Measurement of cosmic ray H and He isotopes in a Balloon Borne Experiment with a Superconducting Solenoid Spectrometer

The Balloon Borne Experiment with a Superconducting Solenoid Spectrometer (BESS) was flown annually in 1993, 1994, and 1995. In this report we present the energy spectra and isotopic composition of cosmic ray H and He measured from the 1993 flight. The low energy fluxes of H and He agree with the IM...

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Veröffentlicht in:Advances in space research 1997-01, Vol.19 (5), p.751-754
Hauptverfasser: Seo, E.S, Matsunaga, H, Anraku, K, Imori, M, Makida, Y, Matsumoto, H, McDonald, F.B, Mitchell, J, Moiseev, A, Motoki, M, Nishimura, J, Nozaki, M, Orito, S, Ormes, J.F, Otoba, M, Saeki, T, Sanuki, T, Streitmatter, R.E, Suzuki, J, Tanaka, K, Ueda, I, Wang, J.Z, Yajima, N, Yamagami, T, Yamamoto, A, Yoshida, T, Yoshimura, K
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Sprache:eng
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Zusammenfassung:The Balloon Borne Experiment with a Superconducting Solenoid Spectrometer (BESS) was flown annually in 1993, 1994, and 1995. In this report we present the energy spectra and isotopic composition of cosmic ray H and He measured from the 1993 flight. The low energy fluxes of H and He agree with the IMP-8 satellite data for a 26 day period (7/14/93 – 8/9/93) that overlapped the BESS flight. Both 2H and 3He were well separated from 1H and 4He. The measured spectra were corrected for the atmospheric overburden and compared with the interstellar/heliospheric propagation calculations.
ISSN:0273-1177
1879-1948
DOI:10.1016/S0273-1177(96)00140-8