CALET observation of nuclear components in primary cosmic rays

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

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

    Abstract

    Although CALET is originally designed for detections of electrons and gamma rays, nuclear components of primary cosmic rays, from protons to iron nucleus and more, are also observable by CALET, utilizing the total absorption calorimeter (TASC). TASC has 1.6 m.f.p. for protons which is enough to measure the energy of protons up to 1000 TeV. Using the observed spectra, the following items will be discussed: (1) the detailed structure of the spectrum, checking the change of the spectrum index and comparing indices of various components. More than 300 iron nuclei with the energy greater than 1 TeV/n will be observed. (2) secondary/primary ratio. Especially we can observe the both of B/C ratio and sub-Fe/Fe ratio. At the space station, the observation is free from the atmospheric contamination corrections. These observations are essential for the acceleration mechanisms and the propagation of cosmic rays.

    Original languageEnglish
    Title of host publication29th International Cosmic Ray Conference, ICRC 2005
    PublisherTata Institute of Fundamental Research
    Pages321-324
    Number of pages4
    Volume3
    Publication statusPublished - 2005
    Event29th International Cosmic Ray Conference, ICRC 2005 - Pune
    Duration: 2005 Aug 32005 Aug 10

    Other

    Other29th International Cosmic Ray Conference, ICRC 2005
    CityPune
    Period05/8/305/8/10

    Fingerprint

    primary cosmic rays
    calorimeters
    protons
    iron
    space stations
    nuclei
    cosmic rays
    rays
    contamination
    gamma rays
    propagation
    energy
    electrons

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    Ichimura, M., Kuramata, S., Torii, S., Tamura, T., Yoshida, K., Kasahara, K., ... Yuda, T. (2005). CALET observation of nuclear components in primary cosmic rays. In 29th International Cosmic Ray Conference, ICRC 2005 (Vol. 3, pp. 321-324). Tata Institute of Fundamental Research.

    CALET observation of nuclear components in primary cosmic rays. / Ichimura, M.; Kuramata, S.; Torii, Shoji; 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.; Terasawa, T.; Tomida, S.; Uchihori, Y.; Ueno, S.; Yamagami, T.; Yuda, T.

    29th International Cosmic Ray Conference, ICRC 2005. Vol. 3 Tata Institute of Fundamental Research, 2005. p. 321-324.

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

    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, Terasawa, T, Tomida, S, Uchihori, Y, Ueno, S, Yamagami, T & Yuda, T 2005, CALET observation of nuclear components in primary cosmic rays. in 29th International Cosmic Ray Conference, ICRC 2005. vol. 3, Tata Institute of Fundamental Research, pp. 321-324, 29th International Cosmic Ray Conference, ICRC 2005, Pune, 05/8/3.
    Ichimura M, Kuramata S, Torii S, Tamura T, Yoshida K, Kasahara K et al. CALET observation of nuclear components in primary cosmic rays. In 29th International Cosmic Ray Conference, ICRC 2005. Vol. 3. Tata Institute of Fundamental Research. 2005. p. 321-324
    Ichimura, M. ; Kuramata, S. ; Torii, Shoji ; 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. ; Terasawa, T. ; Tomida, S. ; Uchihori, Y. ; Ueno, S. ; Yamagami, T. ; Yuda, T. / CALET observation of nuclear components in primary cosmic rays. 29th International Cosmic Ray Conference, ICRC 2005. Vol. 3 Tata Institute of Fundamental Research, 2005. pp. 321-324
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    abstract = "Although CALET is originally designed for detections of electrons and gamma rays, nuclear components of primary cosmic rays, from protons to iron nucleus and more, are also observable by CALET, utilizing the total absorption calorimeter (TASC). TASC has 1.6 m.f.p. for protons which is enough to measure the energy of protons up to 1000 TeV. Using the observed spectra, the following items will be discussed: (1) the detailed structure of the spectrum, checking the change of the spectrum index and comparing indices of various components. More than 300 iron nuclei with the energy greater than 1 TeV/n will be observed. (2) secondary/primary ratio. Especially we can observe the both of B/C ratio and sub-Fe/Fe ratio. At the space station, the observation is free from the atmospheric contamination corrections. These observations are essential for the acceleration mechanisms and the propagation of cosmic rays.",
    author = "M. Ichimura and S. Kuramata and Shoji Torii and T. Tamura and K. Yoshida and K. Kasahara and J. Chang and H. Fuke and K. Hibino and T. Kashiwagi and Y. Katayose and H. Kitamura and T. Kobayashi and Y. Komori and F. Makino and K. Mizutani and H. Murakami and J. Nishimura and S. Okuno and Y. Saito and M. Shibata and M. Takayanagi and N. Tateyama and T. Terasawa and S. Tomida and Y. Uchihori and S. Ueno and T. Yamagami and T. Yuda",
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    TY - GEN

    T1 - CALET observation of nuclear components in primary cosmic rays

    AU - Ichimura, M.

    AU - Kuramata, S.

    AU - Torii, Shoji

    AU - Tamura, T.

    AU - Yoshida, K.

    AU - Kasahara, K.

    AU - Chang, J.

    AU - Fuke, H.

    AU - Hibino, K.

    AU - Kashiwagi, T.

    AU - Katayose, Y.

    AU - Kitamura, H.

    AU - Kobayashi, T.

    AU - Komori, Y.

    AU - Makino, F.

    AU - Mizutani, K.

    AU - Murakami, H.

    AU - Nishimura, J.

    AU - Okuno, S.

    AU - Saito, Y.

    AU - Shibata, M.

    AU - Takayanagi, M.

    AU - Tateyama, N.

    AU - Terasawa, T.

    AU - Tomida, S.

    AU - Uchihori, Y.

    AU - Ueno, S.

    AU - Yamagami, T.

    AU - Yuda, T.

    PY - 2005

    Y1 - 2005

    N2 - Although CALET is originally designed for detections of electrons and gamma rays, nuclear components of primary cosmic rays, from protons to iron nucleus and more, are also observable by CALET, utilizing the total absorption calorimeter (TASC). TASC has 1.6 m.f.p. for protons which is enough to measure the energy of protons up to 1000 TeV. Using the observed spectra, the following items will be discussed: (1) the detailed structure of the spectrum, checking the change of the spectrum index and comparing indices of various components. More than 300 iron nuclei with the energy greater than 1 TeV/n will be observed. (2) secondary/primary ratio. Especially we can observe the both of B/C ratio and sub-Fe/Fe ratio. At the space station, the observation is free from the atmospheric contamination corrections. These observations are essential for the acceleration mechanisms and the propagation of cosmic rays.

    AB - Although CALET is originally designed for detections of electrons and gamma rays, nuclear components of primary cosmic rays, from protons to iron nucleus and more, are also observable by CALET, utilizing the total absorption calorimeter (TASC). TASC has 1.6 m.f.p. for protons which is enough to measure the energy of protons up to 1000 TeV. Using the observed spectra, the following items will be discussed: (1) the detailed structure of the spectrum, checking the change of the spectrum index and comparing indices of various components. More than 300 iron nuclei with the energy greater than 1 TeV/n will be observed. (2) secondary/primary ratio. Especially we can observe the both of B/C ratio and sub-Fe/Fe ratio. At the space station, the observation is free from the atmospheric contamination corrections. These observations are essential for the acceleration mechanisms and the propagation of cosmic rays.

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