Artículos de revistas
Identifying clouds over the Pierre Auger Observatory using infrared satellite data
Registro en:
Astroparticle Physics. Elsevier Science Bv, v. 50-52, n. 92, n. 101, 2013.
0927-6505
1873-2852
WOS:000329271000011
10.1016/j.astropartphys.2013.09.004
Autor
Abreu, P
Aglietta, M
Ahlers, M
Ahn, EJ
Albuquerque, IFM
Allekotte, I
Allen, J
Allison, P
Almela, A
Castillo, JA
Alvarez-Muniz, J
Batista, R
Ambrosio, M
Aminaei, A
Anchordoqui, L
Andringa, S
Anticic, T
Aramo, C
Arqueros, F
Asorey, H
Assis, P
Aublin, J
Ave, M
Avenier, M
Avila, G
Badescu, AM
Barber, KB
Barbosa, AF
Bardenet, R
Baughman, B
Bauml, J
Baus, C
Beatty, JJ
Becker, KH
Belletoile, A
Bellido, JA
BenZvi, S
Berat, C
Bertou, X
Biermann, PL
Billoir, P
Blanco, F
Blanco, M
Bleve, C
Blumer, H
Bohacova, M
Boncioli, D
Bonifazi, C
Bonino, R
Borodai, N
Brack, J
Brancus, I
Brogueira, P
Brown, WC
Buchholz, P
Bueno, A
Buroker, L
Burton, RE
Buscemi, M
Caballero-Mora, KS
Caccianiga, B
Caccianiga, L
Caramete, L
Caruso, R
Castellina, A
Cataldi, G
Cazon, L
Cester, R
Cheng, SH
Chiavassa, A
Chinellato, JA
Chirinos, J
Chudoba, J
Cilmo, M
Clay, RW
Cocciolo, G
Colalillo, R
Collica, L
Coluccia, MR
Conceicao, R
Contreras, F
Cook, H
Cooper, MJ
Coutu, S
Covault, CE
Criss, A
Cronin, J
Curutiu, A
Dallier, R
Daniel, B
Dasso, S
Daumiller, K
Dawson, BR
de Almeida, RM
De Domenico, M
de Jong, SJ
De La Vega, G
de Mello, WJM
Neto, JRTD
De Mitri, I
de Souza, V
de Vries, KD
del Peral, L
Deligny, O
Dembinski, H
Dhital, N
Di Giulio, C
Diaz, JC
Castro, MLD
Diep, PN
Diogo, F
Dobrigkeit, C
Docters, W
D'Olivo, JC
Dong, PN
Dorofeev, A
dos Anjos, JC
Dova, MT
D'Urso, D
Ebr, J
Engel, R
Erdmann, M
Escobar, CO
Espadanal, J
Etchegoyen, A
San Luis, PF
Falcke, H
Fang, K
Farrar, G
Fauth, AC
Fazzini, N
Ferguson, AP
Fick, B
Figueira, JM
Filevich, A
Filipcic, A
Fliescher, S
Fox, BD
Fracchiolla, CE
Fraenkel, ED
Fratu, O
Frohlich, U
Fuchs, B
Gaior, R
Gamarra, RF
Gambetta, S
Garcia, B
Roca, STG
Garcia-Gamez, D
Garcia-Pinto, D
Garilli, G
Bravo, AG
Gemmeke, H
Ghia, PL
Giller, M
Gitto, J
Glaser, C
Glass, H
Golup, G
Albarracin, FG
Berisso, MG
Vitale, PFG
Goncalves, P
Gonzalez, JG
Gookin, B
Gorgi, A
Gorham, P
Gouffon, P
Grebe, S
Griffith, N
Grillo, AF
Grubb, TD
Guardincerri, Y
Guarino, F
Guedes, GP
Hansen, P
Harari, D
Harrison, TA
Harton, JL
Haungs, A
Hebbeker, T
Heck, D
Herve, AE
Hill, GC
Hojvat, C
Hollon, N
Holmes, VC
Homola, P
Horandel, JR
Horvath, P
Hrabovsky, M
Huber, D
Huege, T
Insolia, A
Jansen, S
Jarne, C
Jiraskova, S
Josebachuili, M
Kadija, K
Kampert, KH
Karhan, P
Kasper, P
Katkov, I
Kegl, B
Keilhauer, B
Keivani, A
Kelley, JL
Kemp, E
Kieckhafer, RM
Klages, HO
Kleifges, M
Kleinfeller, J
Knapp, J
Krause, R
Krohm, N
Kromer, O
Kruppke-Hansen, D
Kuempel, D
Kulbartz, JK
Kunka, N
La Rosa, G
LaHurd, D
Latronico, L
Lauer, R
Lauscher, M
Lautridou, P
Le Coz, S
Leao, MSAB
Lebrun, D
Lebrun, P
de Oliveira, MAL
Letessier-Selvon, A
Lhenry-Yvon, I
Link, K
Lopez, R
Aguera, AL
Louedec, K
Bahilo, JL
Lu, L
Lucero, A
Ludwig, M
Lyberis, H
Maccarone, MC
Macolino, C
Malacari, M
Maldera, S
Maller, J
Mandat, D
Mantsch, P
Mariazzi, AG
Marin, J
Marin, V
Maris, IC
Falcon, HRM
Marsella, G
Martello, D
Martin, L
Martinez, H
Bravo, OM
Martraire, D
Meza, JJM
Mathes, HJ
Matthews, J
Matthews, JAJ
Matthiae, G
Maurel, D
Maurizio, D
Mayotte, E
Mazur, PO
Medina-Tanco, G
Melissas, M
Melo, D
Menichetti, E
Menshikov, A
Messina, S
Meyhandan, R
Micanovic, S
Micheletti, MI
Middendorf, L
Minaya, IA
Mirarrionti, L
Mitrica, B
Molina-Bueno, L
Mollerach, S
Monasor, M
Ragaigne, DM
Montanet, F
Morales, B
Morello, C
Moreno, JC
Mostafa, M
Moura, CA
Muller, MA
Muller, G
Munchmeyer, M
Mussa, R
Navarra, G
Navarro, JL
Navas, S
Necesal, P
Nellen, L
Nelles, A
Neuser, TJ
Nhung, PT
Niechciol, M
Niemietz, L
Nierstenhoefer, N
Niggemann, T
Nitz, D
Nosek, D
Nozka, L
Oehlschlager, J
Olinto, A
Oliveira, M
Ortiz, M
Pacheco, N
Selmi-Dei, DP
Palatka, M
Pallotta, J
Palmieri, N
Parente, G
Parra, A
Pastor, S
Paul, T
Pech, M
Pekala, J
Pelayo, R
Pepe, IM
Perrone, L
Pesce, R
Petermann, E
Petrera, S
Petrolini, A
Petrov, Y
Pfendner, C
Piegaia, R
Pierog, T
Pieroni, P
Pimenta, M
Pirronello, V
Platino, M
Plum, M
Ponce, VH
Pontz, M
Porcelli, A
Privitera, P
Prouza, M
Quel, EJ
Querchfeld, S
Rautenberg, J
Ravel, O
Ravignani, D
Revenu, B
Ridky, J
Riggi, S
Risse, M
Ristori, P
Rivera, H
Rizi, V
Roberts, J
de Carvalho, WR
Cabo, IR
Fernandez, GR
Martino, JR
Rojo, JR
Rodriguez-Frias, MD
Ros, G
Rosado, J
Rossler, T
Roth, M
Rouille-d'Orfeuil, B
Roulet, E
Rovero, AC
Ruhle, C
Saffi, SJ
Saftoiu, A
Salamida, F
Salazar, H
Greus, FS
Salina, G
Sanchez, F
Santo, CE
Santos, E
Santos, EM
Sarazin, F
Sarkar, B
Sato, R
Scharf, N
Scherini, V
Schieler, H
Schiffer, P
Schmidt, A
Scholten, O
Schoorlemmer, H
Schovancova, J
Schovanek, P
Schroder, FG
Schulz, J
Schuster, D
Sciutto, S
Scuderi, M
Segreto, A
Settimo, M
Shadkam, A
Shellard, RC
Sidelnik, I
Sigl, G
Sima, O
Smialkowski, A
Smida, R
Snow, GR
Sommers, P
Sorokin, J
Spinka, H
Squartini, R
Srivastava, YN
Stanic, S
Stapleton, J
Stasielak, J
Stephan, M
Straub, M
Stutz, A
Suarez, F
Suomijarvi, T
Supanitsky, AD
Susa, T
Sutherland, MS
Swain, J
Szadkowski, Z
Szuba, M
Tapia, A
Tartare, M
Tascau, O
Tcaciuc, R
Thao, NT
Thomas, D
Tiffenberg, J
Timmermans, C
Tkaczyk, W
Peixoto, CJT
Toma, G
Tomankova, L
Tome, B
Tonachini, A
Elipe, GT
Machado, DT
Travnicek, P
Tridapalli, DB
Trovato, E
Tueros, M
Ulrich, R
Unger, M
Urban, M
Galicia, JFV
Valino, I
Valore, L
van Aar, G
van den Berg, AM
van Velzen, S
van Vliet, A
Varela, E
Cardenas, BV
Varner, G
Vazquez, JR
Vazquez, RA
Veberic, D
Verzi, V
Vicha, J
Videla, M
Villasenor, L
Wahlberg, H
Wahrlich, P
Wainberg, O
Walz, D
Watson, AA
Weber, M
Weidenhaupt, K
Weindl, A
Werner, F
Westerhoff, S
Whelan, BJ
Widom, A
Wieczorek, G
Wiencke, L
Wilczynska, B
Wilczynski, H
Will, M
Williams, C
Winchen, T
Wundheiler, B
Yamamoto, T
Yapici, T
Younk, P
Yuan, G
Yushkov, A
Garcia, BZ
Zas, E
Zavrtanik, D
Zavrtanik, M
Zaw, I
Zepeda, A
Zhou, J
Zhu, Y
Silva, MZ
Ziolkowski, M
Institución
Resumen
We describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud. identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km(2) of the Pierre Auger Observatory twice per hour with a spatial resolution of similar to 2.4 km by similar to 5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories. (C) 2013 Elsevier B.V. All rights reserved. 50-52 92 101 Comision Nacional de Energia Atomica Fundacion Antorchas Gobierno De La Provincia de Mendoza Municipalidad de Malargue