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  <organization>ICN-UNAM</organization>
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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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 <board>191 (10A)</board>
 <track>SH.1.6</track>
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  <name>Poster</name>
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 <title>Magnetic Strom Associated with Energetic Particle Event of January 21, 2005</title>
 <speakers>
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   <title>Dr.</title>
   <name first="Makoto" middle="" last="Hareyama"></name>
   <organization>Advanced Research Institute for Science and Engineering, Waseda University</organization>
   <emailHash>12af7df037572ff89aa2439e5754eb8b</emailHash>
  </user>
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   <title>Dr.</title>
   <name first="Sergey" middle="" last="Kuznetsov"></name>
   <organization>Scobeltsyn Institute of Nuclear Physics, Moscow State University</organization>
   <emailHash>35a15c72bb362412eb5599b51cb7b98d</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Makoto" middle="" last="Hareyama"></name>
   <organization>Advanced Research Institute for Science and Engineering, Waseda University</organization>
   <emailHash>12af7df037572ff89aa2439e5754eb8b</emailHash>
  </user>
 </primaryAuthors>
 <coAuthors>
  <user>
   <title>Dr.</title>
   <name first="Yu" middle="" last="Denisov"></name>
   <organization>Scobeltsyn Institute of Nuclear Physics, Moscow State University</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Boris" middle="" last="Yushkov"></name>
   <organization>Scobeltsyn Institute of Nuclear Physics, Moscow State University</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Nobuyuki" middle="" last="Hasebe"></name>
   <organization>Advanced Research Institute for Science and Engineering, Waseda University</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Satoshi" middle="" last="Kodaira"></name>
   <organization>Advanced Research Institute for Science and Engineering, Waseda University</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Mr.</title>
   <name first="Naoki" middle="" last="Masuyama"></name>
   <organization>Advanced Research Institute for Science and Engineering, Waseda University</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Kunitomo" middle="" last="Sakurai"></name>
   <organization>Advanced Research Institute for Science and Engineering, Waseda University</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Masatsugu" middle="" last="Akiyama"></name>
   <organization>Institute for Unmanned Space Experiment Free Flyer</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Kazumori" middle="" last="Hama"></name>
   <organization>Institute for Unmanned Space Experiment Free Flyer</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
 </location>
 <startDate>2007-07-04T14:45:00</startDate>
 <endDate>2007-07-04T14:45:00</endDate>
 <abstract>A strong magnetic storm occurred in January 21st, 2005. During this magnetic storm,
fluxes of electrons trapped in the radiation belt were observed simultaneously with
two low altitude satellites, CORONAS-F and SERVIS-1 and some geostationary
satellites, LANLs. During under developing of the magnetic storm, both of the
velocity and the dynamic pressure of solar wind increased by two discrete steps. The
data observed from these satellites indicated the large flux variation between the
first and second increase. The flux of about 1 MeV electrons observed by LANLs
decreased at both the 1st and the 2nd increase of the solar wind parameters, while
the flux of about 1 MeV protons increased at the 1st step and then decreased at the
2nd step. However, the flux of 3.4 – 6.8 MeV electrons observed by SERVIS-1 satellite
increased after the 1st step in only outer radiation belt, but not with lower energy
ranges or other regions. Furthermore, the spatial distributions of energetic
electrons observed by SERVIS-1 and COONAS-F satellites largely changed before and
after the onset of the magnetic storm. Thus observed results will be discussed to
find out the nature and its temporal variation of energetic particles in the
magnetosphere.</abstract>
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   <name>http://www.icrc2007.unam.mx/</name>
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