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Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight

Authors :
Abe, K.
Fuke, H.
Haino, S.
Hams, T.
Itazaki, A.
Kim, K. C.
Kumazawa, T.
Lee, M. H.
Makida, Y.
Matsuda, S.
Matsumoto, K.
Mitchell, J. W.
Moiseev, A. A.
Myers, Z.
Nishimura, J.
Nozaki, M.
Orito, R.
Ormes, J. F.
Sasaki, M.
Seo, E. S.
Shikaze, Y.
Streitmatter, R. E.
Suzuki, J.
Takasugi, Y.
Takeuchi, K.
Tanaka, K.
Yamagami, T.
Yamamoto, A.
Yoshida, T.
Yoshimura, K.
Abe, K.
Fuke, H.
Haino, S.
Hams, T.
Itazaki, A.
Kim, K. C.
Kumazawa, T.
Lee, M. H.
Makida, Y.
Matsuda, S.
Matsumoto, K.
Mitchell, J. W.
Moiseev, A. A.
Myers, Z.
Nishimura, J.
Nozaki, M.
Orito, R.
Ormes, J. F.
Sasaki, M.
Seo, E. S.
Shikaze, Y.
Streitmatter, R. E.
Suzuki, J.
Takasugi, Y.
Takeuchi, K.
Tanaka, K.
Yamagami, T.
Yamamoto, A.
Yoshida, T.
Yoshimura, K.
Publication Year :
2008

Abstract

The BESS-Polar spectrometer had its first successful balloon flight over Antarctica in December 2004. During the 8.5-day long-duration flight, almost 0.9 billion events were recorded and 1,520 antiprotons were detected in the energy range 0.1-4.2 GeV. In this paper, we report the antiproton spectrum obtained, discuss the origin of cosmic-ray antiprotons, and use antiprotons to probe the effect of charge sign dependent drift in the solar modulation.<br />Comment: 18 pages, 1 table, 5 figures, submitted to Physics Letters B

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1363354745
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1016.j.physletb.2008.10.053