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SUMMARY:Trapped positrons and electrons observed by  PAMELA experment
DTSTART;VALUE=DATE-TIME:20151009T054000Z
DTEND;VALUE=DATE-TIME:20151009T060500Z
DTSTAMP;VALUE=DATE-TIME:20260306T204659Z
UID:indico-contribution-436@cern.ch
DESCRIPTION:Speakers: Vladimir Mikhailov (NRNU MEPHI)\nMeasurements of ele
 ctron and positron spatial distributions in energy range from 80 MeV to se
 veral GeV below the geomagnetic cutoff rigidity were carried out using the
  PAMELA magnetic spectrometer. \nThe instrument is installed on board the 
 Resurs-DK satellite which was launched June 15th 2006  on an elliptical or
 bit with the inclination 70 degrees and the altitude 350-600 km.\nThe proc
 edure of trajectories calculations in the geomagnetic filed gives a way to
 \nseparate stably trapped and short lived albedo components produced in in
 teractions of cosmic ray protons\nwith the residual atmosphere. The work p
 resents spatial distributions of trapped\, quasitrapped and short-lived al
 bedo  electrons and positrons in the near Earth space. Electron to positro
 n ratio points  out on different production mechanism of trapped and quasi
 trapped particles\n\nOn behalf of PAMELA collaboration\n\nhttps://indico.p
 article.mephi.ru/event/2/contributions/436/
LOCATION:Milan Hotel 4* Verdi&Bellini
URL:https://indico.particle.mephi.ru/event/2/contributions/436/
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