Cosmic ray helium isotopes from the BESS-Polar I experiment

N. Picot-Clemente; K. Abe; H. Fuke; S. Haino; T. Hams; A. Itazaki; K. C. Kim; T. Kumazawa; M. H. Lee; Y. Makida; S. Matsuda; K. Matsumoto; J. W. Mitchell; Z. Myers; J. Nishimura; M. Nozaki; R. Orito; J. F. Ormes; M. Sasaki; E. S. Seo; Y. Shikaze; R. E. Streitmatter; J. Suzuki; Y. Takasugi; K. Takeuchi; K. Tanaka; T. Yamagami; A. Yamamoto; T. Yoshida; K. Yoshimura

doi:10.7529/ICRC2011/V06/0699

Cosmic ray helium isotopes from the BESS-Polar I experiment

N. Picot-Clemente, K. Abe, H. Fuke, S. Haino, T. Hams, A. Itazaki, K. C. Kim, T. Kumazawa, M. H. Lee, Y. Makida, S. Matsuda, K. Matsumoto, J. W. Mitchell, Z. Myers, J. Nishimura, M. Nozaki, R. Orito, J. F. Ormes, M. Sasaki, E. S. SeoY. Shikaze, R. E. Streitmatter, J. Suzuki, Y. Takasugi, K. Takeuchi, K. Tanaka, T. Yamagami, A. Yamamoto, T. Yoshida, K. Yoshimura

Research output: Contribution to conference › Paper › peer-review

Abstract

The first flight of the Balloon-Borne Experiment with a Superconducting Spectrometer (BESS-Polar I) in Antarctica collected about 900 million cosmic ray events during 8.5 days in 2004. Particle charge was determined from energy loss in the scintillators, rigidity by reconstructing each particle trajectory in the magnetic field, and velocity by utilizing time of flights counters. These measurements can clearly identify hydrogen and helium isotopes among the incoming particles. These isotopes are generally believed to result from nuclear interactions of primaries with the interstellar medium. Measurement of their flux is expected to provide important information on cosmic ray sources and particle propagation in interstellar space. The presentation will focus on determination of the helium isotope flux in the kinetic energy per nucleon range 0.1 GeV/n to about 1.5 GeV/n. After quickly introducing the BESS-Polar I detector, the dedicated analysis to differentiate isotopes will be described. Finally, the energy spectra will be presented and compared to previous measurements.

Original language	English
Pages	51-54
Number of pages	4
DOIs	https://doi.org/10.7529/ICRC2011/V06/0699
Publication status	Published - 2011
Externally published	Yes
Event	32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China Duration: Aug 11 2011 → Aug 18 2011

Other

Other	32nd International Cosmic Ray Conference, ICRC 2011
Country	China
City	Beijing
Period	8/11/11 → 8/18/11

Keywords

BESS
BESS-polar I
Balloon-borne experiment
Cosmic-rays
Helium isotopes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.7529/ICRC2011/V06/0699

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Picot-Clemente, N., 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., Myers, Z., Nishimura, J., Nozaki, M., Orito, R., Ormes, J. F., Sasaki, M., ... Yoshimura, K. (2011). Cosmic ray helium isotopes from the BESS-Polar I experiment. 51-54. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China. https://doi.org/10.7529/ICRC2011/V06/0699

Cosmic ray helium isotopes from the BESS-Polar I experiment. / Picot-Clemente, N.; 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.; 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.

2011. 51-54 Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China.

Research output: Contribution to conference › Paper › peer-review

Picot-Clemente, N, Abe, K, Fuke, H, Haino, S, Hams, T, Itazaki, A, Kim, KC, Kumazawa, T, Lee, MH, Makida, Y, Matsuda, S, Matsumoto, K, Mitchell, JW, Myers, Z, Nishimura, J, Nozaki, M, Orito, R, Ormes, JF, Sasaki, M, Seo, ES, Shikaze, Y, Streitmatter, RE, Suzuki, J, Takasugi, Y, Takeuchi, K, Tanaka, K, Yamagami, T, Yamamoto, A, Yoshida, T & Yoshimura, K 2011, 'Cosmic ray helium isotopes from the BESS-Polar I experiment', Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China, 8/11/11 - 8/18/11 pp. 51-54. https://doi.org/10.7529/ICRC2011/V06/0699

Picot-Clemente, N. ; 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. ; 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. / Cosmic ray helium isotopes from the BESS-Polar I experiment. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China.4 p.

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title = "Cosmic ray helium isotopes from the BESS-Polar I experiment",

abstract = "The first flight of the Balloon-Borne Experiment with a Superconducting Spectrometer (BESS-Polar I) in Antarctica collected about 900 million cosmic ray events during 8.5 days in 2004. Particle charge was determined from energy loss in the scintillators, rigidity by reconstructing each particle trajectory in the magnetic field, and velocity by utilizing time of flights counters. These measurements can clearly identify hydrogen and helium isotopes among the incoming particles. These isotopes are generally believed to result from nuclear interactions of primaries with the interstellar medium. Measurement of their flux is expected to provide important information on cosmic ray sources and particle propagation in interstellar space. The presentation will focus on determination of the helium isotope flux in the kinetic energy per nucleon range 0.1 GeV/n to about 1.5 GeV/n. After quickly introducing the BESS-Polar I detector, the dedicated analysis to differentiate isotopes will be described. Finally, the energy spectra will be presented and compared to previous measurements.",

keywords = "BESS, BESS-polar I, Balloon-borne experiment, Cosmic-rays, Helium isotopes",

author = "N. Picot-Clemente and K. Abe and H. Fuke and S. Haino and T. Hams and A. Itazaki and Kim, {K. C.} and T. Kumazawa and Lee, {M. H.} and Y. Makida and S. Matsuda and K. Matsumoto and Mitchell, {J. W.} and Z. Myers and J. Nishimura and M. Nozaki and R. Orito and Ormes, {J. F.} and M. Sasaki and Seo, {E. S.} and Y. Shikaze and Streitmatter, {R. E.} and J. Suzuki and Y. Takasugi and K. Takeuchi and K. Tanaka and T. Yamagami and A. Yamamoto and T. Yoshida and K. Yoshimura",

year = "2011",

doi = "10.7529/ICRC2011/V06/0699",

language = "English",

pages = "51--54",

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TY - CONF

T1 - Cosmic ray helium isotopes from the BESS-Polar I experiment

AU - Picot-Clemente, N.

AU - Abe, K.

AU - Fuke, H.

AU - Haino, S.

AU - Hams, T.

AU - Itazaki, A.

AU - Kim, K. C.

AU - Kumazawa, T.

AU - Lee, M. H.

AU - Makida, Y.

AU - Matsuda, S.

AU - Matsumoto, K.

AU - Mitchell, J. W.

AU - Myers, Z.

AU - Nishimura, J.

AU - Nozaki, M.

AU - Orito, R.

AU - Ormes, J. F.

AU - Sasaki, M.

AU - Seo, E. S.

AU - Shikaze, Y.

AU - Streitmatter, R. E.

AU - Suzuki, J.

AU - Takasugi, Y.

AU - Takeuchi, K.

AU - Tanaka, K.

AU - Yamagami, T.

AU - Yamamoto, A.

AU - Yoshida, T.

AU - Yoshimura, K.

PY - 2011

Y1 - 2011

N2 - The first flight of the Balloon-Borne Experiment with a Superconducting Spectrometer (BESS-Polar I) in Antarctica collected about 900 million cosmic ray events during 8.5 days in 2004. Particle charge was determined from energy loss in the scintillators, rigidity by reconstructing each particle trajectory in the magnetic field, and velocity by utilizing time of flights counters. These measurements can clearly identify hydrogen and helium isotopes among the incoming particles. These isotopes are generally believed to result from nuclear interactions of primaries with the interstellar medium. Measurement of their flux is expected to provide important information on cosmic ray sources and particle propagation in interstellar space. The presentation will focus on determination of the helium isotope flux in the kinetic energy per nucleon range 0.1 GeV/n to about 1.5 GeV/n. After quickly introducing the BESS-Polar I detector, the dedicated analysis to differentiate isotopes will be described. Finally, the energy spectra will be presented and compared to previous measurements.

AB - The first flight of the Balloon-Borne Experiment with a Superconducting Spectrometer (BESS-Polar I) in Antarctica collected about 900 million cosmic ray events during 8.5 days in 2004. Particle charge was determined from energy loss in the scintillators, rigidity by reconstructing each particle trajectory in the magnetic field, and velocity by utilizing time of flights counters. These measurements can clearly identify hydrogen and helium isotopes among the incoming particles. These isotopes are generally believed to result from nuclear interactions of primaries with the interstellar medium. Measurement of their flux is expected to provide important information on cosmic ray sources and particle propagation in interstellar space. The presentation will focus on determination of the helium isotope flux in the kinetic energy per nucleon range 0.1 GeV/n to about 1.5 GeV/n. After quickly introducing the BESS-Polar I detector, the dedicated analysis to differentiate isotopes will be described. Finally, the energy spectra will be presented and compared to previous measurements.

KW - BESS

KW - BESS-polar I

KW - Balloon-borne experiment

KW - Cosmic-rays

KW - Helium isotopes

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DO - 10.7529/ICRC2011/V06/0699

M3 - Paper

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SP - 51

EP - 54

T2 - 32nd International Cosmic Ray Conference, ICRC 2011

Y2 - 11 August 2011 through 18 August 2011

ER -

Cosmic ray helium isotopes from the BESS-Polar I experiment

Abstract

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Keywords

ASJC Scopus subject areas

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