Cosmic protons

Cosmic protons

The primary proton spectrum in the kinetic energy range 0.2 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS–91 at an altitude of 380 km. The complete data set combining three shuttle attitudes and including all known systematic effects is presented.

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Veröffentlicht in:Physics letters. B 2000-09, Vol.490 (1), p.27-35
Hauptverfasser: Ambrosi, G., Ao, L., Arefiev, A., Azzarello, P., Basile, M., Barancourt, D., Barao, F., Becker, R., Becker, U., Berdugo, J., Berges, P., Bertucci, B., Blasko, S., Bourquin, M., Brocco, L., Buenerd, M., Burger, J.D., Burger, W.J., Cai, X.D., Capell, M., Cecchi, C., Chang, Y.H., Chen, Z.G., Cindolo, F., Commichau, V., Crespo, P., Cristinziani, M., Deus, J.D., Djambazov, L., D'Antone, I., Emonet, P., Engelberg, J., Eppling, F.J., Eronen, T., Esposito, G., Fiandrini, E., Fisher, P.H., Gervasi, M., Gu, W.Q., Hangarter, K., Hasan, A., Hermel, V., Huang, M.A., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Kim, W., Kossakowski, R., Kraeber, M., Laborie, G., Lee, S.C., Levtchenko, P., Liu, C.L., Liu, H.T., Lu, G., Lu, Y.S., Luckey, D., Lustermann, W., Palmonari, F., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pojidaev, V., Rapin, D., Ren, Z., Ribordy, M., Roissin, C., Sagdeev, R., Schwering, G., Scolieri, G., Seo, E.S., Song, T., Ting, Samuel C.C., Tornikoski, M., Torsti, J., Trümper, J., Usoskin, I., Vandenhirtz, J., Velcea, F., Verlaat, B., Vezzu, F., Von Gunten, H., Waldmeier Wicki, S., Wang, J.Z., Wang, Y.H., Wiik, K., Wu, S.X., Yan, J.L., Yan, L.G., Yang, C.G., Yang, M., Ye, S.W., Xu, Z.Z., Zhang, Z.P., Zhao, D.X., Zhu, G.Y., Zhuang, H.L., Zimmermann, B.
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Cosmology and Extra-Galactic Astrophysics
Physics
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Zusammenfassung:The primary proton spectrum in the kinetic energy range 0.2 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS–91 at an altitude of 380 km. The complete data set combining three shuttle attitudes and including all known systematic effects is presented.
ISSN:0370-2693
1873-2445
DOI:10.1016/S0370-2693(00)00970-9