Direct measurements of cosmic rays with the calorimetric electron telescope on the international space station

Author:

Akaike Yosui12,Adriani O.34,Asano K.5,Asaoka Y.5,Berti E.34,Bigongiari G.67,Binns W. R.8,Bongi M.34,Brogi P.67,Bruno A.9,Buckley J. H.8,Cannady N.910,Castellini G.11,Checchia C.7,Cherry M. L.11,Collazuol G.1213,Ebisawa K.1,Ficklin A. W.11,Fuke H.1,Gonzi S.34,Guzik T. G.11,Hams T.10,Hibino K.14,Ichimura M.15,Ioka K.16,Ishizaki W.5,Israel M. H.8,Kasahara K.17,Kataoka J.2,Kataoka R.18,Katayose Y.19,Kato C.20,Kawanaka N.16,Kawakubo Y.11,Kobayashi K.12,Kohri K.21,Krawczynski H. S.8,Krizmanic J. F.9,Maestro P.67,Marrocchesi P. S.67,Messineo A. M.622,Mitchell J. W.9,Miyake S.23,Moiseev A. A.924,Mori M.25,Mori N.3,Motz H. M.2,Munakata K.20,Nakahira S.1,Nishimura J.1,de Nolfo G. A.9,Okuno S.14,Ormes J. F.26,Ozawa S.27,Pacini L.3411,Papini P.3,Rauch B. F.8,Ricciarini S. B.328,Sakai K.910,Sakamoto T.29,Sasaki M.924,Shimizu Y.14,Shiomi A.30,Spillantini P.4,Stolzi F.67,Sugita S.29,Sulaj A.67,Takita M.5,Tamura T.14,Terasawa T.5,Torii S.2,Tsunesada Y.31,Uchihori Y.32,Vannuccini E.3,Wefel J. P.11,Yamaoka K.33,Yanagita S.34,Yoshida A.29,Yoshida K.2917,Zober W. V.8

Affiliation:

1. Japan Aerospace Exploration Agency

2. Waseda University

3. INFN Sezione di Firenze

4. University of Florence

5. Institute for Cosmic Ray Research

6. INFN Sezione di Pisa

7. University of Siena

8. Washington University in St. Louis

9. National Aeronautics and Space Administration

10. University of Maryland, Baltimore County

11. Louisiana State University

12. National Institute for Nuclear Physics Padova Division

13. University of Padua

14. Kanagawa University

15. Hirosaki University

16. Kyoto University

17. Shibaura Institute of Technology

18. National Institute of Polar Research

19. Yokohama National University

20. Shinshu University

21. High Energy Accelerator Research Organization

22. University of Pisa

23. National Institute of Technology, Ibaraki College

24. University of Maryland, College Park

25. Ritsumeikan University

26. University of Denver

27. National Institute of Information and Communications Technology

28. Italian National Research Council

29. Aoyama Gakuin University

30. Nihon University

31. Osaka Metropolitan University

32. National Institutes for Quantum and Radiological Science and Technology

33. Nagoya University

34. Ibaraki University

Abstract

The CALorimetric Electron Telescope, CALET, has been measuring high-energy cosmic rays on the International Space Station since October 13, 2015. The scientific objectives addressed by the mission are to search for possible nearby sources of high-energy electrons and potential signatures of dark matter, and to investigate the details of galactic cosmic-ray acceleration and propagation. The calorimetric instrument, which is 30 radiation lengths or 1.3 proton interaction lengths thick with fine imaging capability, is optimized to measure cosmic-ray electrons by achieving large proton rejection and excellent energy resolution well into the TeV region. In addition, very wide dynamic range of energy measurement and individual charge identification capability enable us to measure proton and nuclei spectra from a few tens GeV to a PeV scale. Nearly 20 million cosmic-ray shower events over 10 GeV per month are triggered and the continuous observation has been kept without any major interruption since the start of operation. Using the data obtained over 6.5 years of operation, we will present a brief summary of the CALET observation including electron spectrum, and proton and nuclei spectra as well as the performance study on orbit with MC simulations.

Funder

Agenzia Spaziale Italiana

Japan Society for the Promotion of Science

Ministry of Education, Culture, Sports, Science and Technology

National Aeronautics and Space Administration

Publisher

Stichting SciPost

Subject

General Medicine

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