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<announcer>
 <user>
  <title></title>
  <name first="Admin" middle="" last="Indico"></name>
  <organization>ICN-UNAM</organization>
  <emailHash>1482bc95ee34f0461176da21871284c8</emailHash>
  <userid>3</userid>
 </user>
</announcer>
<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>
 </user>
</chair>
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 <track>SH.3.6</track>
 <type>
  <id>0</id>
  <name>Oral</name>
 </type>
 <title>Burst profile of lightning generated neutrons detected by Gulmarg Lead-free Neutron Monitor</title>
 <speakers>
  <user>
   <title>Dr.</title>
   <name first="G. N." middle="" last="SHAH"></name>
   <organization>BHABHA ATOMIC RESEARCH CENTRE</organization>
   <emailHash>f3e51ba58d8b68ff7faa14ae7bafdfea</emailHash>
  </user>
 </speakers>
 <primaryAuthors>
  <user>
   <title>Dr.</title>
   <name first="G. N." middle="" last="SHAH"></name>
   <organization>BHABHA ATOMIC RESEARCH CENTRE</organization>
   <emailHash>f3e51ba58d8b68ff7faa14ae7bafdfea</emailHash>
  </user>
 </primaryAuthors>
 <coAuthors>
  <user>
   <title></title>
   <name first="P. M." middle="" last="Ishtiaq"></name>
   <organization>BHABHA ATOMIC RESEARCH CENTRE</organization>
   <emailHash>3c16e6ce20437ee2d2e9500d381352de</emailHash>
  </user>
  <user>
   <title></title>
   <name first="S." middle="" last="Mufti"></name>
   <organization>BHABHA ATOMIC RESEARCH CENTRE</organization>
   <emailHash>36f28f3ec6a3022a1dfb7527aa7b9307</emailHash>
  </user>
  <user>
   <title></title>
   <name first="M. A." middle="" last="Darzi"></name>
   <organization>BHABHA ATOMIC RESEARCH CENTRE</organization>
   <emailHash>984e6ce9b5a6fbc403d7ac28a32e054d</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan I (Fiesta Americana)</room>
 </location>
 <duration>00:12</duration>
 <abstract>Lead-free Neutron Monitor operating at High Altitude Research Laboratory, Gulmarg has
been utilized to detect MeV energy neutron bursts produced in the lightning discharge
channels. The experiment provided the first experimental evidence of neutron
production in the lightning discharges. The neutrons were recorded in predetermined
time interval of 320 microseconds  after the detection of the first neutron in
successive time bins of 80-microseconds each. The time-delay between the sensing of 
electric field change associated with lightning discharges and detection of first
neutron from the production site would relate to the distance of the neutron
production site. However, the system was not capable of recording the profile of the
neutron bursts and was not able to identify the specific stroke responsible for the
production of these neutrons in a multi-stroke lightning discharge. To overcome these
limitations the electronic circuitry of the system was redesigned. The modified
system has the  provision of  recording neutron burst profile in time range of 315
microseconds to 4.41 milliseconds in sixty three sucessive time bins with each bin
adjustable from 5 microseconds to 70 microseconds. The new system has sucessfully
detected several major neutron burst events after the initiation of  the
lightnings in the vicinity of the detector. Burst profiles of these neutron will be
presented and discussed in relation to the propagation characteristics of these
neutrons and their mode of production in the lightning channels.</abstract>
</contribution>
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 <title>More information about the venue</title>
 <description></description>
 <type></type>
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   <name>http://www.icrc2007.unam.mx/</name>
   <type>link</type>
   <url>http://www.icrc2007.unam.mx/</url>
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