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 <user>
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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>
<participants></participants>
<closed>True</closed>
<location>
 <name>Merida, Mexico</name>
 <address></address>
 <room></room>
</location>
<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>
<chair>
 <user>
  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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  <id>1</id>
  <name>Poster</name>
 </type>
 <title>Space radiation storm : associated cosmic ray intensity variation and geomagnetic effects</title>
 <speakers>
  <user>
   <title>Ms.</title>
   <name first="Sonia" middle="" last="Sharma"></name>
   <organization>School of Studies in Physics, Jiwaji University, Gwalior, M.P. 475 001, INDIA</organization>
   <emailHash>ababa05fa73a12f3217dab344e36d614</emailHash>
  </user>
 </speakers>
 <primaryAuthors>
  <user>
   <title>Ms.</title>
   <name first="Sonia" middle="" last="Sharma"></name>
   <organization>School of Studies in Physics, Jiwaji University, Gwalior, M.P. 475 001, INDIA</organization>
   <emailHash>ababa05fa73a12f3217dab344e36d614</emailHash>
  </user>
 </primaryAuthors>
 <coAuthors>
  <user>
   <title>Dr.</title>
   <name first="Subhash    Chandra" middle="" last="Kaushik"></name>
   <organization>Department of Physics, Government Autonomous (P.G.) College,  Datia  486 661 M.P. INDIA</organization>
   <emailHash>cabf00ddfe72009c282fb1714ad8d798</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <abstract>NOAA satellites and the orbiting Solar and Heliospheric observatory (SOHO) recorded
one of the most powerful solar flares of the previous solar cycle 23 on 14 July 2000.
This intense X 5 –class flare was erupted from sunspot region 9077 at 1024 UT.
Simultaneously the coronagraph on board the SOHO recorded a ‘full-halo’ coronal mass
ejection (CME) aimed toward the Earth. As CME’s are gigantic bubbles of electrified
gas carrying away as much as 10 billion tons of solar material, such a release of
solar particles produced very intense  geomagnetic disturbances and further modulates
the cosmic ray intensities.  In this study an
attempt has been made to analyze the influence of this space radiation storm on
Earth’s geomagnetic field as well as on the cosmic ray intensity variation. as
reflected b a strong Forbush decrease event.  We have used the geomagnetic indices
Dst, Ap and AE and for cosmic rays the data from Calgary NM 64 (geographic Lat. North
51.08, Long. East 245.87, cut off rigidity 1.09 GV) is used.  The study revealed that
event is well correlated with the Forbush decrease and producing significant
depressions in the geomagnetic indices.  We have obtained the encouraging results
that are discussed in the detailed paper.</abstract>
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