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1. Cosmic-Ray Spectra and Composition in the Energy Range of 10-1000 TeV per Particle Obtained by the RUNJOB Experiment

Author

The, RUNJOB Collaboration, Derbina, V. A., Galkin, V. I., Kopenkin, V. V., Managadze, A. K., Misnikova, N. P., Mukhamedshin, R. A., Nazarov, S. N., Osedlo, V. I., Oshuev, D. S., Publichenko, P. A., Rakobolskaya, I. V., Roganova, T. M., Sazhina, G. P., Sveshnikova, L. G., Taran, V. M., Yashin, I. V., Zamchalova, E. A., Zatsepin, G. T., Zayarnaya, I. S., Hareyama, M., Hirakawa, Y., Horiuchi, Y., Ichimura, M., Inoue, N., Kamioka, E., Kobayashi, T., Kuramata, S., Matsutani, H., Nagasawa, S., Nakano, R., Namiki, Michiyoshi, Nakazawa, M., Nanjo, H., Ohata, S., Ohtomo, H., Saito, C., Semba, H., Shibata, T., Shuto, D., Sugimoto, H., Suzuki, R., Yajima, Nobuyuki, and Yamagami, Takamasa

Subjects
Physics, Shock wave, Range (particle radiation), Proton, Astrophysics::High Energy Astrophysical Phenomena, chemistry.chemical_element, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Spectral line, Intensity (physics), Particle acceleration, chemistry, Space and Planetary Science, Helium
Abstract

著者人数: 43名, Accepted: 2005-06-15, 資料番号: SA1003415000

Published
2005

2. Energy determination by means of the emulsion chamber with diffuser module

Author

V., I. Galkin, V., Kopenkin, A., K. Managadze, N., P. Misnikova, R., A. Mukhamedshin, S., N. Nazarov, D., S. Oshuev, P., A. Publichenko, I., V. Rakobolskaya, T., M. Roganova, G., P. Sazhina, L., G. Sveshnikova, I., V. Yashin, E., A. Zamchalova, G., T. Zatsepin, I., S. Zayarnaya, Hareyama, M., Fujii, M., Galkin, V. I., Goto, Y., Ichimura, M., Kamioka, E., Kobayashi, T., Kopenkin, V., Kuramata, S., Managadze, A. K., Matsutani, H., Misnikova, N. P., Mukhamedshin, R. A., Nanjo, H., Nazarov, S. N., Oshuev, D. S., Publichenko, P. A., Rakobolskaya, I. V., Roganova, T. M., Sazhina, G. P., Semba, H., Shibata, T., Sugimoto, H., Sveshnikova, L. G., Takahashi, K., Yashin, I. V., Zamchalova, E. A., Zatsepin, G. T., and Zayarnaya, I. S.

Abstract

シャワー拡散層付エマルションチェンバーによるエネルギー決定法について報告する． この方法は，1995年の日ロ共同気球実験(RUNJOB-program, RUssia-Nippon JOint Balloon-program) で観測されたPeV陽子のエネルギー推定方法を基に開発され，1997年のRUNJOB実験より導入した．シャワー拡散層はカロリメーター層の下部に設置され，カロリメーター層で発達した電磁カスケードシャワーはシャワー拡散層で幾何学的に広がり，電子数密度が減少する．普通，電磁カスケードシャワーによるエネルギー決定の場合，シャワー最大発達点を捉えていないとそのエネルギーは信頼できない．しかし，本論文で報告する方法により，シャワー極大を捉えていない場合でもエネルギー決定が可能となった．約４ｃｍの厚さのシャワー拡散層があれば陽子の場合，６c.u.の鉛厚で数１０TeVまで，９c.u.あれば１００TeV近くまでシャワーエネルギーをσ～０．２以内の精度で決定できる．又，鉄核の場合，６c.u.の鉛厚で１００TeVまでのシャワーエネルギーをやはりσ～０．２以内の精度で決定できる．したがって，これまでシャワー極大を捉えていないためデータとして採用できないような高エネルギーシャワーについてもエネルギー決定が行え，特に高エネルギー領域の統計量を増やす事ができる．本論文では，主にシャワー拡散層付エマルションチェンバー内でのカスケードシャワーシミュレーション方法およびエネルギー決定精度について議論する．また実際にRUNJOB実験データに対して適用した例についても報告する．, We report a new energy determination method using the emulsion calorimeter with diffuser module. The idea of diffuser method is based on the energy estimation for a PeV proton observed by the first RUNJOB(RUssia-Nippon JOint Balloon-program) experiment in 1995 and we have used a new type of emulsion chamber with diffuser module since 1997. The diffuser module was set below calorimeter, and the electromagnetic cascade shower develops in the calorimeter, and spreads geometcally in the diffuser. In general, it is very hard to determine the energy unless we detect the shower maximum, but it might be possible to determine the shower energy with help of the diffuser module. We find the energy resolution is better than σ～0.2 for proton with several tens TeV and for iron with 100TeV if the path length of calorimeter and the diffuser are 6c.u. and 4cm respectively. With the thickness of calorimeter of 9c.u. with 4cm diffuser, we can estimate the energy up to nearly 100TeV for proton with the resolution of better than σ～0.2. In this report, we disscus the energy resolution in the present method based on the simulation calculation of cascade shower in the calorimeter with diffuser module. We show several events observed by RUNJOB experiment in 1997 and alloy the present method for the energy determination., 資料番号: SA0200107000

Published
2003

3. Observation of High Energy Primary Cosmic-rays by Japanese-Russo Joint Balloon Experiment

Author

APANASENKO, A.V., BEREZOVSKAYA, V.A., FUJII, M., FUKUDA, T., HAREYAMA, M., HASHIMOTO, G., ICHIMURA, M., KAMIOKA, E., KOBAYASHI, T., KOPENKIN, V., KURAMATA, S., LAPSHIN, V.I., MANAGADZE, A.K., MATSUTANI, M., MISNIKOVA, N.P., MISU, T., MUKHAMEDSHIN, R.A., NAKAMURA, A., NANJO, H., NIKOLSKY, S.I., OGURA, K., OSHUEV, D.S., PUBLICHENKO, P.A., RAKOBOLSKAYA, I.V., ROGANOVA, T.M., SAZHINA, G.P., SEMBA, H., SHIBATA, T., SHIOTA, T., SUGIMOTO, H., SVESHNIKOVA, L.G., TARAN, V.M., WATANABE, Z., YASHIN, I.V., ZAMCHALOVA, E.A., ZATSEPIN, G.T., and ZAYARNAYA, I.S.

Subjects
1次宇宙線, RUNJOB, エマルションチェンバー
Abstract

広間隙型エマルションチェンバーを搭載した最初の日露共同気球実験(RUNJOB-program : RUssia-Nippon JOint Balloon-program)の結果を報告する。1995年7月に2機の気球がカムチャッカ半島から放球され, 両機ともヴォルガ川の近くで無事回収された。飛翔時間は1号機が130時間, 2号機が168時間であり, 水平浮遊の高度は両機とも約32kmであった。エマルションチェンバーの総面積は0.8m^2,厚さは陽子の衝突平均自由行程にして0.385m.f.p., 鉄核の場合には2.28m.f.p.である。Fuji-#200型X線フィルム上で検出された宇宙線飛跡の総数は381ケであるが, そのうち174ケが大気中で生成されたγ線であり, 解析対象となる宇宙線1次核は207ケであった。観測エネルギー領域は, 陽子の場合には20∿200TeV, ヘリウム核では3∿30TeV/nucleon, 鉄核では0.7∿5TeV/nucleonであった。このなかでPeVのエネルギーをもった陽子が1例検出されたことは注目すべきことである。よく知られている衝撃波加速(第一段加速)ではその寿命の制限から, 高々数10TeVが陽子加速の限界とされている。PeV陽子の存在は数100TeV以上の領域でなんらかの第二段階の加速が起きている可能性, あるいは銀河系外陽子の可能性を示唆している。この論文では, 主に1次宇宙線の各成分についてエネルギースペクトルを報告するが, エネルギー決定法についても議論し, PeV陽子の様相およびそのエネルギー推定の方法についても議論する。さらに全粒子スペクトル, 1次宇宙線の平均質量数についても報告する。, We report experimental results obtained by the wide-gap type emulsion chamber on board the first Japanese-Russo joint balloon, called RUNJOB (RUssia-Nippon JOint Balloon-program). Two balloons were launched subsequently from Kamchatka on July 1995,and the both were recovered successfully near Volga River. The exposure time is 130hrs for the first flight and 168hrs for the second. Altitude of the level flight is both approximately 32km on average, corresponding to 10g/cm^2. Total area of the emulsion chamber is 0.8m^2,and the thickness is 0.385 and 2.28 collision m.f.p.'s in vertical for proton- and iron-primaries, respectively. We detected 381 showers on Fuji-#200-type X-ray film, among which 174 showers originate in atmospheric secondary γ's, and the rest 207 come from nuclear components. The energy range covers 20∿200TeV for proton-primary, 3∿30TeV/nucleon for helium-primary, and 0.7∿5TeV/nucleon for iron-primary. It is remarkable that a very high energy proton with a few PeV is detected in the present experiment. It means no spectral break appears at around 10^eV, in contrast to the maximum energy predicted by the current shock wave acceleration (first stage acceleration). This evidence indicates either some second stage acceleration occurs beyond a few hundreds TeV, or an extragalactic proton is detected directly. We give energy spectra for various elements (proton, helium, ..., iron) as well as a new method for the energy determination using the opening-angle of γ-ray core. We show also the feature of the PeV proton and discuss the estimation of primary energy. All-particle spectrum and the average mass of primary cosmic ray are also presented., 資料番号: SA0167116000

Published
1998

4. Solar Activity during Two Millennia as Estimated from Annual Tree Rings

Author

Muraki, Y., Mitsutani, T., Kuramata, S., Masuda, K., Nagaya, K., and Shibata, S.

Subjects
Physics - Atmospheric and Oceanic Physics, Astrophysics - Solar and Stellar Astrophysics, Atmospheric and Oceanic Physics (physics.ao-ph), FOS: Physical sciences, Solar and Stellar Astrophysics (astro-ph.SR)
Abstract

The relationship between solar activity and the global climate is not only an academically interesting issue, but also an important problem for human beings. Lean and Rind have analyzed a considerable amount of climate data from around the world from 1889 to 2006. According to their analysis, the global effect was estimated to be 0.17 plus-minus 0.01K between the solar maximum and minimum. However, they noticed that the effect strongly appeared in the zones between 70N and 30N, and between 25S and 50S. At its peak latitude (near 40), the effect was estimated to be 0.5 K. Therefore, we analyzed a tree that survived at the Murooji temple in Nara prefecture (34d32mN, 136d2mE) Japan, for 391 years. Quite surprisingly, Fourier analysis of the annual growth rate identified two cycles with periodicities of 12 and 25 years during the Maunder minimum. We have continued the analysis, using different samples from the Nagusa shrine in Hyogo Prefecture, Itayanagi City, Aomori Prefecture, Japan, and from Yaku Island in Kyusyu, Japan. An evidence of solar activity was found in all of the samples. In particular, we have discovered a correlation between Swiss glacier fluctuation and the growth rate of the Yaku tree ring., Comment: 6 pages, 8 figures paper presented in icrc2013 at Rio

Published
2013
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5. High Energy Astro-particle Physics with the CALET Experiment

Author

Adriani, O., Asano, K., Bagliesi, M. G., Bigongiari, G., Binns, W. R., Bongi, M., Buckley, J. H., Castellini, G., Cherry, M. L., Gianmaria Collazuol, Ebisawa, K., Di Felice, V., Fuke, H., Gherardi, A., Guzik, T. G., Hams, T., Hasebe, N., Hareyama, M., Hibino, K., Ichimura, M., Ioka, K., Isbert, J. B., Israel, M. H., Kamioka, E., Kasahara, K., Katayose, Y., Kataoka, J., Kataoka, R., Kawanaka, N., Kim, M. Y., Kitamura, H., Komori, Y., Kotani, T., Krawczynski, H. S., Krizmanic, J. F., Kubota, A., Kuramata, S., Lomtadze, T., Maestro, P., Marcelli, L., Marrocchesi, P. S., Millucci, V., Mitchell, J. W., Mizutani, K., Moiseev, A. A., Mori, K., Mori, M., Mori, N., Munakata, K., Murakami, H., Nakagawa, Y. E., Nishimura, J., Okuno, S., Ormes, J. F., Ozawa, S., Papini, P., Rauch, B. F., Ricciarini, S., Saito, Y., Sasaki, M., Shibata, M., Shimizu, Y., Shiomi, A., Sparvoli, R., Spillantini, P., Takayanagi, M., Takita, M., Tamura, T., Tateyama, N., Terasawa, T., Tomida, H., Torii, S., Tunesada, Y., Uchihori, Y., Ueno, S., Vannuccini, E., Wefel, J. P., Yamaoka, K., Yoshida, A., Yoshida, K., and Yuda, T.

Published
2012

6. Measurement of B(D_s+ -> mu+ nu_mu)/B(D_s+ -> phi mu+ nu_mu) and Determination of the Decay Constant f_{D_s}

Author

Kodama, K., Torikai, S., Ushida, N., Mokhtarani, A., Paolone, V. S., Volk, J. T., Wilcox, J. O., Yager, P. M., Edelstein, R. M., Freyberger, A. P., Gibaut, D. B., Lipton, R. J., Nichols, W. R., Potter, D. M., Russ, J. S., Zhang, C., Zhang, Y., Jang, H. I., Kim, J. Y., Baller, B. R., Stefanski, R. J., Nakazawa, K., Chung, S. H., Park, M. S., Park, I. G., Song, J. S., Yoon, C. S., Aryal, M., Reay, N. W., Sidwell, R. A., Stanton, N. R., Yoshida, S., Chikawa, M., Hara, T., Aoki, S., Hoshino, K., Kobayashi, M., Komatsu, M., Miyanishi, M., Nakamura, M., Nakanishi, S., Niwa, K., Nomura, M., Okada, K., Tajima, H., Teraoka, K., Dunlea, J. M., Frederiksen, S. G., Kuramata, S., Lundberg, B. G., Oleynik, G. A., Reibel, K., Kalbfleisch, G. R., Skubic, P., Snow, J. M., Willis, S. E., Nakamura, K., Okusawa, T., Yoshida, T., Okabe, H., Yokota, J., Ihara, N., Kazuno, M., Koya, T., Niu, E., Ogawa, S., Shibuya, H., Watanabe, S., Yasuda, N., Ehara, K., Horie, K., Sato, Y., Suzuki, K., and Tezuka, I.

Subjects
High Energy Physics::Phenomenology, High Energy Physics::Experiment, High Energy Physics - Experiment
Abstract

We have observed $23.2 \pm 6.0_{-0.9}^{+1.0}$ purely-leptonic decays of $D_s^+ -> \mu^+ \nu_\mu$ from a sample of muonic one prong decay events detected in the emulsion target of Fermilab experiment E653. Using the $D_s^+ -> \phi \mu^+ \nu_\mu$ yield measured previously in this experiment, we obtain $B(D_s^+ --> \mu^+ \nu_\mu) / B(D_s^+ --> \phi \mu^+ \nu_\mu) =0.16 \pm 0.06 \pm 0.03$. In addition, we extract the decay constant $f_{D_s}=194 \pm 35 \pm 20 \pm 14 MeV$., Comment: 15 pages including one figure

Published
1996

7. Measurement of B(D_s+ -> mu+ nu_mu)/B(D_s+ -> phi mu+ nu_mu) and Determination of the Decay Constant f_{D_s}

Author

Kodama, K., Torikai, S., Ushida, N., Mokhtarani, A., Paolone, V. S., Volk, J. T., Wilcox, J. O., Yager, P. M., Edelstein, R. M., Freyberger, A. P., Gibaut, D. B., Lipton, R. J., Nichols, W. R., Potter, D. M., Russ, J. S., Zhang, C., Zhang, Y., Jang, H. I., Kim, J. Y., Baller, B. R., Stefanski, R. J., Nakazawa, K., Chung, S. H., Park, M. S., Park, I. G., Song, J. S., Yoon, C. S., Aryal, M., Reay, N. W., Sidwell, R. A., Stanton, N. R., Yoshida, S., Chikawa, M., Hara, T., Aoki, S., Hoshino, K., Kobayashi, M., Komatsu, M., Miyanishi, M., Nakamura, M., Nakanishi, S., Niwa, K., Nomura, M., Okada, K., Tajima, H., Teraoka, K., Dunlea, J. M., Frederiksen, S. G., Kuramata, S., Lundberg, B. G., Oleynik, G. A., Reibel, K., Kalbfleisch, G. R., Skubic, P., Snow, J. M., Willis, S. E., Nakamura, K., Okusawa, T., Yoshida, T., Okabe, H., Yokota, J., Ihara, N., Kazuno, M., Koya, T., Niu, E., Ogawa, S., Shibuya, H., Watanabe, S., Yasuda, N., Ehara, K., Horie, K., Sato, Y., Suzuki, K., and Tezuka, I.

Subjects
High Energy Physics - Experiment (hep-ex), FOS: Physical sciences
Abstract

We have observed $23.2 \pm 6.0_{-0.9}^{+1.0}$ purely-leptonic decays of $D_s^+ -> ��^+ ��_��$ from a sample of muonic one prong decay events detected in the emulsion target of Fermilab experiment E653. Using the $D_s^+ -> ����^+ ��_��$ yield measured previously in this experiment, we obtain $B(D_s^+ --> ��^+ ��_��) / B(D_s^+ --> ����^+ ��_��) =0.16 \pm 0.06 \pm 0.03$. In addition, we extract the decay constant $f_{D_s}=194 \pm 35 \pm 20 \pm 14 MeV$., 15 pages including one figure

Published
1996
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8. Balloon Measurement of New Particles

Author

FUCHI, H., HOSHINO, K., NIU, K., NIWA, K., TASAKA, S., SHIBUYA, H., YANAGISAWA, Y., KURAMATA, S., MAEDA, Y., KIMURA, H., and USHIDA, N.

Abstract

原子核乾板を主体とした,発生層付エマルジョン・チェンバーを気球に搭載して,字宙線に露出を行い,多重発生現象の観測を行った.そして,その中に発生した新粒子の研究を行ってきた.この報告では,1976年5月に三陸の基地から放球したチェンバーに見いだされた,新粒子が多体に崩壊したと思われる例について述べる., 資料番号: SA0125682000

Published
1978

9. The CALET instrument for experiment on the ISS

Author

Torii, S., Tamura, T., Yoshida, K., Tateyama, N., Hibino, K., Yuda, T., Kashiwagi, K., Okuno, S., Nishimura, J., Yamagami, T., Takayanagi, M., Saito, Y., Fuke, H., Tomida, H., Ueno, S., Makino, F., Shibata, M., Yusaku KATAYOSE, Kuramata, S., Ichimura, M., Uchihori, Y., Kitamura, H., Murakami, H., Kasahara, K., Kobayashi, T., Komori, Y., Mizutani, K., Terasawa, T., and Chang, J.

10. CALET observations of galactic electrons in the heliosphere

Author

Komori, Y., Torii, S., Tamura, T., Yoshida, K., Nishimura, J., Toshio Terasawa, Fuke, H., Hibino, K., Ichimura, M., Kasahara, K., Kashiwagi, K., Katayose, Y., Kitamura, H., Kobayashi, T., Kuramata, S., Makino, F., Mizutani, K., Murakami, H., Okuno, S., Saito, Y., Shibata, M., Takayanagi, M., Tateyama, N., Tomida, H., Uchihori, Y., Ueno, S., Yamagami, T., and Yuda, T.

11. Overview of the CALET Mission to the ISS

Author

Adriani, O., Asano, K., Bagliesi, M. G., Bigongiari, G., Binns, W. R., Bongi, M., Buckley, J. H., Castellini, G., Cherry, M. L., Gianmaria Collazuol, Ebisawa, K., Di Felice, V., Fuke, H., Gherardi, A., Guzik, T. G., Hams, T., Hasebe, N., Hareyama, M., Hibino, K., Ichimura, M., Ioka, K., Isbert, J. B., Israel, M. H., Kamioka, E., Kasahara, K., Katayose, Y., Kataoka, J., Kataoka, R., Kawanaka, N., Kim, M. Y., Kitamura, H., Komori, Y., Kotani, T., Krawczynski, H. S., Krizmanic, J. F., Kubota, A., Kuramata, S., Lomtadze, T., Maestro, P., Marcelli, L., Marrocchesi, P. S., Millucci, V., Mitchell, J. W., Mizutani, K., Moiseev, A. A., Mori, K., Mori, M., Mori, N., Munakata, K., Murakami, H., Nakagawa, Y. E., Nishimura, J., Okuno, S., Ormes, J. F., Ozawa, S., Papini, P., Rauch, B. F., Ricciarini, S., Saito, Y., Sasaki, M., Shibata, M., Shimizu, Y., Shiomi, A., Sparvoli, R., Spillantini, P., Takayanagi, M., Takita, M., Tamura, T., Tateyama, N., Terasawa, T., Tomida, H., Torii, S., Tunesada, Y., Uchihori, Y., Ueno, S., Vannuccini, E., Wefel, J. P., Yamaoka, K., Yoshida, A., Yoshida, K., and Yuda, T.

Subjects
Calorimeter, ISS, Dark matter, High Energy Electrons

12. Investigation of primary cosmic rays of high energy in russian-japaneese balloon experiment RUNJOB

Author

Apanasenko, A. V., Vatanabe, Z., Galkin, V. I., Getsov, G. G., Derbina, V. A., Zamchalova, E. A., Zatsepin, G. T., Zayarnaya, I. S., Ichimura, M., Kamioka, E., Kitanii, T., Kobayashi, T., Kopenkin, V. V., Kotunova, N. M., Kurijama, Yu, Kuramata, S., Lapshin, V. I., Alexander Managadze, Matsutani, M., Mikami, H., Misnikova, N. P., Mukhamedshin, R. A., Nazarov, S. N., Nakamura, A., Namiki, M., Nandjo, H., Nikolsky, S. I., Oe, T., Osedlo, V. I., Oshuev, D. S., Ökhta, S., Podorozhny, D. M., Publichenko, P. A., Rakobolskaya, I. V., Roganova, T. M., Sazhina, G. P., Saito, M., Sveshnikova, L. G., Semba, H., Sugimoto, H., Sukhadolskaya, V. A., Taran, V. M., Takachashi, K., Tsuchija, T., Fukuda, T., Fujii, M., Hareyama, M., Hashimoto, G., Shibata, T., Shiota, T., Shabanova, Y. N., Yadzhima, N., Yamagami, T., Yamamoto, K., and Yashin, I. V.

13. Russian-Japanese baloon experiment (RUNJOB) to study chemical composition and spectra of the primary cosmic emission in the energy range 1-500 BeV

Author

Zatsepin, G. T., Oshuev, D. S., Kakoboiskaya, I. V., Kotunova, N., Zamchalova, E. A., Alexander Managadze, Roganova, T. M., Sazhina, G. P., Sveshnikova, L. G., Apanasenko, A. V., Zayarnaya, I., Lapshin, V. I., Nikolsky, S. I., Kamioka, E., Kobayashi, T., Misu, T., Nakamura, A., Masuda, R., Shibata, T., Shiota, T., Fukuda, T., Hashimoto, G., Ichimura, M., Kuramata, S., Matsutani, H., Nanzho, H., Ogura, K., Tanabe, K., Takumi, M., Sugimoto, H., Fudjii, M., Watanabe, Z., Akiama, H., Namiki, M., Ota, S., Iazima, N., Iamagami, R., and Semba, H.

14. Observation of high-energy electron, gamma ray, and dark matter with CALET

Author

Yoshida, K., Torii, S., Tamura, T., Kasahara, K., Chang, J., Fuke, H., Hibino, K., Ichimura, M., Kashiwagi, T., Katayose, Y., Hisashi Kitamura, Kobayashi, T., Komori, Y., Kuramata, S., Makino, F., Mizutani, K., Murakami, H., Nishimura, J., Okuno, S., Saito, Y., Shibata, M., Takayanagi, M., Tateyama, N., Terasawa, T., Tomida, S., Uchihori, Y., Ueno, S., Yamagami, T., and Yuda, T.

15. The CALET mission on international space station

Author

Torii, S., Shimizu, Y., Kasahara, K., Hasebe, N., Hareyama, M., Kodaira, S., Okudaira, O., Yamashita, N., Miyazima, M., Miyaji, T., Tkayanagi, M., Ueno, S., Tomida, H., Saito, Y., Fuke, H., Yamagami, T., Nishimura, J., Tamura, T., Tateyama, N., Hibino, K., Okuno, S., Shiomi, A., Takita, M., Yuda, T., Kakimoto, F., Tsunesada, Y., Terasawa, T., Kobayashi, T., Yoshida, A., Yamaoka, K., Katayose, Y., Shibata, M., Ichimura, M., Kuramata, S., Uchihori, Y., Kitamura, A., Yoshida, K., Murakami, H., Komori, Y., Mizutani, K., Munakata, K., Streitmatter, R. E., Mitchell, J. W., Barbier, L. M., Moiseev, A. A., Krizmanic, J. F., Ormes, J. F., Wefel, J. P., Case, G., Cherry, M. L., Guzik, T. G., Isbert, J. B., Binns, W. R., Israel, M. H., Krawczynski, H. S., Marrocchesi, P. S., Gabriele Bigongiari, Batkov, K., Kim, M. Y., Bagliesi, M. G., Masestro, P., Millucci, V., Zei, R., Adriani, O., Papini, P., Vannuccini, E., Bonechi, L., Chang, J., Yan, J., and Gan, W.

16. Proton and Helium spectra obtained by RUNJOB experiment

Author

Hareyama, M., Derbina, V. A., Galkin, V. I., Hirakawa, Y., Horiuchi, Y., Ichimura, M., Inoue, N., Eiji Kamioka, Kobayashi, T., Kopenkin, V. V., Kuramata, S., Managadze, A. K., Matsutani, H., Misnikova, N. P., Mukhamedshin, R. A., Nagasawa, S., Nakano, R., Namiki, M., Nakazawa, M., Nanjo, H., Nazarov, S. N., Ohata, S., Ohtomo, H., Osedlo, V. I., Oshuev, D. S., Publichenko, P. A., Rakobolskaya, I. V., Roganova, T. M., Saito, C., Sazhina, G. P., Semba, H., Shibata, T., Shuto, D., Sugimoto, H., Suzuki, R., Sveshnikova, L. G., Taran, V. M., Yajima, N., Yamagami, T., Yashin, I. V., Zamchalova, E. A., Zatsepin, G. T., and Zayarnaya, I. S.

17. The CALET mission on international space station

Author

Torii, S., Tamura, T., Tateyama, N., Hibino, K., Yuda, T., Yoshida, K., Kashiwagi, K., Okuno, S., Nishimura, J., Yamagami, T., Saito, Y., Fuke, H., Takayanagi, M., Tomida, H., Ueno, S., Makino, F., Shibata, M., Katayose, Y., Kuramata, S., Ichimura, M., Uchihori, Y., Kitamura, H., Kasahara, K., Murakami, H., Kobayashi, T., Komori, Y., Mizutani, K., Terasawam, T., Streitmatter, R. E., Mitchell, J. W., Barbier, L. M., Moiseev, A. A., Krizmanic, J. F., Ormes, J. F., Binns, W. R., Israel, M. H., Krawzczynski, H. S., Case, G., Cherry, M. L., Guzik, T. G., Isbert, J. B., Wefel, J. P., Marrocchesi, P. S., Maestro, P., Bagliesi, M. G., Millucci, V., Meucci, M., Bigongiari, G., Zei, R., Franco Ligabue, Morsani, F., Adriani, O., Papini, P., Spillantini, P., Bonechi, L., Vannuccini, E., Chang, J., Gan, W., and Lu, T.

Subjects
SUPERNOVA-REMNANTS, COSMIC-RAY ELECTRONS

18. Spectra of primary cosmic ray nuclei obtained in RUNJOB experiment

Author

Galkin, V. I., Derbina, V. A., Zamchalova, E. A., Zatsepin, G. T., Zayarnaya, I. S., Ichimura, M., Inoue, N., Kamioka, E., Kobayashi, T., Kopenkin, V. V., Kuramata, S., Alexander Managadze, Matsutani, H., Misnikova, N. P., Mukhamedshin, R. A., Nagasawa, S., and Nakano, R.

19. Muon-neutrino to tau-neutrino oscillations: Proposal

Author

Kodama, K., Ushida, N., Tzanakos, G. S., Yager, P. M., Paolone, V. S., Hahn, C. H., Kim, J. Y., Bolton, T., Conrad, J., Shaevitz, M., Bogert, D., Koizumi, G., Lundberg, B., Malensek, A. J., Rameika, R., Song, J. S., Park, I. G., Nakazawa, K., Tasaka, S., Kuramata, S., Reay, N. W., Sidwell, R. A., Stanton, N. R., Green, K., Levin, D., James Matthews, Nitz, D., Tarle, G., Thun, R., Velde, J., Rusack, R. W., Singh, V., Chikawa, M., Aoki, S., Hara, T., Kim, Jae Kwan, Kang, J. S., Kim, C. O., Isokane, Y., Tsuneoka, Y., Hoshino, K., Kitamura, H., Kobayashi, M., Miyanishi, M., Nakamura, M., Nakamura, Y., Nakanishi, S., Niu, K., Niwa, K., Nomura, M., Saito, K., Tajima, H., Teraoka, K., Yoshida, S., Moriyama, K., Shibata, H., Okusawa, T., Teranaka, M., Tominaga, T., Yoshida, T., Watanabe, T., Fujioka, G., Takahashi, Y., Okabe, H., Yokota, J., Kusumoto, O., Kim, Jewan, Avignone, F. T., Rosenfeld, C., Goldberg, J., Adachi, M., Kazuno, M., Kobayashi, Y., Niu, E., Ono, S., Shibuya, H., Umezawa, Y., Napier, A., Oliver, W. P., Kafka, T., Schneps, J., Maeda, Y., Sato, Y., and Tezuka, I.

20. Performance of the CALET calorimeter by accelerator beam test

Author

Katayose, Y., Torii, S., Tamura, T., Yoshida, K., Murakami, H., Fuke, H., Hibino, K., Ichimura, M., Kasahara, K., Kashiwagi, K., Kitamura, H., Komori, Y., Kuramata, S., Kobayashi, T., Makino, F., Mizutani, K., Nishimura, J., Okuno, S., Saito, Y., Shibata, M., Takayanagi, M., Tateyama, N., Toshio Terasawa, Tomida, H., Uchihori, Y., Ueno, S., Yamagami, T., and Yuda, T.

21. All particle spectrum and average mass obtained by RUNJOB experiment

Author

Sveshnikova, L. G., Derbina, V. A., Galkin, V. I., Hareyama, M., Hirakawa, Y., Horiuchi, Y., Ichimura, M., Inoue, N., Kamioka, E., Kobayashi, T., Kopenkin, V. V., Kuramata, S., Alexander Managadze, Matsutani, H., Misnikova, N. P., Mukhamedshin, R. A., Nagasawa, S., Nakano, R., Namiki, M., Nakazawa, M., Nanjo, H., Nazarov, S. N., Ohata, S., Ohtomo, H., Osedlo, V. I., Oshuev, D. S., Publichenko, P. A., Rakobolskaya, I. V., Roganova, T. M., Saito, C., Sazhina, G. P., Semba, H., Shibatae, T., Shuto, D., Sugimoto, H., Suzuki, R., Taran, V. M., Yajima, N., Yamagami, T., Yashin, I. V., Zamchalova, E. A., Zatsepin, G. T., and Zayarnaya, I. S.

22. Heavy component spectra and secondary to primary ratios obtained by RUNJOB experiment

Author

Ichimura, M., Derbina, V. A., Galkin, V. I., Hareyama, M., Hirakawa, Y., Horiuchi, Y., Inoue, N., Kamioka, E., Kobayashi, T., Kopenkin, V. V., Kuramata, S., Alexander Managadze, Matsutani, H., Misnikova, N. P., Mukhamedshin, R. A., Nagasawa, S., Nakano, R., Namiki, M., Nakazawa, M., Nanjo, H., Nazarov, S. N., Ohata, S., Ohtomo, H., Osedlo, V. I., Oshuev, D. S., Publichenko, P. A., Rakobolskaya, I. V., Roganova, T. M., Saito, C., Sazhina, G. P., Semba, H., Shibata, T., Shuto, D., Sugimoto, H., Suzuki, R., Sveshnikova, L. G., Taran, V. M., Yajima, N., Yamagami, T., Yashin, I. V., Zamchalova, E. A., Zatsepin, G. T., and Zayarnaya, I. S.

23. CALET observation of nuclear components in primary cosmic rays

Author

Ichimura, M., Kuramata, S., Torii, S., Tamura, T., Yoshida, K., Kasahara, K., Chang, J., Fuke, H., Hibino, K., Kashiwagi, T., Katayose, Y., Kitamura, H., Kobayashi, T., Komori, Y., Makino, F., Mizutani, K., Murakami, H., Nishimura, J., Okuno, S., Saito, Y., Shibata, M., Takayanagi, M., Tateyama, N., Toshio Terasawa, Tomida, S., Uchihori, Y., Ueno, S., Yamagami, T., and Yuda, T.

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