Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica

K. Yoshida; H. Kitamura; Shoji Torii; T. Tamura; K. Kasahara; J. Chang; I. Iijima; A. Kadokura; Y. Katayose; T. Kobayashi; Y. Komori; Y. Matsuzaka; K. Mizutani; H. Murakami; M. Namiki; J. Nishimura; S. Ohta; Y. Saito; M. Shibata; N. Tateyama; T. Yamagami; H. Yamagishi; T. Yuda

Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica

K. Yoshida, H. Kitamura, Shoji Torii, T. Tamura, K. Kasahara, J. Chang, I. Iijima, A. Kadokura, Y. Katayose, T. Kobayashi, Y. Komori, Y. Matsuzaka, K. Mizutani, H. Murakami, M. Namiki, J. Nishimura, S. Ohta, Y. Saito, M. Shibata, N. TateyamaT. Yamagami, H. Yamagishi, T. Yuda

研究成果: Conference contribution

抄録

Since atmospheric gamma rays at high altitude are mainly produced by a single interaction of primary cosmic rays with atmospheric nuclei, they are very useful to study nuclear interaction models and atmospheric neutrinos. We have observed atmospheric gamma rays from 100 GeV to 1 TeV with PPB-BETS by a long duration balloon flight of Polar Patrol Balloon (PPB) in Antarctica. The observation was carried out for 13 days at an altitudeof ∼35 km in January 2004. The detector of PPB-BETS is an imaging calorimeter composed of scintillating-fiber belts and plastic scintillators inserted between lead plates. We have collected 5.7×10³ events over 100 GeV. The number of observed atmospheric gamma rays is 1.0×10² events in the energy range of 100 GeV to 1 TeV.

本文言語	English
ホスト出版物のタイトル	29th International Cosmic Ray Conference, ICRC 2005
出版社	Tata Institute of Fundamental Research
ページ	53-56
ページ数	4
巻	9
出版ステータス	Published - 2005
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune 継続期間: 2005 8月 3 → 2005 8月 10

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
City	Pune
Period	05/8/3 → 05/8/10

ASJC Scopus subject areas

核物理学および高エネルギー物理学

他のファイルとリンク

引用スタイル

Yoshida, K., Kitamura, H., Torii, S., Tamura, T., Kasahara, K., Chang, J., Iijima, I., Kadokura, A., Katayose, Y., Kobayashi, T., Komori, Y., Matsuzaka, Y., Mizutani, K., Murakami, H., Namiki, M., Nishimura, J., Ohta, S., Saito, Y., Shibata, M., ... Yuda, T. (2005). Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica. In 29th International Cosmic Ray Conference, ICRC 2005 (Vol. 9, pp. 53-56). Tata Institute of Fundamental Research.

Yoshida, K, Kitamura, H, Torii, S, Tamura, T, Kasahara, K, Chang, J, Iijima, I, Kadokura, A, Katayose, Y, Kobayashi, T, Komori, Y, Matsuzaka, Y, Mizutani, K, Murakami, H, Namiki, M, Nishimura, J, Ohta, S, Saito, Y, Shibata, M, Tateyama, N, Yamagami, T, Yamagishi, H & Yuda, T 2005, Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica. in 29th International Cosmic Ray Conference, ICRC 2005. vol. 9, Tata Institute of Fundamental Research, pp. 53-56, 29th International Cosmic Ray Conference, ICRC 2005, Pune, 05/8/3.

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title = "Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica",

abstract = "Since atmospheric gamma rays at high altitude are mainly produced by a single interaction of primary cosmic rays with atmospheric nuclei, they are very useful to study nuclear interaction models and atmospheric neutrinos. We have observed atmospheric gamma rays from 100 GeV to 1 TeV with PPB-BETS by a long duration balloon flight of Polar Patrol Balloon (PPB) in Antarctica. The observation was carried out for 13 days at an altitudeof ∼35 km in January 2004. The detector of PPB-BETS is an imaging calorimeter composed of scintillating-fiber belts and plastic scintillators inserted between lead plates. We have collected 5.7×103 events over 100 GeV. The number of observed atmospheric gamma rays is 1.0×102 events in the energy range of 100 GeV to 1 TeV.",

author = "K. Yoshida and H. Kitamura and Shoji Torii and T. Tamura and K. Kasahara and J. Chang and I. Iijima and A. Kadokura and Y. Katayose and T. Kobayashi and Y. Komori and Y. Matsuzaka and K. Mizutani and H. Murakami and M. Namiki and J. Nishimura and S. Ohta and Y. Saito and M. Shibata and N. Tateyama and T. Yamagami and H. Yamagishi and T. Yuda",

year = "2005",

language = "English",

volume = "9",

pages = "53--56",

booktitle = "29th International Cosmic Ray Conference, ICRC 2005",

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TY - GEN

T1 - Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica

AU - Yoshida, K.

AU - Kitamura, H.

AU - Torii, Shoji

AU - Tamura, T.

AU - Kasahara, K.

AU - Chang, J.

AU - Iijima, I.

AU - Kadokura, A.

AU - Katayose, Y.

AU - Kobayashi, T.

AU - Komori, Y.

AU - Matsuzaka, Y.

AU - Mizutani, K.

AU - Murakami, H.

AU - Namiki, M.

AU - Nishimura, J.

AU - Ohta, S.

AU - Saito, Y.

AU - Shibata, M.

AU - Tateyama, N.

AU - Yamagami, T.

AU - Yamagishi, H.

AU - Yuda, T.

PY - 2005

Y1 - 2005

N2 - Since atmospheric gamma rays at high altitude are mainly produced by a single interaction of primary cosmic rays with atmospheric nuclei, they are very useful to study nuclear interaction models and atmospheric neutrinos. We have observed atmospheric gamma rays from 100 GeV to 1 TeV with PPB-BETS by a long duration balloon flight of Polar Patrol Balloon (PPB) in Antarctica. The observation was carried out for 13 days at an altitudeof ∼35 km in January 2004. The detector of PPB-BETS is an imaging calorimeter composed of scintillating-fiber belts and plastic scintillators inserted between lead plates. We have collected 5.7×103 events over 100 GeV. The number of observed atmospheric gamma rays is 1.0×102 events in the energy range of 100 GeV to 1 TeV.

AB - Since atmospheric gamma rays at high altitude are mainly produced by a single interaction of primary cosmic rays with atmospheric nuclei, they are very useful to study nuclear interaction models and atmospheric neutrinos. We have observed atmospheric gamma rays from 100 GeV to 1 TeV with PPB-BETS by a long duration balloon flight of Polar Patrol Balloon (PPB) in Antarctica. The observation was carried out for 13 days at an altitudeof ∼35 km in January 2004. The detector of PPB-BETS is an imaging calorimeter composed of scintillating-fiber belts and plastic scintillators inserted between lead plates. We have collected 5.7×103 events over 100 GeV. The number of observed atmospheric gamma rays is 1.0×102 events in the energy range of 100 GeV to 1 TeV.

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UR - http://www.scopus.com/inward/citedby.url?scp=84899016678&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84899016678

VL - 9

SP - 53

EP - 56

BT - 29th International Cosmic Ray Conference, ICRC 2005

PB - Tata Institute of Fundamental Research

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

Atmospheric gamma-ray observation over 100GeV with PPB-BETS by long duration balloon flight in Antarctica

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