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Measurements of Cosmic-ray Low-energy Antiproton and Proton Spectra in a Transient Period of the Solar Field Reversal
Preprint
Y. Asaoka ,
Y. Shikaze ,
K. Abe ,
K. Anraku ,
M. Fujikawa ,
H. Fuke ,
S. Haino ,
M. Imori ,
K. Izumi ,
T. Maeno ,
Y. Makida ,
S. Matsuda ,
N. Matsui ,
T. Matsukawa ,
H. Matsumoto ,
H. Matsunaga ,
J. Mitchell ,
T. Mitsui ,
A. Moiseev ,
M. Motoki ,
J. Nishimura ,
M. Nozaki ,
S. Orito ,
J. F. Ormes ,
T. Saeki ,
T. Sanuki ,
M. Sasaki ,
E. S. Seo ,
T. Sonoda ,
R. Streitmatter ,
J. Suzuki ,
K. Tanaka ,
K. Tanizaki ,
I. Ueda ,
J. Z. Wang ,
Y. Yajima ,
Y. Yamagami ,
A. Yamamoto ,
Y. Yamamoto ,
K. Yamato ,
T. Yoshida ,
K. Yoshimura
02 September 2001
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Abstract
The energy spectra of cosmic-ray low-energy antiprotons and protons have been measured by BESS in 1999 and 2000, during a period covering the solar magnetic field reversal. Based on these measurements, a sudden increase of the antiproton to proton flux ratio following the solar magnetic field reversal was observed, and it generally agrees with a drift model of the solar modulation.
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Most cited references21
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Effects of drift on the transport of cosmic rays. IV - Modulation by a wavy interplanetary current sheet
J. Jokipii, B. Thomas (1981)
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- Abstract: not found
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Solar modulation of galactic cosmic rays, 2
L. Fisk (1971)
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- Abstract: not found
- Article: not found
Toward a Realistic Diffusion Tensor for Galactic Cosmic Rays
R A Burger, M. Hattingh (1998)
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