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SUMMARY:Magnetic Clouds: The cylindrical elliptic approach
DTSTART;VALUE=DATE-TIME:20070704T194500Z
DTEND;VALUE=DATE-TIME:20070704T194500Z
DTSTAMP;VALUE=DATE-TIME:20260312T161433Z
UID:indico-contribution-1309@cern.ch
DESCRIPTION:Speakers: Dr. MALANDRAKI\, Olga (Research and Scientific Suppo
 rt Department of ESA ESTEC\, Noordwijk)\nMagnetic clouds\, as subsets of I
 nterplanetary Coronal Mass Ejections\, are\nmodulating the interplanetary 
 space. We present six observed magnetic clouds\nand simulate them accordin
 g to the circular and the new elliptic cylindrical\nmodels. Both models co
 rrespond to magnetic clouds attached to the sun and \nthe \nsimulations es
 timate the characteristics of the clouds\, such\nprobable shapes\, orienta
 tion of their axis\, duration\, etc. In general\,\nmagnetic clouds can be 
 described by closed (attached) cylindrical models\,\nbut with an elliptic 
 rather than circular cylindrical shape.\n\n(This presentation is supported
  by the Greek-Czech Bilateral Cooperation).\n\nhttps://indico.nucleares.un
 am.mx/event/4/session/8/contribution/1309
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/8/contribution/1309
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