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SUMMARY:Forbush decreases in relation to CME related shocks and solar wind
    disturbances.
DTSTART;VALUE=DATE-TIME:20070704T194500Z
DTEND;VALUE=DATE-TIME:20070704T194500Z
DTSTAMP;VALUE=DATE-TIME:20260615T114952Z
UID:indico-contribution-546@cern.ch
DESCRIPTION:Speakers: Dr. VERMA\, PL (HIGHER EDUCATION)\nForbush decreases
  in relation to CME related shocks and solar wind   \ndisturbances.\n\n \n
 \nP.L. VERMA \n \n\nDepartment of Physics Govt. Vivekanand P.G. College Ma
 ihar Distt. Satna (M.P.) \nIndia\n \nABSTRACT\n \n\nCoronal mass ejections
  (CMEs) are the most energetic events in the \nheliosphere and are widely 
 recognized as being responsible for production of \nlarge disturbances in 
 solar wind\, transient interplanetary shocks and Forbush \ndecreases in co
 smic ray intensity. I studied Forbush decreases\, recorded with \nground b
 ased monitor at Oul for the period 1997-2006 with variation in solar \nwin
 d plasma velocity\, proton density\, temperature and different types of \n
 interplanetary shocks related to ejecta and magnetic clouds which are \nin
 terplanetary manifestations of coronal mass ejections. I found a weak \npo
 sitive co-relation between magnitude of jump in solar wind velocity\, prot
 on \ndensity\, temperature and magnitude of Forbush decreases.  Further I 
 have \nconcluded that the forward shocks which are related to ejecta\, mag
 netic clouds \nor ejecta and magnetic clouds both are very much effective 
 in producing \nForbush decreases of higher magnitudes in cosmic ray intens
 ity. The results \nobtained in this study gives very important information
 s about the events \nwhich are mainly responsible for Forbush decreases.\n
 \nhttps://indico.nucleares.unam.mx/event/4/session/8/contribution/546
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/8/contribution/546
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