Title of article
Cosmic-ray observations of the heliosphere with the PAMELA experiment Original Research Article
Author/Authors
M. Casolino، نويسنده , , F. Altamura، نويسنده , , A. Basili، نويسنده , , R. Bencardino، نويسنده , , M.P. De Pascale، نويسنده , , L. Marcelli، نويسنده , , M. Minori، نويسنده , , A. Morselli، نويسنده , , M. Nagni، نويسنده , , P. Picozza، نويسنده , , S. Russo، نويسنده , , R. Sparvoli، نويسنده , , M. Ambriola، نويسنده , , R. Bellotti، نويسنده , , F.S. Cafagna، نويسنده , , M. Circella، نويسنده , , C. De Marzo، نويسنده , , N. Giglietto، نويسنده , , N. Mirizzi، نويسنده , , M. Romita، نويسنده , , e، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2006
Pages
5
From page
1848
To page
1852
Abstract
The PAMELA experiment is a multi-purpose apparatus built around a permanent magnet spectrometer, with the main goal of studying in detail the antiparticle component of cosmic rays. The apparatus will be carried in space by means of a Russian satellite, due to launch in 2005, for a three year-long mission. The characteristics of the detectors composing the instrument, alongside the long lifetime of the mission and the orbital characteristics of the satellite, will allow to address several items of cosmic-ray physics. In this paper, we will focus on the solar and heliospheric observation capabilities of PAMELA.
Keywords
Cosmic rays , Satellite-borne experiment , Solar wind , Solar energetic particles , Jovian particles
Journal title
Advances in Space Research
Serial Year
2006
Journal title
Advances in Space Research
Record number
1130878
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