Direct detection of p+, p-, e+, e-, muons, d and He.

Details Direct detection of p+, p-, e+, e-, muons, d and He. Direct detection of p+, p-, e+, e-, muons, d and He.

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995nuphs..39..182s&link_type=abstract

Nuclear Physics B - Proceedings Supplements, vol. 39, issue 1, pp. 182-190

Physics

Nuclear Physics

Cosmic Rays: Balloons, Cosmic Rays: Methods Of Observation, Cosmic Rays: Detectors

Scientific paper

The author reports on the main results of the present balloon program in the study of the elementary particle component of CR (p+, e-, e+, p-, muons at different depths, and also deuteron and He) and on the RIM (Russian-Italian Mission) program on Resource satellites. The author describes the characteristics and expected performance of the three flights foreseen for the RIM program: the NINA experiment (already approved and funded by INFN in Italy and by MEPhI and VNIIEM in Moscow) mainly dedicated to the anomalous component of CR, the PAMELA experiment studying the antimatter component of CR and the R&D for the GILDA experiment to explore the high energy gamma ray sources.

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