Light Isotope Abundances in Solar Energetic Particles Measured by the NINA-2 Instrument

Details Light Isotope Abundances in Solar Energetic Particles Measured by the NINA-2 Instrument Light Isotope Abundances in Solar Energetic Particles Measured by the NINA-2 Instrument

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3249m&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

The instrument NINA-2 flew on board the satellite MITA between July 2000 and August 2001, in circular polar orbit. This paper reports about a set of Solar Energetic Particle events measured by the NINA-2 instrument. The detector has mass resolution of about 0.15 amu for light nuclei and gives the possibility to observe hydrogen and helium isotop es in the energy range 10-50 MeV/n. Data of 3 He and 4 He were used to determine the 3 He/4 He ratio. For each event the deuterium-to-proton ratio was also estimated. This ratio, averaged over all events, is less than 3×10-5 .

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