Precise Measurement of Cosmic-Ray Proton and Helium Spectra with the BESS Spectrometer

Precise Measurement of Cosmic-Ray Proton and Helium Spectra with the BESS Spectrometer
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DOI:
10.1086/317873
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发表时间:
2000-02
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
T. Sanuki;M. Motoki;M. Motoki;H. Matsumoto;E. Seo;J. Z. Wang;K. Abe;K. Anraku;Y. Asaoka;M. Fujikawa;M. Imori;T. Maeno;Y. Makida;N. Matsui;H. Matsunaga;H. Matsunaga;J. Mitchell;T. Mitsui;T. Mitsui;A. Moiseev;J. Nishimura;M. Nozaki;S. Orito;J. Ormes;T. Saeki;M. Sasaki;Y. Shikaze;T. Sonoda;R. Streitmatter;Junichi Suzuki;Kenichi Tanaka;I. Ueda;N. Yajima;T. Yamagami;A. Yamamoto;T. Yoshida;K. Yoshimura
T. Sanuki;M. Motoki;M. Motoki;H. Matsumoto;E. Seo;J. Z. Wang;K. Abe;K. Anraku;Y. Asaoka;M. Fujikawa;M. Imori;T. Maeno;Y. Makida;N. Matsui;H. Matsunaga;H. Matsunaga;J. Mitchell;T. Mitsui;T. Mitsui;A. Moiseev;J. Nishimura;M. Nozaki;S. Orito;J. Ormes;T. Saeki;M. Sasaki;Y. Shikaze;T. Sonoda;R. Streitmatter;Junichi Suzuki;Kenichi Tanaka;I. Ueda;N. Yajima;T. Yamagami;A. Yamamoto;T. Yoshida;K. Yoshimura
中科院分区:
其他
文献类型:
--
作者:
T. Sanuki;M. Motoki;M. Motoki;H. Matsumoto;E. Seo;J. Z. Wang;K. Abe;K. Anraku;Y. Asaoka;M. Fujikawa;M. Imori;T. Maeno;Y. Makida;N. Matsui;H. Matsunaga;H. Matsunaga;J. Mitchell;T. Mitsui;T. Mitsui;A. Moiseev;J. Nishimura;M. Nozaki;S. Orito;J. Ormes;T. Saeki;M. Sasaki;Y. Shikaze;T. Sonoda;R. Streitmatter;Junichi Suzuki;Kenichi Tanaka;I. Ueda;N. Yajima;T. Yamagami;A. Yamamoto;T. Yoshida;K. Yoshimura

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我们报告宇宙射线质子和氦谱的能量范围为1-120 GeV的核子-1和1-54 GeV的核子-1,分别由一个飞行的超导谱仪(BESS)在1998年测量的。通过对1 T均匀螺线管磁场中的圆形轨迹的高精度测量,可靠地确定了宇宙线的磁刚度。这些光谱在质子的±5%和氦核的±10%的总体不确定度内确定,包括统计和系统误差。
We report cosmic-ray proton and helium spectra in energy ranges of 1-120 GeV nucleon-1 and 1-54 GeV nucleon-1, respectively, measured by a flight of the Balloon-borne Experiment with Superconducting Spectrometer (BESS) in 1998. The magnetic rigidity of the cosmic ray was reliably determined by highly precise measurement of the circular track in a uniform solenoidal magnetic field of 1 T. Those spectra were determined within overall uncertainties of ±5% for protons and ±10% for helium nuclei including statistical and systematic errors.