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Search for neutrino induced cascades with the AMANDA detector
Physical review D 67, 012003 (2003)
Handle: Document-17251
Owner: Site Administrator (User-2, admin:DocuShare)DS
Friday, October 14, 2005 02:34:04 PM CDT
Tuesday, April 3, 2007 05:49:17 PM CDT
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  • 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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