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  <organization>ICN-UNAM</organization>
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  <userid>3</userid>
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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<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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 <name>Merida, Mexico</name>
 <address></address>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <title>Calibrating the Milagro Instrument for Measuring Forbush Decreases</title>
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   <title>Prof.</title>
   <name first="James" middle="" last="Ryan"></name>
   <organization>University of New Hampshire</organization>
   <emailHash>4cb446044e49533035824eb31449dc1c</emailHash>
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   <title>Prof.</title>
   <name first="James" middle="" last="Ryan"></name>
   <organization>University of New Hampshire</organization>
   <emailHash>4cb446044e49533035824eb31449dc1c</emailHash>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan I (Fiesta Americana)</room>
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 <startDate>2007-07-06T09:30:00</startDate>
 <endDate>2007-07-06T09:42:00</endDate>
 <duration>00:12</duration>
 <abstract>The Milagro TeV ground-level gamma-ray telescope detects Forbush decreases
in several of its data channels.  To understand how the instrument responds
to Forbush decreases, one must calculate, through simulations, its behavior
to a changing galactic cosmic-ray background as that background is modulated
by heliospheric activity.  To this end, we have been modeling the response
of the instrument as a function of the Gleeson and Axford heliospheric
electrostatic potential.  We will present ongoing progress in modeling the
October and November 2003 Forbush decreases using several independent data
channels.  We will compare the results to the predicted response of the
Climax neutron monitor in nearby Colorado.</abstract>
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