Speaker
Dr.
Vladimir Mikhailov
(NRNU MEPHI)
Description
Magnetic spectrometer PAMELA was launched onboard a satellite Resurs-DK1
into low-Earth polar orbit with altitude 350-600 km to the study cosmic ray antiparticle fluxes in a wide energy range from ~ 100 MeV to hundreds GeV. This paper presents the results of observations of temporal variations of the positron and electron fluxes in the 2006-2015. The ratio of the positron and electron fluxes below 2 GV shows sharp increasing since 2014 due to changing of the polarity of the solar magnetic field.
Primary author
Dr.
Vladimir Mikhailov
(NRNU MEPHI)
