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Protons in near earth orbit

The proton spectrum in the kinetic energy range 0.1 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at an altitude of 380 km. Above the geomagnetic cutoff the observed spectrum is parameterized by a power law. Below the geomagnetic cutoff a substan...

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Bibliographic Details
Published in:Physics letters. B 2000, Vol.472 (1), p.215-226
Main Authors: Alcaraz, J., Ambrosi, G., Ao, L., Azzarello, P., Baldini, L., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, R., Becker, U., Bellagamba, L., Béné, P., Bertucci, B., Boella, G., Boschini, M., Bourquin, M., Burger, J.D., Cai, X.D., Capell, M., Casaus, J., Castellini, G., Chen, H.F., Chen, H.S., Chen, Z.G., Chernoplekov, N.A., Chiarini, A., Chiueh, T.H., Commichau, V., Contin, A., Crespo, P., da Cunha, J.P., D'Antone, I., Emonet, P., Eronen, T., Esposito, G., Favier, J., Fiandrini, E., Galaktionov, Yu, Giusti, P., Grandi, D., Hofer, H., Hungerford, W., Ionica, M., Karlamaa, K., Karpinski, W., Kenney, G., Kim, W., Klimentov, A., Laborie, G., Laitinen, T., Laurenti, G., Lee, S.C., Lopes, I., Lu, G., Lustermann, W., Margotti, A., Mayet, F., Meillon, B., Menichelli, M., Mujunen, A., Pauss, F., Perrin, E., Pevsner, A., Pilastrini, R., Plyaskin, V., Postolache, V., Prati, E., Produit, N., Rancoita, P.G., Ren, D., Richeux, J.P., Roeser, U., Sagdeev, R., Sartorelli, G., Schultz von Dratzig, A., Sun, G.S., Suter, H., Ting, Samuel C.C., Ting, S.M., Tornikoski, M., Ulbricht, J., Valtonen, E., Vandenhirtz, J., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J.P., Vité, D., Von Gunten, H., Wang, B.C., Wang, Y.H., Wiik, K., Xia, P.C., Yan, J.L., Xu, Z.Z., Zhang, Z.P., Zhu, G.Y., Zhu, W.Z.
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Language:English
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Summary:The proton spectrum in the kinetic energy range 0.1 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at an altitude of 380 km. Above the geomagnetic cutoff the observed spectrum is parameterized by a power law. Below the geomagnetic cutoff a substantial second spectrum was observed concentrated at equatorial latitudes with a flux ∼70 m −2 s −1 sr −1. Most of these second spectrum protons follow a complicated trajectory and originate from a restricted geographic region.
ISSN:0370-2693
1873-2445
DOI:10.1016/S0370-2693(99)01427-6