Measurements of cosmic-ray low-energy antiproton and proton spectra in a transient period of solar field reversal

被引：153

作者：

Asaoka, Y ^{[1
]}

Shikaze, Y

Abe, K

Anraku, K

Fujikawa, M

Fuke, H

Haino, S

Imori, M

Izumi, K

Maeno, T

Makida, Y

Matsuda, S

Matsui, N

Matsukawa, T

Matsumoto, H

Matsunaga, H

Mitchell, J

Mitsui, T

Moiseev, A

Motoki, M

Nishimura, J

Nozaki, M

Orito, S

Ormes, JF

Saeki, T

Sanuki, T

Sasaki, M

Seo, ES

Sonoda, T

Streitmatter, R

Suzuki, J

Tanaka, K

Tanizaki, K

Ueda, I

Wang, JZ

Yajima, Y

Yamagami, Y

Yamamoto, A

Yamamoto, Y

Yamato, K

Yoshida, T

Yoshimura, K

机构：

[1] Univ Tokyo, Tokyo 1130033, Japan

[2] Kobe Univ, Kobe, Hyogo 6578501, Japan

[3] High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan

[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[5] Univ Maryland, College Pk, MD 20742 USA

[6] Inst Space & Astronaut Sci, Kanagawa 2298510, Japan

来源：

PHYSICAL REVIEW LETTERS | 2002年 / 88卷 / 05期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevLett.88.051101

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The energy spectra of cosmic-ray low-energy antiprotons ((p) over bar 's) and protons (p's) have been measured by BESS in 1999 and 2000, during a period covering reversal at the solar magnetic field. Based an these measurements, a sudden increase of the (p) over bar /p flux ratio following the solar magnetic field reversal was observed, and it generally agrees with a drift model of the solar modulation.

引用

页码：511011 / 511014

页数：4

共 33 条

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