Measurement of the total spectrum of electrons and positrons in the energy range of 300–1500 GeV in the PAMELA experiment with the aid of a sampling calorimeter and a neutron detector
Journal Article
·
· Physics of Atomic Nuclei
- National Research Nuclear University MEPhI (Russian Federation)
A method based on the use of a sampling calorimeter was developed for measuring the total energy spectrum of electrons and positrons from high-energy cosmic rays in the PAMELA satellite-borne experiment. This made it possible to extend the range of energies accessible to measurements by the magnetic system of the PAMELA spectrometer. Themethod involves a procedure for selecting electrons on the basis of features of a secondary-particle shower in the calorimeter. The results obtained by measuring the total spectrum of cosmic-ray electrons and positrons in the energy range of 300–1500 GeV by the method in question are presented on the basis of data accumulated over a period spanning 2006 and 2013.
- OSTI ID:
- 22472344
- Journal Information:
- Physics of Atomic Nuclei, Vol. 78, Issue 2; Other Information: Copyright (c) 2015 Pleiades Publishing, Ltd.; Country of input: International Atomic Energy Agency (IAEA); ISSN 1063-7788
- Country of Publication:
- United States
- Language:
- English
Similar Records
Dark Matter Research and the PAMELA Space Mission
Separation of the electron and proton cosmic-ray components by means of a calorimeter in the PAMELA satellite-borne experiment for the case of particle detection within a large aperture
The PAMELA electromagnetic calorimeter: performances
Journal Article
·
Tue Sep 08 00:00:00 EDT 2009
· AIP Conference Proceedings
·
OSTI ID:22472344
+17 more
Separation of the electron and proton cosmic-ray components by means of a calorimeter in the PAMELA satellite-borne experiment for the case of particle detection within a large aperture
Journal Article
·
Sat Jun 15 00:00:00 EDT 2013
· Physics of Atomic Nuclei
·
OSTI ID:22472344
The PAMELA electromagnetic calorimeter: performances
Journal Article
·
Fri Oct 27 00:00:00 EDT 2006
· AIP Conference Proceedings
·
OSTI ID:22472344
+7 more