The PAMELA experiment is being conducted aboard the Russian satellite Resurs-DK 1, which was launched into a near-Earth circumpolar orbit on June 15, 2006. The instrument, which includes a magnetic spectrometer and an electromagnetic calorimeter (16X 0), allows us to measure the fluxes of cosmic-ray electrons and positrons over a wide range of energies from ∼100 MeV to hundreds of GeV. This work presents the measurement data collected from July 2006 through January 2010 on the spectra of primary cosmic-ray electrons and positrons. At low energies, this spectrum is in good agreement with a diffusion model that includes reacceleration and damping. At high energies, the measured spectrum is harder than the one predicted

Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment / V. V. Mikhailov, O. Adriani, G. A. Bazilevskaya, G. C. Barbarino, R. Belotti, E. A. Bogomolov, M. Boezio, V. Bonvicini, M. Bongi, L. Bonechi, S. Bottai, A. Bruno, A. Vacchi, E. Vannuccini, G. I. Vasilyev, S. A. Voronov, J. Wu, A. M. Galper, L. A. Grishantseva, C. Santis, et al.. - In: BULLETIN OF THE RUSSIAN ACADEMY OF SCIENCES. PHYSICS. - ISSN 1062-8738. - STAMPA. - 77:(2013), pp. 1309-1311. [10.3103/S1062873813110221]

Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment

ADRIANI, OSCAR;BONGI, MASSIMO;BONECHI, LORENZO;MORI, NICOLA;
2013

Abstract

The PAMELA experiment is being conducted aboard the Russian satellite Resurs-DK 1, which was launched into a near-Earth circumpolar orbit on June 15, 2006. The instrument, which includes a magnetic spectrometer and an electromagnetic calorimeter (16X 0), allows us to measure the fluxes of cosmic-ray electrons and positrons over a wide range of energies from ∼100 MeV to hundreds of GeV. This work presents the measurement data collected from July 2006 through January 2010 on the spectra of primary cosmic-ray electrons and positrons. At low energies, this spectrum is in good agreement with a diffusion model that includes reacceleration and damping. At high energies, the measured spectrum is harder than the one predicted
2013
77
1309
1311
V. V. Mikhailov;O. Adriani;G. A. Bazilevskaya;G. C. Barbarino;R. Belotti;E. A. Bogomolov;M. Boezio;V. Bonvicini;M. Bongi;L. Bonechi;S. Bott...espandi
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in FLORE sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/866193
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 2
  • ???jsp.display-item.citation.isi??? ND
social impact