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The space experiment PAMELA

Boezio, M. (author)
Bonvicini, V. (author)
Mocchiutti, E. (author)
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Schiavon, P. (author)
Vacchi, A. (author)
Carlson, Per (author)
KTH,Fysik
Lund, Jens (author)
KTH,Fysik
Lundquist, Johan (author)
KTH,Fysik
Pearce, Mark (author)
KTH,Fysik
al, et (author)
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 (creator_code:org_t)
Elsevier BV, 2004
2004
English.
In: Nuclear Physics B - Proceedings Supplements. - : Elsevier BV. ; , s. 39-46
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • We present in this paper a status report of the space experiment PAMELA. PAMELA is a satellite-borne experiment which primarily aims to measure the antiproton and positron spectra in the cosmic radiation over a large energy range (from 80 MeV up to 190 GeV for antiprotons and from 50 MeV up to 270 GeV for positrons) and to search for antinuclei with a sensitivity of the order of 10(-8) in the antihelium/ helium ratio. In addition, it will measure the light nucleax component of cosmic rays and investigate phenomena connected with Solar and Earth physics. The apparatus will be installed onboard the polar orbiting Resurs DK1 satellite, which will be launched into space by a Soyuz TM2 rocket in 2004 from Baikonur cosmodrome in Kazakhstan, for a 3 year long mission. PAMELA consists of: a time of flight system, a transition radiation detector, a magnetic spectrometer, an anticoincidence detector, an electromagnetic imaging calorimeter, a shower tail catcher scintillator and a neutron detector.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

cosmic-ray electrons
solar minimum activity
magnetic spectrometer
imaging calorimeter
antiproton spectrum
positrons
flux
radiation
ratio
orbit

Publication and Content Type

ref (subject category)
kon (subject category)

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