Measurements of quasi-trapped electron and positron fluxes with PAMELA

Details Measurements of quasi-trapped electron and positron fluxes with PAMELA Measurements of quasi-trapped electron and positron fluxes with PAMELA

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jgra..11412218a&link_type=abstract

Journal of Geophysical Research, Volume 114, Issue A12, CiteID A12218

Physics

2

Magnetospheric Physics: Energetic Particles: Trapped, Magnetospheric Physics: Magnetosphere: Inner, Space Weather: Space Radiation Environment, Magnetospheric Physics: Radiation Belts

Scientific paper

This paper presents precise measurements of the differential energy spectra of quasi-trapped secondary electrons and positrons and their ratio between 80 MeV and 10 GeV in the near-equatorial region (altitudes between 350 km and 600 km). Latitudinal dependences of the spectra are analyzed in detail. The results were obtained from July until November 2006 onboard the Resurs-DK satellite by the PAMELA spectrometer, a general purpose cosmic ray detector system built around a permanent magnet spectrometer and a silicon-tungsten calorimeter.

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