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The PAMELA space experiment: first year of operation
by
Boezio, M
, Collaboration, the PAMELA
in
Anticoincidence systems
/ Antiparticles
/ Antiprotons
/ Charged particle identification
/ Charged particles
/ Cosmic ray antiprotons
/ Cosmic rays
/ Cosmology
/ Dark matter
/ Electromagnetic calorimeter
/ High energy physics
/ Launching facilities
/ Magnetic spectrometers
/ Neutron counters
/ Neutrons
/ Physics
/ Scintillation counters
/ Silicon
/ Silicon micro-strip
/ Space experiments
/ Time of flight systems
2008
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The PAMELA space experiment: first year of operation
by
Boezio, M
, Collaboration, the PAMELA
in
Anticoincidence systems
/ Antiparticles
/ Antiprotons
/ Charged particle identification
/ Charged particles
/ Cosmic ray antiprotons
/ Cosmic rays
/ Cosmology
/ Dark matter
/ Electromagnetic calorimeter
/ High energy physics
/ Launching facilities
/ Magnetic spectrometers
/ Neutron counters
/ Neutrons
/ Physics
/ Scintillation counters
/ Silicon
/ Silicon micro-strip
/ Space experiments
/ Time of flight systems
2008
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Do you wish to request the book?
The PAMELA space experiment: first year of operation
by
Boezio, M
, Collaboration, the PAMELA
in
Anticoincidence systems
/ Antiparticles
/ Antiprotons
/ Charged particle identification
/ Charged particles
/ Cosmic ray antiprotons
/ Cosmic rays
/ Cosmology
/ Dark matter
/ Electromagnetic calorimeter
/ High energy physics
/ Launching facilities
/ Magnetic spectrometers
/ Neutron counters
/ Neutrons
/ Physics
/ Scintillation counters
/ Silicon
/ Silicon micro-strip
/ Space experiments
/ Time of flight systems
2008
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Journal Article
The PAMELA space experiment: first year of operation
2008
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Overview
On the 15th of June 2006 the PAMELA experiment, mounted on the Resurs DK1 satellite, was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. PAMELA is a satellite-borne apparatus designed to study charged particles in the cosmic radiation, to investigate the nature of dark matter, measuring the cosmic-ray antiproton and positron spectra over the largest energy range ever achieved, and to search for antinuclei with unprecedented sensitivity. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. The combination of these devices allows charged particle identification over a wide energy range.
Publisher
IOP Publishing
Subject
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