Search for neutrino induced cascades with the AMANDA detector