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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>
 <room></room>
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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>
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  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <track>SH.3.6</track>
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  <name>Oral</name>
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 <title>Status of a calibration neutron monitor experiment</title>
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   <title>Prof.</title>
   <name first="Harm" middle="" last="Moraal"></name>
   <organization>NWU, Potchefstroom, South Africa</organization>
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   <title>Dr.</title>
   <name first="Helena" middle="" last="Kruger"></name>
   <organization>NWU, Potchefstroom, South Africa</organization>
   <emailHash>e222bc15a9959a57149619b059fcbb8a</emailHash>
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   <title>Prof.</title>
   <name first="Harm" middle="" last="Moraal"></name>
   <organization>NWU, Potchefstroom, South Africa</organization>
   <emailHash>1e5383192ab41daaf044b1ea14bce5e6</emailHash>
  </user>
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   <title></title>
   <name first="John" middle="" last="Bieber"></name>
   <organization>Bartol Research Institute, University of Delaware</organization>
   <emailHash>43dee64fa876834c163abdcfdbd00e34</emailHash>
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   <title></title>
   <name first="John" middle="" last="Clem"></name>
   <organization>Bartol Research Institute, University of Delaware</organization>
   <emailHash>a285e18d1f61d8ca7d92d95ab0db885c</emailHash>
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   <title>Prof.</title>
   <name first="Paul" middle="" last="Evenson"></name>
   <organization>Bartol Research Institute, University of Delaware</organization>
   <emailHash>a490c98c4472281f9923e1ecac513fb4</emailHash>
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   <title></title>
   <name first="Roger" middle="" last="Pyle"></name>
   <organization>Bartol Research Institute, University of Delaware</organization>
   <emailHash>a215516648dc2ed7a75b6192b5600d70</emailHash>
  </user>
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   <title></title>
   <name first="Marc" middle="" last="Duldig"></name>
   <organization>Australian Antarctic Division, Tasmania, Australia</organization>
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  <user>
   <title></title>
   <name first="John" middle="" last="Humble"></name>
   <organization>University of Tasmania, Australia</organization>
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 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan I (Fiesta Americana)</room>
 </location>
 <startDate>2007-07-07T11:18:00</startDate>
 <endDate>2007-07-07T11:30:00</endDate>
 <duration>00:12</duration>
 <abstract>At the previous ICRC, Kruger et al. 2005, Proc. 29th ICRC, Pune, 2, 473, and 2, 
477, reported on the first tests of two newly constructed calibration neutron 
monitors. These monitors are designed to provide an intercalibration between the 50-
odd neutron monitors around the world, so that rigidity spectra can be calculated 
from them. In those papers we described the difference in the latitudinal (energy) 
dependence between the calibrator and a standard 3NM64 neutron monitor. We also 
reported on a larger than expected instrumental temperature effect on the 
calibrator, being 0.12%/ degree C. Here we summarize these results and report on 
new experiments on the sensitivity of the calibrator to its environment, in 
particular to different ground surfaces. These surface effects have to be 
eliminated in the calibration procedure for the stationary neutron monitors.</abstract>
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