Relative Nuclear Abundances Measurements Inside Mir and ISS with Sileye-2 and Sileye-3 Experiments

Details Relative Nuclear Abundances Measurements Inside Mir and ISS with Sileye-2 and Sileye-3 Experiments Relative Nuclear Abundances Measurements Inside Mir and ISS with Sileye-2 and Sileye-3 Experiments

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.4245c&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

In this work we present measurements of cosmic ray nuclear abundances above 100 MeV/n inside Mir and the International Space Station (ISS). Observations inside Mir Space Station were performed with SilEye-2 experiment, a 6 plane silicon strip detector telescope designed to measure environmental radiation and investigate on the Light Flash (LF) phenomenon. A total of 100 sessions comprising more than 1000 hours of observation was performed in the years 19982000. ISS data have been taken in 2002 with Sileye-3/Alteino (an 8 plane, 32 strip silicon detector) device during the Soyuz-34 flight. We report on SilEye-3/Alteino relative abundances from Boron to Silicon measured in Pirs module of ISS and on the comparison with Sileye-2 results.

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