Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01

Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propag...

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Detalles Bibliográficos
Autores principales: Aguilar, M., Alcaraz, J., Allaby, J., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Arruda, L., Azzarello, P., Basile, M., Barao, F., Barreira, G., Bartoloni, A., Battiston, R., Becker, R., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bindi, V., Boella, G., Boschini, M., Bourquin, M., Bruni, G., Buenerd, M., Burger, J.D., Burger, W.J., Cai, X.D., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cernuda, I., Chang, Y.H., Chen, H.F., Chen, H.S., Chen, Z.G., Chernoplekov, N.A., Chiueh, T.H., Choi, Y.Y., Cindolo, F., Commichau, V., Contin, A., Cortina-Gil, E., Crespo, D., Cristinziani, M., Dai, T.S., de la Guia, C., Delgado, C., Di Falco, S., Djambazov, L., D'Antone, I., Dong, Z.R., Duranti, M., Engelberg, J., Eppling, F.J., Eronen, T., Extermann, P., Favier, J., Fiandrini, E., Fisher, P.H., Flugge, G., Fouque, N., Galaktionov, Y., Gervasi, M., Giovacchini, F., Giusti, P., Grandi, D., Grimm, O., Gu, W.Q., Haino, S., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Hungerford, W., Ionica, M., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kim, D.H., Kim, G.N., Kim, K.S., Kirn, T., Klimentov, A., Kossakowski, R., Kounine, A., Koutsenko, V., Kraeber, M., Laborie, G., Laitinen, T., Lamanna, G., Laurenti, G., Lebedev, A., Lechanoine-Leluc, C., Lee, M.W., Lee, S.C., Levi, G., Lin, C.H., Liu, H.T., Lu, G., Lu, Y.S., Lubelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., McNeil, R.R., Menichelli, M., Mihul, A., Mujunen, A., Oliva, A., Palmonari, F., Park, H.B., Park, W.H., Pauluzzi, M., Pauss, F., Pereira, R., Perrin, E., Pevsner, A., Pilo, F., Pimenta, M., Plyaskin, V., Pojidaev, V., Pohl, M., Produit, N., Quadrani, L., Rancoita, P.G., Rapin, D., Ren, D., Ren, Z., Ribordy, M., Richeux, J.P., Riihonen, E., Ritakari, J., Ro, S., Roeser, U., Sagdeev, R., Santos, D., Sartorelli, G., Sbarra, C., Schael, S., Schultz von Dratzig, A., Schwering, G., Seo, E.S., Shin, J.W., Shoumilov, E., Shoutko, V., Siedenburg, T., Siedling, R., Son, D., Song, T., Spada, F.R., Spinella, F., Steuer, M., Sun, G.S., Suter, H., Tang, X.W., Ting, Samuel C.C., Ting, S.M., Tomassetti, N., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Valtonen, E., Vandenhirtz, J., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J.P., Viertel, G., Vite, D., Von Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, J.Z., Wiik, K., Williams, C., Wu, S.X., Xia, P.C., Xu, S., Xu, Z.Z., Yan, J.L., Yan, L.G., Yang, C.G., Yang, J., Yang, M., Ye, S.W., Zhang, H.Y., Zhang, Z.P., Zhao, D.X., Zhou, F., Zhou, Y., Zhu, G.Y., Zhu, W.Z., Zhuang, H.L., Zichichi, A., Zimmermann, B., Zuccon, P.
Lenguaje:eng
Publicado: 2010
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1088/0004-637X/724/1/329
http://cds.cern.ch/record/1288148
_version_ 1780920627138396160
author Aguilar, M.
Alcaraz, J.
Allaby, J.
Alpat, B.
Ambrosi, G.
Anderhub, H.
Ao, L.
Arefiev, A.
Arruda, L.
Azzarello, P.
Basile, M.
Barao, F.
Barreira, G.
Bartoloni, A.
Battiston, R.
Becker, R.
Becker, U.
Bellagamba, L.
Bene, P.
Berdugo, J.
Berges, P.
Bertucci, B.
Biland, A.
Bindi, V.
Boella, G.
Boschini, M.
Bourquin, M.
Bruni, G.
Buenerd, M.
Burger, J.D.
Burger, W.J.
Cai, X.D.
Cannarsa, P.
Capell, M.
Casadei, D.
Casaus, J.
Castellini, G.
Cernuda, I.
Chang, Y.H.
Chen, H.F.
Chen, H.S.
Chen, Z.G.
Chernoplekov, N.A.
Chiueh, T.H.
Choi, Y.Y.
Cindolo, F.
Commichau, V.
Contin, A.
Cortina-Gil, E.
Crespo, D.
Cristinziani, M.
Dai, T.S.
de la Guia, C.
Delgado, C.
Di Falco, S.
Djambazov, L.
D'Antone, I.
Dong, Z.R.
Duranti, M.
Engelberg, J.
Eppling, F.J.
Eronen, T.
Extermann, P.
Favier, J.
Fiandrini, E.
Fisher, P.H.
Flugge, G.
Fouque, N.
Galaktionov, Y.
Gervasi, M.
Giovacchini, F.
Giusti, P.
Grandi, D.
Grimm, O.
Gu, W.Q.
Haino, S.
Hangarter, K.
Hasan, A.
Hermel, V.
Hofer, H.
Hungerford, W.
Ionica, M.
Jongmanns, M.
Karlamaa, K.
Karpinski, W.
Kenney, G.
Kim, D.H.
Kim, G.N.
Kim, K.S.
Kirn, T.
Klimentov, A.
Kossakowski, R.
Kounine, A.
Koutsenko, V.
Kraeber, M.
Laborie, G.
Laitinen, T.
Lamanna, G.
Laurenti, G.
Lebedev, A.
Lechanoine-Leluc, C.
Lee, M.W.
Lee, S.C.
Levi, G.
Lin, C.H.
Liu, H.T.
Lu, G.
Lu, Y.S.
Lubelsmeyer, K.
Luckey, D.
Lustermann, W.
Mana, C.
Margotti, A.
Mayet, F.
McNeil, R.R.
Menichelli, M.
Mihul, A.
Mujunen, A.
Oliva, A.
Palmonari, F.
Park, H.B.
Park, W.H.
Pauluzzi, M.
Pauss, F.
Pereira, R.
Perrin, E.
Pevsner, A.
Pilo, F.
Pimenta, M.
Plyaskin, V.
Pojidaev, V.
Pohl, M.
Produit, N.
Quadrani, L.
Rancoita, P.G.
Rapin, D.
Ren, D.
Ren, Z.
Ribordy, M.
Richeux, J.P.
Riihonen, E.
Ritakari, J.
Ro, S.
Roeser, U.
Sagdeev, R.
Santos, D.
Sartorelli, G.
Sbarra, C.
Schael, S.
Schultz von Dratzig, A.
Schwering, G.
Seo, E.S.
Shin, J.W.
Shoumilov, E.
Shoutko, V.
Siedenburg, T.
Siedling, R.
Son, D.
Song, T.
Spada, F.R.
Spinella, F.
Steuer, M.
Sun, G.S.
Suter, H.
Tang, X.W.
Ting, Samuel C.C.
Ting, S.M.
Tomassetti, N.
Tornikoski, M.
Torsti, J.
Trumper, J.
Ulbricht, J.
Urpo, S.
Valtonen, E.
Vandenhirtz, J.
Velikhov, E.
Verlaat, B.
Vetlitsky, I.
Vezzu, F.
Vialle, J.P.
Viertel, G.
Vite, D.
Von Gunten, H.
Waldmeier Wicki, S.
Wallraff, W.
Wang, J.Z.
Wiik, K.
Williams, C.
Wu, S.X.
Xia, P.C.
Xu, S.
Xu, Z.Z.
Yan, J.L.
Yan, L.G.
Yang, C.G.
Yang, J.
Yang, M.
Ye, S.W.
Zhang, H.Y.
Zhang, Z.P.
Zhao, D.X.
Zhou, F.
Zhou, Y.
Zhu, G.Y.
Zhu, W.Z.
Zhuang, H.L.
Zichichi, A.
Zimmermann, B.
Zuccon, P.
author_facet Aguilar, M.
Alcaraz, J.
Allaby, J.
Alpat, B.
Ambrosi, G.
Anderhub, H.
Ao, L.
Arefiev, A.
Arruda, L.
Azzarello, P.
Basile, M.
Barao, F.
Barreira, G.
Bartoloni, A.
Battiston, R.
Becker, R.
Becker, U.
Bellagamba, L.
Bene, P.
Berdugo, J.
Berges, P.
Bertucci, B.
Biland, A.
Bindi, V.
Boella, G.
Boschini, M.
Bourquin, M.
Bruni, G.
Buenerd, M.
Burger, J.D.
Burger, W.J.
Cai, X.D.
Cannarsa, P.
Capell, M.
Casadei, D.
Casaus, J.
Castellini, G.
Cernuda, I.
Chang, Y.H.
Chen, H.F.
Chen, H.S.
Chen, Z.G.
Chernoplekov, N.A.
Chiueh, T.H.
Choi, Y.Y.
Cindolo, F.
Commichau, V.
Contin, A.
Cortina-Gil, E.
Crespo, D.
Cristinziani, M.
Dai, T.S.
de la Guia, C.
Delgado, C.
Di Falco, S.
Djambazov, L.
D'Antone, I.
Dong, Z.R.
Duranti, M.
Engelberg, J.
Eppling, F.J.
Eronen, T.
Extermann, P.
Favier, J.
Fiandrini, E.
Fisher, P.H.
Flugge, G.
Fouque, N.
Galaktionov, Y.
Gervasi, M.
Giovacchini, F.
Giusti, P.
Grandi, D.
Grimm, O.
Gu, W.Q.
Haino, S.
Hangarter, K.
Hasan, A.
Hermel, V.
Hofer, H.
Hungerford, W.
Ionica, M.
Jongmanns, M.
Karlamaa, K.
Karpinski, W.
Kenney, G.
Kim, D.H.
Kim, G.N.
Kim, K.S.
Kirn, T.
Klimentov, A.
Kossakowski, R.
Kounine, A.
Koutsenko, V.
Kraeber, M.
Laborie, G.
Laitinen, T.
Lamanna, G.
Laurenti, G.
Lebedev, A.
Lechanoine-Leluc, C.
Lee, M.W.
Lee, S.C.
Levi, G.
Lin, C.H.
Liu, H.T.
Lu, G.
Lu, Y.S.
Lubelsmeyer, K.
Luckey, D.
Lustermann, W.
Mana, C.
Margotti, A.
Mayet, F.
McNeil, R.R.
Menichelli, M.
Mihul, A.
Mujunen, A.
Oliva, A.
Palmonari, F.
Park, H.B.
Park, W.H.
Pauluzzi, M.
Pauss, F.
Pereira, R.
Perrin, E.
Pevsner, A.
Pilo, F.
Pimenta, M.
Plyaskin, V.
Pojidaev, V.
Pohl, M.
Produit, N.
Quadrani, L.
Rancoita, P.G.
Rapin, D.
Ren, D.
Ren, Z.
Ribordy, M.
Richeux, J.P.
Riihonen, E.
Ritakari, J.
Ro, S.
Roeser, U.
Sagdeev, R.
Santos, D.
Sartorelli, G.
Sbarra, C.
Schael, S.
Schultz von Dratzig, A.
Schwering, G.
Seo, E.S.
Shin, J.W.
Shoumilov, E.
Shoutko, V.
Siedenburg, T.
Siedling, R.
Son, D.
Song, T.
Spada, F.R.
Spinella, F.
Steuer, M.
Sun, G.S.
Suter, H.
Tang, X.W.
Ting, Samuel C.C.
Ting, S.M.
Tomassetti, N.
Tornikoski, M.
Torsti, J.
Trumper, J.
Ulbricht, J.
Urpo, S.
Valtonen, E.
Vandenhirtz, J.
Velikhov, E.
Verlaat, B.
Vetlitsky, I.
Vezzu, F.
Vialle, J.P.
Viertel, G.
Vite, D.
Von Gunten, H.
Waldmeier Wicki, S.
Wallraff, W.
Wang, J.Z.
Wiik, K.
Williams, C.
Wu, S.X.
Xia, P.C.
Xu, S.
Xu, Z.Z.
Yan, J.L.
Yan, L.G.
Yang, C.G.
Yang, J.
Yang, M.
Ye, S.W.
Zhang, H.Y.
Zhang, Z.P.
Zhao, D.X.
Zhou, F.
Zhou, Y.
Zhu, G.Y.
Zhu, W.Z.
Zhuang, H.L.
Zichichi, A.
Zimmermann, B.
Zuccon, P.
author_sort Aguilar, M.
collection CERN
description Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propagation models. In this paper the relative abundances of the light nuclei lithium, beryllium, boron and carbon are presented. The secondary to primary ratios Li/C, Be/C and B/C have been measured in the kinetic energy range 0.35-45 GeV/nucleon. The isotopic ratio 7Li/6Li is also determined in the magnetic rigidity interval 2.5-6.3 GV. The secondary to secondary ratios Li/Be, Li/B and Be/B are also reported. These measurements are based on the data collected by the Alpha Magnetic Spectrometer AMS-01 during the STS-91 space shuttle flight in 1998 June. Our experimental results are in substantial agreement with other measurements, where they exist. We describe our light-nuclei data with a diffusive-reacceleration model. A 10-15% overproduction of Be is found in the model predictions and can be attributed to uncertainties in the production cross-section data.
id cern-1288148
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2010
record_format invenio
spelling cern-12881482023-03-17T03:33:52Zdoi:10.1088/0004-637X/724/1/329http://cds.cern.ch/record/1288148engAguilar, M.Alcaraz, J.Allaby, J.Alpat, B.Ambrosi, G.Anderhub, H.Ao, L.Arefiev, A.Arruda, L.Azzarello, P.Basile, M.Barao, F.Barreira, G.Bartoloni, A.Battiston, R.Becker, R.Becker, U.Bellagamba, L.Bene, P.Berdugo, J.Berges, P.Bertucci, B.Biland, A.Bindi, V.Boella, G.Boschini, M.Bourquin, M.Bruni, G.Buenerd, M.Burger, J.D.Burger, W.J.Cai, X.D.Cannarsa, P.Capell, M.Casadei, D.Casaus, J.Castellini, G.Cernuda, I.Chang, Y.H.Chen, H.F.Chen, H.S.Chen, Z.G.Chernoplekov, N.A.Chiueh, T.H.Choi, Y.Y.Cindolo, F.Commichau, V.Contin, A.Cortina-Gil, E.Crespo, D.Cristinziani, M.Dai, T.S.de la Guia, C.Delgado, C.Di Falco, S.Djambazov, L.D'Antone, I.Dong, Z.R.Duranti, M.Engelberg, J.Eppling, F.J.Eronen, T.Extermann, P.Favier, J.Fiandrini, E.Fisher, P.H.Flugge, G.Fouque, N.Galaktionov, Y.Gervasi, M.Giovacchini, F.Giusti, P.Grandi, D.Grimm, O.Gu, W.Q.Haino, S.Hangarter, K.Hasan, A.Hermel, V.Hofer, H.Hungerford, W.Ionica, M.Jongmanns, M.Karlamaa, K.Karpinski, W.Kenney, G.Kim, D.H.Kim, G.N.Kim, K.S.Kirn, T.Klimentov, A.Kossakowski, R.Kounine, A.Koutsenko, V.Kraeber, M.Laborie, G.Laitinen, T.Lamanna, G.Laurenti, G.Lebedev, A.Lechanoine-Leluc, C.Lee, M.W.Lee, S.C.Levi, G.Lin, C.H.Liu, H.T.Lu, G.Lu, Y.S.Lubelsmeyer, K.Luckey, D.Lustermann, W.Mana, C.Margotti, A.Mayet, F.McNeil, R.R.Menichelli, M.Mihul, A.Mujunen, A.Oliva, A.Palmonari, F.Park, H.B.Park, W.H.Pauluzzi, M.Pauss, F.Pereira, R.Perrin, E.Pevsner, A.Pilo, F.Pimenta, M.Plyaskin, V.Pojidaev, V.Pohl, M.Produit, N.Quadrani, L.Rancoita, P.G.Rapin, D.Ren, D.Ren, Z.Ribordy, M.Richeux, J.P.Riihonen, E.Ritakari, J.Ro, S.Roeser, U.Sagdeev, R.Santos, D.Sartorelli, G.Sbarra, C.Schael, S.Schultz von Dratzig, A.Schwering, G.Seo, E.S.Shin, J.W.Shoumilov, E.Shoutko, V.Siedenburg, T.Siedling, R.Son, D.Song, T.Spada, F.R.Spinella, F.Steuer, M.Sun, G.S.Suter, H.Tang, X.W.Ting, Samuel C.C.Ting, S.M.Tomassetti, N.Tornikoski, M.Torsti, J.Trumper, J.Ulbricht, J.Urpo, S.Valtonen, E.Vandenhirtz, J.Velikhov, E.Verlaat, B.Vetlitsky, I.Vezzu, F.Vialle, J.P.Viertel, G.Vite, D.Von Gunten, H.Waldmeier Wicki, S.Wallraff, W.Wang, J.Z.Wiik, K.Williams, C.Wu, S.X.Xia, P.C.Xu, S.Xu, Z.Z.Yan, J.L.Yan, L.G.Yang, C.G.Yang, J.Yang, M.Ye, S.W.Zhang, H.Y.Zhang, Z.P.Zhao, D.X.Zhou, F.Zhou, Y.Zhu, G.Y.Zhu, W.Z.Zhuang, H.L.Zichichi, A.Zimmermann, B.Zuccon, P.Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01Astrophysics and AstronomyMeasurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propagation models. In this paper the relative abundances of the light nuclei lithium, beryllium, boron and carbon are presented. The secondary to primary ratios Li/C, Be/C and B/C have been measured in the kinetic energy range 0.35-45 GeV/nucleon. The isotopic ratio 7Li/6Li is also determined in the magnetic rigidity interval 2.5-6.3 GV. The secondary to secondary ratios Li/Be, Li/B and Be/B are also reported. These measurements are based on the data collected by the Alpha Magnetic Spectrometer AMS-01 during the STS-91 space shuttle flight in 1998 June. Our experimental results are in substantial agreement with other measurements, where they exist. We describe our light-nuclei data with a diffusive-reacceleration model. A 10-15% overproduction of Be is found in the model predictions and can be attributed to uncertainties in the production cross-section data.Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propagation models. In this paper the relative abundances of the light nuclei lithium, beryllium, boron and carbon are presented. The secondary to primary ratios Li/C, Be/C and B/C have been measured in the kinetic energy range 0.35-45 GeV/nucleon. The isotopic ratio 7Li/6Li is also determined in the magnetic rigidity interval 2.5-6.3 GV. The secondary to secondary ratios Li/Be, Li/B and Be/B are also reported. These measurements are based on the data collected by the Alpha Magnetic Spectrometer AMS-01 during the STS-91 space shuttle flight in 1998 June. Our experimental results are in substantial agreement with other measurements, where they exist. We describe our light-nuclei data with a diffusive-reacceleration model. A 10-15% overproduction of Be is found in the model predictions and can be attributed to uncertainties in the production cross-section data.arXiv:1008.5051oai:cds.cern.ch:12881482010-08-31
spellingShingle Astrophysics and Astronomy
Aguilar, M.
Alcaraz, J.
Allaby, J.
Alpat, B.
Ambrosi, G.
Anderhub, H.
Ao, L.
Arefiev, A.
Arruda, L.
Azzarello, P.
Basile, M.
Barao, F.
Barreira, G.
Bartoloni, A.
Battiston, R.
Becker, R.
Becker, U.
Bellagamba, L.
Bene, P.
Berdugo, J.
Berges, P.
Bertucci, B.
Biland, A.
Bindi, V.
Boella, G.
Boschini, M.
Bourquin, M.
Bruni, G.
Buenerd, M.
Burger, J.D.
Burger, W.J.
Cai, X.D.
Cannarsa, P.
Capell, M.
Casadei, D.
Casaus, J.
Castellini, G.
Cernuda, I.
Chang, Y.H.
Chen, H.F.
Chen, H.S.
Chen, Z.G.
Chernoplekov, N.A.
Chiueh, T.H.
Choi, Y.Y.
Cindolo, F.
Commichau, V.
Contin, A.
Cortina-Gil, E.
Crespo, D.
Cristinziani, M.
Dai, T.S.
de la Guia, C.
Delgado, C.
Di Falco, S.
Djambazov, L.
D'Antone, I.
Dong, Z.R.
Duranti, M.
Engelberg, J.
Eppling, F.J.
Eronen, T.
Extermann, P.
Favier, J.
Fiandrini, E.
Fisher, P.H.
Flugge, G.
Fouque, N.
Galaktionov, Y.
Gervasi, M.
Giovacchini, F.
Giusti, P.
Grandi, D.
Grimm, O.
Gu, W.Q.
Haino, S.
Hangarter, K.
Hasan, A.
Hermel, V.
Hofer, H.
Hungerford, W.
Ionica, M.
Jongmanns, M.
Karlamaa, K.
Karpinski, W.
Kenney, G.
Kim, D.H.
Kim, G.N.
Kim, K.S.
Kirn, T.
Klimentov, A.
Kossakowski, R.
Kounine, A.
Koutsenko, V.
Kraeber, M.
Laborie, G.
Laitinen, T.
Lamanna, G.
Laurenti, G.
Lebedev, A.
Lechanoine-Leluc, C.
Lee, M.W.
Lee, S.C.
Levi, G.
Lin, C.H.
Liu, H.T.
Lu, G.
Lu, Y.S.
Lubelsmeyer, K.
Luckey, D.
Lustermann, W.
Mana, C.
Margotti, A.
Mayet, F.
McNeil, R.R.
Menichelli, M.
Mihul, A.
Mujunen, A.
Oliva, A.
Palmonari, F.
Park, H.B.
Park, W.H.
Pauluzzi, M.
Pauss, F.
Pereira, R.
Perrin, E.
Pevsner, A.
Pilo, F.
Pimenta, M.
Plyaskin, V.
Pojidaev, V.
Pohl, M.
Produit, N.
Quadrani, L.
Rancoita, P.G.
Rapin, D.
Ren, D.
Ren, Z.
Ribordy, M.
Richeux, J.P.
Riihonen, E.
Ritakari, J.
Ro, S.
Roeser, U.
Sagdeev, R.
Santos, D.
Sartorelli, G.
Sbarra, C.
Schael, S.
Schultz von Dratzig, A.
Schwering, G.
Seo, E.S.
Shin, J.W.
Shoumilov, E.
Shoutko, V.
Siedenburg, T.
Siedling, R.
Son, D.
Song, T.
Spada, F.R.
Spinella, F.
Steuer, M.
Sun, G.S.
Suter, H.
Tang, X.W.
Ting, Samuel C.C.
Ting, S.M.
Tomassetti, N.
Tornikoski, M.
Torsti, J.
Trumper, J.
Ulbricht, J.
Urpo, S.
Valtonen, E.
Vandenhirtz, J.
Velikhov, E.
Verlaat, B.
Vetlitsky, I.
Vezzu, F.
Vialle, J.P.
Viertel, G.
Vite, D.
Von Gunten, H.
Waldmeier Wicki, S.
Wallraff, W.
Wang, J.Z.
Wiik, K.
Williams, C.
Wu, S.X.
Xia, P.C.
Xu, S.
Xu, Z.Z.
Yan, J.L.
Yan, L.G.
Yang, C.G.
Yang, J.
Yang, M.
Ye, S.W.
Zhang, H.Y.
Zhang, Z.P.
Zhao, D.X.
Zhou, F.
Zhou, Y.
Zhu, G.Y.
Zhu, W.Z.
Zhuang, H.L.
Zichichi, A.
Zimmermann, B.
Zuccon, P.
Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01
title Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01
title_full Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01
title_fullStr Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01
title_full_unstemmed Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01
title_short Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01
title_sort relative composition and energy spectra of light nuclei in cosmic rays. results from ams-01
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1088/0004-637X/724/1/329
http://cds.cern.ch/record/1288148
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