Results 41 to 50 of about 3,608,924 (307)
Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station.
Physical Review Letters, 2018 We report on the observation of new properties of secondary cosmic rays Li, Be, and B measured in the rigidity (momentum per unit charge) range 1.9 GV to 3.3 TV with a total of 5.4×10^{6} nuclei collected by AMS during the first five years of operation ...M. Aguilar, L. Ali Cavasonza, G. Ambrosi, L. Arruda, N. Attig, S. Aupetit, P. Azzarello, A. Bachlechner, F. Barão, A. Barrau, L. Barrin, A. Bartoloni, L. Basara, S. Başeğmez-du Pree, M. Battarbee, R. Battiston, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, K. F. Bindel, V. Bindi, W. de Boer, K. Bollweg, V. Bonnivard, B. Borgia, M. Boschini, M. Bourquin, E. Bueno, J. Burger, W. Burger, F. Cadoux, X. Cai, M. Capell, S. Caroff, J. Casaus, G. Castellini, F. Cervelli, M. Chae, Y. H. Chang, A. Chen, G. Chen, H. Chen, L. Cheng, H. Chou, E. Choumilov, V. Choutko, C. Chung, C. Clark, R. Clavero, Nicolas Produit, C. Consolandi, A. Contin, C. Corti, W. Creus, M. Crispoltoni, Z. Cui, K. Dadzie, Y. Dai, A. Datta, C. Delgado, S. Della Torre, M. Demirköz, L. Derome, S. Di Falco, F. Dimiccoli, C. Díaz, P. von Doetinchem, F. Dong, F. Donnini, M. Duranti, D. D’Urso, A. Egorov, A. Eline, T. Eronen, J. Feng, E. Fiandrini, P. Fisher, V. Formato, Y. Galaktionov, G. Gallucci, R. García-López, C. Gargiulo, H. Gast, I. Gebauer, M. Gervasi, A. Ghelfi, F. Giovacchini, D. Gómez-Coral, J. Gong, C. Goy, V. Grabski, D. Grandi, M. Graziani, K. Guo, S. Haino, K. Han, Z. H. He, M. Heil, T. Hsieh, H. Huang, Z. Huang, C. Huh, M. Incagli, M. Ionica, W. Jang, Yi Jia, H. Jinchi, S. Kang, K. Kanishev, B. Khiali, G. Kim, K. Kim, T. Kirn, C. Konak, O. Kounina, A. Kounine, V. Koutsenko, A. Kulemzin, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S. Lee, C. Leluc, H. S. Li, J. Li, Q. Li, T. X. Li, Y. Li, Z. Li, Z. Li, S. Lim, C. H. Lin, P. Lipari, T. Lippert, D. Liu, Hu Liu, V. D. Lordello, S. Lu, Y. Lu, K. Luebelsmeyer, F. Luo, J. Luo, S. Lyu, F. Machate, C. Mañá, J. Marin, T. Martin, G. Martinez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, V. Mikuni, D. Mo, P. Mott, T. Nelson, J. Ni, N. Nikonov, F. Nozzoli, A. Oliva, M. Orcinha, M. Palermo, Federico Palmonari, C. Palomares, M. Paniccia, M. Pauluzzi, S. Pensotti, C. Perrina, H. Phan, N. Picot-Clemente, F. Pilo, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, L. Quadrani, X. Qi, X. Qin, Z. Qu, T. Räihä, P. Rancoita, D. Rapin, J. Ricol, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Sagdeev, S. Schael, S. M. Schmidt, A. Schulz von Dratzig, G. Schwering, E. Seo, B. Shan, J. Shi, T. Siedenburg, D. Son, J. Song, M. Tacconi, X. Tang, Z. Tang, D. Tescaro, S. Ting, S. Ting, N. Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, E. Valtonen, M. Vazquez Acosta, M. Vecchi, M. Velasco, J. Vialle, V. Vitale, L. Wang, N. Wang, Q. Wang, X. Wang, X. Wang, Z. Wang, C. Wei, Z. Weng, K. Whitman, H. Wu, X. Wu, R. Xiong, W. Xu, Qi Yan, J. Yang, M. Yang, Y. Yang, H. Yi, Y. Yu, Z. Yu, M. Zannoni, S. Zeissler, C. Zhang, F. Zhang, J. Zhang, J. Zhang, S. Zhang, Z. Zhang, Z. Zheng, H. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon +253 moresemanticscholar +1 more sourceConstraining the $\bar{p}/p$ Ratio in TeV Cosmic Rays with Observations
of the Moon Shadow by HAWC [PDF]
, 2018 An indirect measurement of the antiproton flux in cosmic rays is possible as
the particles undergo deflection by the geomagnetic field. This effect can be
measured by studying the deficit in the flux, or shadow, created by the Moon as
it absorbs cosmic ...Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Alvarez, J. D., Arceo, R., Arroyo, M. Seglar, Arteaga-Velázquez, J. C., Belmont-Moreno, E., BenZvi, S. Y., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., De León, C., de León, S. Coutiño, Dichiara, S., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Engels, K., Enríquez-Rivera, O., Fleischhack, H., Fraija, N., Galván-Gámez, A., García-González, J. A., González, M. M., Goodman, J. A., Greus, F. Salesa, Hampel-Arias, Z., Harding, J. P., Hernandez, R. Diaz, Hernandez, S., Hona, B., Hueyotl-Zahuantitla, F., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., la Fuentem, E. D, Lara, A., Lee, W. H., Linnemann, J. T., Longinotti, A. L., Luis-Raya, G., Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Muñoz, A. González, Nayerhoda, A., Nellena, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Riviére, C., Rojas, D. Avila, Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Solares, H. A. Ayala, Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Vargas, H. León, Villaseñor, L., Weisgarber, T., Westerhoff, S., Wood, J., Yapici, T., Yodha, G. B., Zepeda, A., Zhou, H. +100 morecore +3 more sourcesAntiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station.
Physical Review Letters, 2016 A precision measurement by AMS of the antiproton flux and the antiproton-to-proton flux ratio in primary cosmic rays in the absolute rigidity range from 1 to 450 GV is presented based on 3.49×10^{5} antiproton events and 2.42×10^{9} proton events.M. Aguilar, L. Ali Cavasonza, B. Alpat, G. Ambrosi, L. Arruda, N. Attig, S. Aupetit, P. Azzarello, A. Bachlechner, F. Barão, A. Barrau, L. Barrin, A. Bartoloni, L. Basara, S. Başeğmez-du Pree, M. Battarbee, R. Battiston, J. Bazo, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, V. Bindi, G. Boella, W. de Boer, K. Bollweg, V. Bonnivard, B. Borgia, M. Boschini, M. Bourquin, E. Bueno, J. Burger, F. Cadoux, X. Cai, M. Capell, S. Caroff, J. Casaus, G. Castellini, I. Cernuda, F. Cervelli, M. Chae, Y. H. Chang, A. Chen, G. Chen, H. Chen, L. Cheng, H. Chou, E. Choumilov, V. Choutko, C. Chung, C. Clark, R. Clavero, Nicolas Produit, C. Consolandi, A. Contin, C. Corti, B. Coste, W. Creus, M. Crispoltoni, Z. Cui, Y. Dai, C. Delgado, S. Della Torre, M. Demirköz, L. Derome, S. Di Falco, F. Dimiccoli, C. Díaz, P. von Doetinchem, F. Dong, F. Donnini, M. Duranti, D. D’Urso, A. Egorov, A. Eline, T. Eronen, J. Feng, E. Fiandrini, E. Finch, P. Fisher, V. Formato, Y. Galaktionov, G. Gallucci, B. Garcia, R. García-López, C. Gargiulo, H. Gast, I. Gebauer, M. Gervasi, A. Ghelfi, F. Giovacchini, P. Goglov, D. Gómez-Coral, J. Gong, C. Goy, V. Grabski, D. Grandi, M. Graziani, I. Guerri, K. Guo, M. Habiby, S. Haino, K. Han, Z. H. He, M. Heil, J. Hoffman, T. Hsieh, H. Huang, Z. Huang, C. Huh, M. Incagli, M. Ionica, W. Jang, H. Jinchi, S. Kang, K. Kanishev, G. Kim, K. Kim, T. Kirn, C. Konak, O. Kounina, A. Kounine, V. Koutsenko, Matthew Scott Krafczyk, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S. Lee, C. Leluc, H. S. Li, J. Li, J. Li, Q. Li, T. X. Li, W. Li, Z. Li, Z. Li, S. Lim, C. H. Lin, P. Lipari, T. Lippert, D. Liu, Hu Liu, S. Lu, Y. Lu, K. Luebelsmeyer, F. Luo, J. Luo, S. Lv, R. Majka, C. Mañá, J. Marin, T. Martin, G. Martinez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, D. Mo, L. Morescalchi, P. Mott, T. Nelson, J. Ni, N. Nikonov, F. Nozzoli, P. Nunes, A. Oliva, M. Orcinha, Federico Palmonari, C. Palomares, M. Paniccia, M. Pauluzzi, S. Pensotti, R. Pereira, N. Picot-Clemente, F. Pilo, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, A. Putze, L. Quadrani, X. Qi, X. Qin, Z. Qu, T. Räihä, P. Rancoita, D. Rapin, J. Ricol, I. Rodríguez, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Sagdeev, J. Sandweiss, P. Saouter, S. Schael, S. M. Schmidt, A. Schulz von Dratzig, G. Schwering, E. Seo, B. Shan, J. Shi, T. Siedenburg, D. Son, J. Song, W. Sun, M. Tacconi, X. Tang, Z. Tang, L. Tao, D. Tescaro, S. Ting, S. Ting, N. Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, C. Vannini, E. Valtonen, M. Vazquez Acosta, M. Vecchi, M. Velasco, J. Vialle, V. Vitale, S. Vitillo, L. Wang, N. Wang, Q. Wang, X. Wang, X. Wang, Z. Wang, C. Wei, Z. Weng, K. Whitman, J. Wienkenhöver, M. Willenbrock, H. Wu, X. Wu, X. Xia, R. Xiong, W. Xu, Qi Yan, J. Yang, M. Yang, Y. Yang, H. Yi, Y. Yu, Z. Yu, S. Zeissler, C. Zhang, J. Zhang, J. Zhang, S. Zhang, S. Zhang, Z. Zhang, Z. Zheng, Z. Q. Zhu, H. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon +268 moresemanticscholar +1 more sourceNote on the nature of cosmic rays [PDF]
, 1930 The recent experiments of Bothe and Kolhoerster(1) have led to an important and interesting conclusion. The ionization phenomena, by means of which cosmic rays are measured, are produced by highly penetrating corpuscular rays.Epstein, Paul S.core +1 more sourceARE THERE STRANGELETS IN COSMIC RAYS? [PDF]
International Journal of Modern Physics A, 2005 Assuming that cosmic rays entering the Earth's atmosphere contain a small admixture of nuggets of strange quark matter in form of strangelets one can explain a number of apparently "strange" effects observed in different cosmic rays experiments.Z. Włodarczyk, G. Wilk, M. Rybczyńskiopenaire +3 more sourcesProtostars: Forges of cosmic rays? [PDF]
, 2016 Galactic cosmic rays (CR) are particles presumably accelerated in supernova remnant shocks that propagate in the interstellar medium up to the densest parts of molecular clouds, losing energy and their ionisation efficiency because of the presence of ...M. Padovani, A. Marcowith, P. Hennebelle, K. F. L. U. E. P. D. Montpellier, U. Montpellier, France., Inaf - Arcetri, Firenze, Italy., Cea, Irfu, Sap, C. Saclay, Gif-sur-Yvette, Irap, U. Toulouse +15 moresemanticscholar +1 more source
