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Photovoltaic monitoring system for Auger Muons and Infill for the Ground Array
Energy Science &Engineering, Volume 6, Issue 4, Page 289-305, August 2018., 2018 The characterization of a PV system with solar controllers in parallel is made. The telemetric monitoring system is used, designed for characterizing the PV system. Data analysis of solar radiation and photovoltaic system behavior is made. The PV system is used in the AMIGA project of the Pierre Auger Observatory.Angel Cancio Montbrun, Alexis Mancilla, Javier Maya, Beatriz García, Alejandro Almela, Belén Andrada, Ana M. Botti, Alberto Etchegoyen, Juan M. Figueira, Alan Fuster, Nicolas González, Matías R. Hampel, Ewa Holt, Johannes Hulsman, Mariela Jose Bachuili, Nicolas Leal, Agustín Lucero, Diego Melo, Sarah Müller, Matías Perlin, Manuel Platino, Diego Ravignani, Matias Roncoroni, Federico Sánchez, Christian Sarmiento‐Cano, David Schmidt, Gaia Silli, Federico Suarez, Alvaro Taboada, Oscar Wainberg, Brian Wundheiler, Diana Yelós +31 morewiley +1 more sourceThe rate of cosmic ray showers at large zenith angles: a step towards
the detection of ultra-high energy neutrinos by the Pierre Auger Observatory [PDF]
, 2000 It is anticipated that the Pierre Auger Observatory can be used to detect
cosmic neutrinos of >10^19 eV that arrive at very large zenith angles.A.A. Watson, Antoni, Bird, Capelle, E. Zas, Edge, Engel, Fletcher, J.A. Hinton, Kalmykov, Kalmykov, Kalmykov, Lawrence, M. Ave, Mikamo, Nagano, Nagano, Navarra, R.A. Vázquez, Tennent, Zas +20 morecore +2 more sourcesCapability of the HAWC Gamma‐Ray Observatory for the Indirect Detection of Ultrahigh‐Energy Neutrinos
Advances in Astronomy, Volume 2017, Issue 1, 2017., 2017 The detection of ultrahigh‐energy neutrinos, with energies in the PeV range or above, is a topic of great interest in modern astroparticle physics. The importance comes from the fact that these neutrinos point back to the most energetic particle accelerators in the Universe and provide information about their underlying acceleration mechanisms ...Hermes León Vargas, Andrés Sandoval, Ernesto Belmont, Rubén Alfaro, Dieter Horns +4 morewiley +1 more sourceHighlights from the Pierre Auger Observatory
, 2013 The Pierre Auger Observatory is the world's largest cosmic ray observatory.
Our current exposure reaches nearly 40,000 km$^2$ str and provides us with an
unprecedented quality data set.Aab, A., Abreu, P., Aglietta, M., Aguera, A. Lopez, Ahlers, M., Ahn, E. J., Albarracin, F. Gomez, Albuquerque, I. F. M., Allekotte, I., Allen, J., Allison, P., Almela, A., Alvarez-Muniz, J., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Anjos, J. C. Dos, Antivcic, T., Aramo, C., Arqueros, F., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Badescu, A. M., Baeuml, J., Bahilo, J. Lozano, Barber, K. B., Bardenet, R., Batista, R. Alves, Baus, C., Beatty, J. J., Becker, K. H., Belletoile, A., Bellido, J. A., Benzvi, S., Berat, C., Berg, A. M. Van Den, Berisso, M. Gomez, Bertou, X., Biermann, P. L., Billoir, P., Blanco, F., Blanco, M., Bleve, C., Blumer, H., Bohacova, M., Boncioli, D., Bonifazi, C., Bonino, R., Borodai, N., Brack, J., Brancus, I., Bravo, A. Gascon, Bravo, O. Martinez, Brogueira, P., Brown, W. C., Buchholz, P., Bueno, A., Burton, R. E., Buscemi, M., Caballero-Mora, K. S., Cabo, I. Rodriguez, Caccianiga, B., Caccianiga, L., Candusso, M., Caramete, L., Cardenas, B. Vargas, Caruso, R., Castellina, A., Castillo, J. Alvarez, Castro, M. L. Diaz, Cataldi, G., Cazon, L., Cester, R., Cheng, S. H., Chiavassa, A., Chinellato, J. A., Chudoba, J., Cilmo, M., Clay, R. W., Cocciolo, G., Colalillo, R., Collaboration, For The Pierre Auger, Collica, L., Coluccia, M. R., Conceicao, R., Contreras, F., Cook, H., Cooper, M. J., Coutu, S., Covault, C. E., Criss, A., Cronin, J., Curutiu, A., D'Olivo, J. C., D, J. Knapp, Dallier, Richard, Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., De Almeida, R. M., De Carvalho, W. Rodrigues, De Domenico, M., De Jong, S. J., De La Vega, G., De Mitri, I., De Oliveira, M. A. Leigui, De Souza, V., De Vries, K. D., Del Peral, L., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Diaz, J. C., Diep, P. N., Diogo, F., Dobrigkeit, C., Docters, W., Dong, P. N., Dorofeev, A., Dova, M. T., Ebr, J., Elipe, G. Torralba, Engel, R., Erdmann, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Falcke, H., Falcon, H. R. Marquez, Fang, K., Farrar, G., Fauth, A. C., Fazzini, N., Ferguson, A. P., Fernandez, G. Rodriguez, Fick, B., Figueira, J. M., Filevich, A., Filipcic, A., Foerster, N., Fox, B. D., Fracchiolla, C. E., Fraenkel, E. D., Fratu, O., Frohlich, U., Fuchs, B., Gaior, R., Galicia, J. F. Valdes, Gamarra, R. F., Gambetta, S., Garcia, B., Garcia-Gamez, D., Garcia-Pinto, D., Garilli, G., Gemmeke, H., Ghia, P. L., Giller, M., Gitto, J., Glaser, C., Glass, H., Goncalves, P., Gonzalez, J. G., Gookin, B., Gorgi, A., Gorham, P., Gouffon, P., Grebe, S., Greus, F. Salesa, Griffith, N., Grillo, A. F., Grubb, T. D., Guardincerri, Y., Guarino, F., Guedes, G. P., Hansen, P., Harari, D., Harrison, T. A., Harton, J. L., Haungs, A., Hebbeker, T., Heck, D., Herve, A. E., Hill, G. C., Hoerandel, J. R., Hojvat, C., Hollon, N., Homola, P., Horvath, P., Hrabovsky, M., Huber, D., Huege, T., Insolia, A., Isar, P. G., Jansen, S., Jarne, C., Josebachuili, M., Junior, W. J. M. De Mello, Kadija, K., Kambeitz, O., Kampert, K. H., Karhan, P., Kasper, P., Katkov, I., Kegl, B., Keilhauer, B., Keivani, A., Kemp, E., Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Kroemer, O., Krohm, N., Kruppke-Hansen, D., Kuempel, D., Kunka, N., La Rosa, G., LaHurd, D., Latronico, L., Lauer, R., Lauscher, M., Lautridou, Pascal, Le Coz, S., Leao, M. S. A. B., Lebrun, D., Lebrun, P., Letessier-Selvon, Antoine, Lhenry-Yvon, I., Link, K., Lopez, R., Louedec, K., Lu, L., Lucero, A., Ludwig, M., Luis, P. Facal San, Lyberis, H., Maccarone, M. C., Machado, D. Torres, Macolino, C., Malacari, M., Maldera, S., Maller, J., Mandat, D., Mantsch, P., Mariazzi, A. G., Marin, V., Maris, I. C., Marsella, G., Martello, D., Martin, Lilian, Martinez, H., Martino, J. Rodriguez, Martraire, D., Mathes, H. J., Matthews, J., Matthews, J. A. J., Matthiae, G., Maurel, D., Maurizio, D., Mayotte, E., Mazur, P. O., Medina, C., Medina-Tanco, G., Melissas, M., Melo, D., Menichetti, E., Menshikov, A., Messina, S., Meyhandan, R., Meza, J. J. Masias, Micanovic, S., Micheletti, M. I., Middendorf, L., Minaya, I. A., Miramonti, L., Mitrica, B., Molina-Bueno, L., Mollerach, S., Monasor, M., Montanet, F., Morales, B., Morello, C., Moreno, J. C., Mostafa, M., Moura, C. A., Muller, G., Muller, M. A., Munchmeyer, M., Mussa, R., Navarra, G., Navarro, J. L., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neto, J. R. T. De Mello, Neuser, J., Nhung, P. T., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novzka, L., Oehlschlager, J., Olinto, A., Oliveira, M., Ortiz, M., Pacheco, N., Palatka, M., Pallotta, J., Palmieri, N., Parente, G., Parra, A., Pastor, S., Paul, T., Pech, M., Peixoto, C. J. Todero, Pekala, J., Pelayo, R., Pepe, I. M., Perrone, L., Pesce, R., Petermann, E., Petrera, S., Petrolini, A., Petrov, Y., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Plum, M., Pontz, M., Porcelli, A., Preda, T., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Ragaigne, D. Monnier, Rautenberg, J., Ravel, O., Ravignani, D., Revenu, Benoît, Ridky, J., Riggi, S., Risse, M., Ristori, P., Rivera, H., Rizi, V., Roberts, J., Roca, S. T. Garcia, Rodriguez-Frias, M. D., Rojo, J. Rodriguez, Ros, G., Rosado, J., Rossler, T., Roth, M., Rouille-D'Orfeuil, B., Roulet, E., Rovero, A. C., Ruhle, C., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Salina, G., Sanchez, F., Sanchez-Lucas, P., Santo, C. E., Santos, E., Santos, E. M., Sarazin, F., Sarkar, B., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, A., Scholten, O., Schoorlemmer, H., Schovanek, P., Schroeder, F. G., Schulz, A., Schulz, J., Sciutto, S. J., Scuderi, M., Segreto, A., Selmi-Dei, D. Pakk, Settimo, M., Shadkam, A., Shellard, R. C., Sidelnik, I., Sigl, G., Silva, M. Zimbres, Sima, O., Smialkowski, A., Smida, R., Snow, G. R., Sommers, P., Sorokin, J., Spinka, H., Squartini, R., Srivastava, Y. N., Stanic, S., Stapleton, J., Stasielak, J., Stephan, M., Straub, M., Stutz, A., Suarez, F., Suomijarvi, T., Supanitsky, A. D., Susa, T., Sutherland, M. S., Swain, J., Szadkowski, Z., Szuba, M., Tacscuau, O., Tapia, A., Tartare, M., Tcaciuc, R., Thao, N. T., Tiffenberg, J., Timmermans, C., Tkaczyk, W., Toma, G., Tomankova, L., Tome, B., Tonachini, A., Travnicek, P., Tridapalli, D. B., Trovato, E., Tueros, M., Ulrich, R., Unger, M., Valino, I., Valore, L., Van Aar, G., Van Velzen, S., Van Vliet, A., Varela, E., Varner, G., Vazquez, J. R., Vazquez, R. A., Veberic, D., Verzi, V., Vicha, J., Videla, M., Villasenor, L., Vitale, P. F. Gomez, Wahlberg, H., Wahrlich, P., Wainberg, O., Walz, D., Watson, A. A., Weber, M., Weidenhaupt, K., Weindl, A., Werner, F., Westerhoff, S., Whelan, B. J., Widom, A., Wieczorek, G., Wiencke, L., Wilczynska, B., Wilczynski, H., Will, M., Williams, C., Winchen, T., Wundheiler, B., Wykes, S., Yamamoto, T., Yapici, T., Younk, P., Yuan, G., Yushkov, A., Zamorano, B., Zas, E., Zavrtanik, D., Zavrtanik, M., Zaw, I., Zepeda, A., Zhou, J., Zhu, Y., Ziolkowski, M. +497 morecore +2 more sourcesAbsolute Calibration of a Large-diameter Light Source [PDF]
, 2013 A method of absolute calibration for large aperture optical systems is
presented, using the example of the Pierre Auger Observatory fluorescence
detectors.Brack, J. T., Cope, R., Dorofeev, A., Gookin, B., Harton, J. L., Petrov, Y., Rovero, A. C. +6 morecore +2 more sourcesOn the Impact of Tsallis Statistics on Cosmic Ray Showers
Advances in High Energy Physics, Volume 2016, Issue 1, 2016., 2016 We investigate the impact of the Tsallis nonextensive statistics introduced by intrinsic temperature fluctuations in p‐Air ultrahigh energy interactions on observables of cosmic ray showers, such as the slant depth of the maximum Xmax and the muon number on the ground Nμ. The results show that these observables are significantly affected by temperature M. Abrahão, W. G. Dantas, R. M. de Almeida, D. R. Gratieri, T. J. P. Penna, Sally Seidel +5 morewiley +1 more sourcePierre Auger Observatory: status report [PDF]
Brazilian Journal of Physics, 2004 The Pierre Auger Observatory is a large international effort to provide measurements of extensive air showers (EAS) initiated in the upper atmosphere by cosmic rays with energies above 10 18 eV , the Ultra High Energy Cosmic Rays (UHECR’s). The explanations for the origin, acceleration processes and composition of the UHECR’s face theoretical and ...openaire +3 more sources