Precise measurement of cosmic-ray proton and helium spectra with the BEES spectrometer

T. Sanuki; M. Motoki; H. Matsumoto; E. S. Seo; J. Z. Wang; K. Abe; K. Anraku; Y. Asaoka; M. Fujikawa; M. Imori; T. Maeno; Y. Makida; N. Matsui; H. Matsunaga; J. Mitchell; T. Mitsui; A. Moiseev; J. Nishimura; M. Nozaki; S. Orito; J. Ormes; T. Saeki; M. Sasaki; Y. Shikaze; T. Sonoda; R. Streitmatter; J. Suzuki; K. Tanaka; I. Ueda; N. Yajima; T. Yamagami; A. Yamamoto; T. Yoshida; K. Yoshimura

doi:10.1086/317873

Precise measurement of cosmic-ray proton and helium spectra with the BEES spectrometer

T. Sanuki, M. Motoki, H. Matsumoto, E. S. Seo, J. Z. Wang, K. Abe, K. Anraku, Y. Asaoka, M. Fujikawa, M. Imori, T. Maeno, Y. Makida, N. Matsui, H. Matsunaga, J. Mitchell, T. Mitsui, A. Moiseev, J. Nishimura, M. Nozaki, S. OritoJ. Ormes, T. Saeki, M. Sasaki, Y. Shikaze, T. Sonoda, R. Streitmatter, J. Suzuki, K. Tanaka, I. Ueda, N. Yajima, T. Yamagami, A. Yamamoto, T. Yoshida, K. Yoshimura

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307 Citations (Scopus)

Abstract

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.

Original language	English
Pages (from-to)	1135-1142
Number of pages	8
Journal	Astrophysical Journal
Volume	545
Issue number	2 PART 1
DOIs	https://doi.org/10.1086/317873
Publication status	Published - Dec 20 2000
Externally published	Yes

Keywords

Cosmic rays
Elementary particles

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/317873

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Sanuki, T., Motoki, M., Matsumoto, H., Seo, E. S., Wang, J. Z., Abe, K., Anraku, K., Asaoka, Y., Fujikawa, M., Imori, M., Maeno, T., Makida, Y., Matsui, N., Matsunaga, H., Mitchell, J., Mitsui, T., Moiseev, A., Nishimura, J., Nozaki, M., ... Yoshimura, K. (2000). Precise measurement of cosmic-ray proton and helium spectra with the BEES spectrometer. Astrophysical Journal, 545(2 PART 1), 1135-1142. https://doi.org/10.1086/317873

Sanuki, T, Motoki, M, Matsumoto, H, Seo, ES, Wang, JZ, Abe, K, Anraku, K, Asaoka, Y, Fujikawa, M, Imori, M, Maeno, T, Makida, Y, Matsui, N, Matsunaga, H, Mitchell, J, Mitsui, T, Moiseev, A, Nishimura, J, Nozaki, M, Orito, S, Ormes, J, Saeki, T, Sasaki, M, Shikaze, Y, Sonoda, T, Streitmatter, R, Suzuki, J, Tanaka, K, Ueda, I, Yajima, N, Yamagami, T, Yamamoto, A, Yoshida, T & Yoshimura, K 2000, 'Precise measurement of cosmic-ray proton and helium spectra with the BEES spectrometer', Astrophysical Journal, vol. 545, no. 2 PART 1, pp. 1135-1142. https://doi.org/10.1086/317873

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abstract = "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.",

keywords = "Cosmic rays, Elementary particles",

author = "T. Sanuki and M. Motoki and H. Matsumoto and Seo, {E. S.} and Wang, {J. Z.} and K. Abe and K. Anraku and Y. Asaoka and M. Fujikawa and M. Imori and T. Maeno and Y. Makida and N. Matsui and H. Matsunaga and J. Mitchell and T. Mitsui and A. Moiseev and J. Nishimura and M. Nozaki and S. Orito and J. Ormes and T. Saeki and M. Sasaki and Y. Shikaze and T. Sonoda and R. Streitmatter and J. Suzuki and K. Tanaka and I. Ueda and N. Yajima and T. Yamagami and A. Yamamoto and T. Yoshida and K. Yoshimura",

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T1 - Precise measurement of cosmic-ray proton and helium spectra with the BEES spectrometer

AU - Sanuki, T.

AU - Motoki, M.

AU - Matsumoto, H.

AU - Seo, E. S.

AU - Wang, J. Z.

AU - Abe, K.

AU - Anraku, K.

AU - Asaoka, Y.

AU - Fujikawa, M.

AU - Imori, M.

AU - Maeno, T.

AU - Makida, Y.

AU - Matsui, N.

AU - Matsunaga, H.

AU - Mitchell, J.

AU - Mitsui, T.

AU - Moiseev, A.

AU - Nishimura, J.

AU - Nozaki, M.

AU - Orito, S.

AU - Ormes, J.

AU - Saeki, T.

AU - Sasaki, M.

AU - Shikaze, Y.

AU - Sonoda, T.

AU - Streitmatter, R.

AU - Suzuki, J.

AU - Tanaka, K.

AU - Ueda, I.

AU - Yajima, N.

AU - Yamagami, T.

AU - Yamamoto, A.

AU - Yoshida, T.

AU - Yoshimura, K.

PY - 2000/12/20

Y1 - 2000/12/20

N2 - 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.

AB - 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.

KW - Cosmic rays

KW - Elementary particles

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U2 - 10.1086/317873

DO - 10.1086/317873

M3 - Article

AN - SCOPUS:0042268859

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SP - 1135

EP - 1142

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 PART 1

ER -

Precise measurement of cosmic-ray proton and helium spectra with the BEES spectrometer

Abstract

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