Results 21 to 30 of about 121,402 (277)

Modeling the optical Cherenkov signals by cosmic ray extensive air showers directly observed from suborbital and orbital altitudes [PDF]

Physical Review D, 2021
A.L. Cummings, 2 R. Aloisio, 2 J.Eser, and J.F. Krizmanic 5 Gran Sasso Science Institute (GSSI), L’Aquila 67100, Italy INFN-Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67010, Italy Department of Astronomy & Astrophysics, University of Chicago ...
A. Cummings, R. Aloisio, J. Eser, J. Krizmanic   +3 more
semanticscholar   +1 more source

Simulation of radiopulses from Atmosphere-Skimming Extensive Air Showers with ZHAireS-RASPASS

Arena, 2023
Earth-skimming neutrinos and Atmosphere-skimming neutrinos or cosmic rays can induce extensive air showers that present some peculiarities in comparison to the better-characterized down-going showers.
M. Tueros
semanticscholar   +1 more source

First Results on the Revealing of Cognate Ancestors among the Particles of the Primary Cosmic Rays That Gave Rise to Extensive Air Showers Observed by the GELATICA Network

Symmetry, 2022
For the data on the observation times and directions of the motion of extensive air showers, which are observed at two stations of the GELATICA network, for the first time we apply the method we have developed previously for identifying pairs of mutually
Yuri Verbetsky, M. Svanidze, O. Ruimi, T. Wibig, L. Kakabadze, P. Homola, D. Alvarez-Castillo, D. Beznosko, E. Sarkisyan-Grinbaum, O. Bar, O. Sushchov, A. Tursunov   +11 more
semanticscholar   +1 more source

Modeling of the tau and muon neutrino-induced optical Cherenkov signals from upward-moving extensive air showers [PDF]

Physical Review D, 2020
We present a detailed modeling and computation methodology to determine the optical Cherenkov signals produced by upward-moving extensive air showers (EASs) induced by $\ensuremath{\tau}$-leptons and muons, sourced from the interaction of high-energy ...
A. Cummings, R. Aloisio, J. Krizmanic
semanticscholar   +1 more source

Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory [PDF]

, 2009
Atmospheric parameters, such as pressure (P), temperature (T) and density, affect the development of extensive air showers initiated by energetic cosmic rays.
A. Anzalone, A. Bellétoile, A. Bueno, A. Castellina, A. Chiavassa, A. Chou, A. Cordier, A. Creusot, A. Criss, A. Curutiu, A. Della Selva, A. Dorofeev, A. Etchegoyen, A. Ferrero, A. Filevich, A. Filipčič, A. Gorgi, A. Haungs, A. Horneffer, A. Insolia, A. Italiano, A. Krieger, A. Kusenko, A. Lemiere, A. Letessier-Selvon, A. Lopez Agüera, A. Lucero, A. Menshikov, A. Olinto, A. Petrolini, A. Redondo, A. Rouillé-d’Orfeuil, A. Schmidt, A. Segreto, A. Smiałkowski, A. Stutz, A. Tamashiro, A. Tamburro, A. Tonachini, A. Velarde, A. Zepeda, A.A. Watson, A.C. Fauth, A.C. Rovero, A.D. Supanitsky, A.F. Barbosa, A.F. Grillo, A.G. Mariazzi, A.M. van den Berg, Abraham, Abraham, Allekotte, B. Baughman, B. Connolly, B. Fick, B. García, B. Keilhauer, B. Kégl, B. Morales, B. Revenu, B. Tomé, B. Wilczyńska, B. Wundheiler, B.B. Siffert, B.E. Smith, B.J. Whelan, B.L. Lago, B.R. Becker, B.R. Dawson, C. Aguirre, C. Aramo, C. Berat, C. Bleve, C. Bonifazi, C. De Donato, C. Delle Fratte, C. Di Giulio, C. Dobrigkeit, C. Hojvat, C. Lachaud, C. Macolino, C. Morello, C. Morris, C. Newman-Holmes, C. Pfendner, C. Rivière, C. Robledo, C. Timmermans, C. Wileman, C.A. Moura, C.E. Covault, C.E. Fracchiolla, C.E. Santo, C.J. Todero Peixoto, C.O. Escobar, D. Allard, D. Badagnani, D. Dornic, D. D’Urso, D. Garcia-Pinto, D. García Gámez, D. Gonzalez, D. Góra, D. Harari, D. Heck, D. Kruppke-Hansen, D. Kuempel, D. Lebrun, D. Mandat, D. Martello, D. Maurizio, D. Melo, D. Monnier Ragaigne, D. Newton, D. Nitz, D. Nosek, D. Pakk Selmi-Dei, D. Ravignani, D. Schuster, D. Semikoz, D. Tcherniakhovski, D. Thomas, D. Veberič, D. Warner, D. Zavrtanik, D.-H. Koang, D.B. Tridapalli, E. Arganda, E. Colombo, E. Grashorn, E. Kemp, E. Menichetti, E. Parizot, E. Petermann, E. Roulet, E. Strazzeri, E. Trovato, E. Zas, E.D. Fraenkel, E.J. Ahn, E.J. Quel, E.M. Santos, Engel, F. Arneodo, F. Arqueros, F. Blanco, F. Contreras, F. Ferrer, F. Gomez Albarracin, F. Guarino, F. Ionita, F. Montanet, F. Ortolani, F. Salamida, F. Sarazin, F. Schmidt, F. Schroeder, F. Schüssler, F. Suarez, F. Sánchez, F.A.S. Rezende, Fletcher, G. Avila, G. De La Vega, G. Decerprit, G. Farrar, G. Gelmini, G. Golup, G. Hebrero, G. La Rosa, G. Matthiae, G. Medina-Tanco, G. Miele, G. Navarra, G. Parente, G. Rodriguez, G. Ros, G. Salina, G. Tristram, G. Wieczorek, G. Yuan, G.P. Guedes, G.R. Snow, Greisen, H. Asorey, H. Blümer, H. Dembinski, H. Falcke, H. Gemmeke, H. Glass, H. Lyberis, H. Salazar, H. Schieler, H. Schoorlemmer, H. Spinka, H. Wahlberg, H. Wilczyński, H. Wu, H.J. Mathes, H.O. Klages, H.R. Marquez Falcon, Hillas, I. Allekotte, I. De Mitri, I. Dutan, I. Fleck, I. Lhenry-Yvon, I. Rodriguez-Cabo, I. Sidelnik, I. Torres, I. Valiño, I. Zaw, I.C. Maris, I.M. Pepe, J. Abraham, J. Allen, J. Alvarez-Muñiz, J. Aublin, J. Brack, J. Chauvin, J. Chudoba, J. Chye, J. Coppens, J. Cronin, J. Gutiérrez, J. Kleinfeller, J. Knapp, J. Lee, J. Lozano Bahilo, J. Martínez, J. Matthews, J. Oehlschläger, J. Pallotta, J. Petrovic, J. Pe¸kala, J. Pochon, J. Rautenberg, J. Ridky, J. Rodriguez Martino, J. Rodriguez Rojo, J. Rosado, J. Schovancova, J. Sorokin, J. Swain, J. Tiffenberg, J.A. Bellido, J.A. Chinellato, J.A.J. Matthews, J.C. Diaz, J.C. dos Anjos, J.C. D’Olivo, J.C. Moreno, J.D. Hague, J.F. Valdés Galicia, J.G. Gonzalez, J.J. Beatty, J.L. Harton, J.L. Navarro, J.R. Hörandel, J.R. Vázquez, J.R.T. de Mello Neto, K. Arisaka, K. Daumiller, K. Louedec, K. Payet, K.B. Barber, K.D. de Vries, K.H. Becker, K.H. Kampert, K.S. Caballero-Mora, Kamata, Keilhauer, Keilhauer, Kobal, L. Anchordoqui, L. Caramete, L. Cazon, L. del Peral, L. Miramonti, L. Nellen, L. Nožka, L. Perrone, L. Valore, L. Villaseñor, L. Voyvodic, L. Wiencke, L.M. Goggin, M. Aglietta, M. Ambrosio, M. Ave, M. Boháčová, M. De Domenico, M. Erdmann, M. Giller, M. Gonçalves do Amaral, M. Grigat, M. Gómez Berisso, M. Hrabovský, M. Hussain, M. Iarlori, M. Kaducak, M. Kleifges, M. Leuthold, M. McEwen, M. Melissas, M. Monasor, M. Mostafá, M. Nyklicek, M. Ortiz, M. Palatka, M. Patel, M. Pech, M. Pimenta, M. Platino, M. Pontz, M. Prouza, M. Risse, M. Roth, M. Santander, M. Scuderi, M. Settimo, M. Tueros, M. Unger, M. Urban, M. Videla, M. Zavrtanik, M. Ziolkowski, M.A. DuVernois, M.A. Leigui de Oliveira, M.A. Muller, M.C. Maccarone, M.D. Healy, M.D. Rodríguez-Frías, M.G. Winnick, M.I. Micheletti, M.S. Gold, M.S. Sutherland, M.S.A.B. Leão, M.T. Dova, N. Borodai, N. Fazzini, N. Kunka, N. Nierstenhoefer, N. Pacheco, N. Scharf, N.G. Busca, N.T. Thao, Newton, O. Blanch-Bigas, O. Catalano, O. Deligny, O. Krömer, O. Martínez Bravo, O. Pisanti, O. Ravel, O. Scholten, O. Taşcău, O. Wainberg, Ostapchenko, P. Abreu, P. Allison, P. Assis, P. Bauleo, P. Bernardini, P. Billoir, P. Brogueira, P. Buchholz, P. Facal San Luis, P. Gonçalves, P. Gouffon, P. Hansen, P. Homola, P. Kasper, P. Lautridou, P. Lebrun, P. Mantsch, P. Necesal, P. Oliva, P. Petrinca, P. Privitera, P. Schiffer, P. Schovánek, P. Sommers, P. Travnicek, P. Wahrlich, P. Younk, P.L. Biermann, P.L. Ghia, P.N. Diep, P.N. Dong, P.O. Mazur, P.T. Nhung, R. Bonino, R. Bruijn, R. Caruso, R. Cester, R. Conceição, R. Dallier, R. Engel, R. Knapik, R. Luna García, R. López, R. Meyhandan, R. Mussa, R. Pelayo, R. Pesce, R. Piegaia, R. Sato, R. Squartini, R. Tcaciuc, R. Ticona, R. Ulrich, R. Šmída, R.A. Vázquez, R.C. Shellard, R.E. Burton, R.F. Gamarra, R.M. de Almeida, R.M. Kieckhafer, R.R. McNeil, R.W. Clay, S. Andringa, S. Argirò, S. BenZvi, S. Coutu, S. Dagoret-Campagne, S. Fliescher, S. Gambetta, S. Grebe, S. Harmsma, S. Jiraskova, S. Maldera, S. Mollerach, S. Mueller, S. Navas, S. Parlati, S. Pastor, S. Petrera, S. Reucroft, S. Riggi, S. Sarkar, S. Schulte, S. Vorobiov, S. Westerhoff, S.J. de Jong, S.J. Sciutto, S.L.C. Barroso, Schmidt, T. Asch, T. Beau, T. Bäcker, T. Hebbeker, T. Huege, T. Karova, T. Paul, T. Pierog, T. Pinto, T. Rossler, T. Schmidt, T. Suomijärvi, T. Tarutina, T. Venters, T. Yamamoto, U. Cotti, U. Giaccari, V. de Souza, V. Halenka, V. Pavlidou, V. Pirronello, V. Rizi, V. Scherini, V. Tuci, V. Verzi, V.C. Holmes, V.H. Ponce, V.M. Olmos-Gilbaja, W. Carvalho, W. Fulgione, W. Miller, W. Tkaczyk, W.C. Brown, W.J.M. de Mello, X. Bertou, X. Garrido, Y. Guardincerri, Y. Petrov, Z. Szadkowski   +486 more
core   +14 more sources

Neutron production in extensive air showers

International Conference on Rebooting Computing, 2021
We use the Monte Carlo simulation package FLUKA to study the production of neutrons in extensive air showers. In contrast to typical shower simulations, we consider the full range of neutron energies extending down to thermal neutrons.
R. Engel, A. Ferrari, M. Roth, M. Schimassek, D. Schmidt, D. Veberič   +5 more
semanticscholar   +1 more source

Synthesis of radio signals from extensive air showers using previously computed microscopic simulations [PDF]

Journal of Instrumentation, 2020
The detection of extensive air showers (EAS) through their radio signal is becoming one of the most promising techniques for the study of neutrinos and cosmic rays at the highest energies. For the design, optimization and characterization of radio arrays
Matías Tueros, A. Zilles
semanticscholar   +1 more source

Measurements of Horizontal Air Showers with the Auger Engineering Radio Array [PDF]

EPJ Web of Conferences, 2019
The Pierre Auger Observatory is the largest observatory for the detection of cosmic rays. With the Auger Engineering Radio Array (AERA) we measure the emitted radio signal of extensive air showers and reconstruct properties of the primary cosmic rays ...
Gottowik Marvin
doaj   +1 more source

Determination of the Cosmic-Ray Chemical Composition: Open Issues and Prospects

Galaxies, 2022
Cosmic rays are relativistic particles that come to the Earth from outer space. Despite a great effort made in both experimental and theoretical research, their origin is still unknown. One of the main keys to understand their nature is the determination
Alberto Daniel Supanitsky
doaj   +1 more source

Hadronic interaction model sibyll 2.3d and extensive air showers

Physical Review D, 2020
We present a new version of the hadron interaction event generator sibyll. While the core ideas of the model have been preserved, the new version handles the production of baryon pairs and leading particles in a new way.
F. Riehn, R. Engel, A. Fedynitch, T. Gaisser, T. Stanev   +4 more
semanticscholar   +1 more source