The atmospheric monitoring system of the JEM-EUSO instrument
Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the pr...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Adams, J. H. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media Dordrecht 2014 |
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| Übergeordnetes Werk: |
Enthalten in: Experimental astronomy - Springer Netherlands, 1989, 40(2014), 1 vom: 23. Juli, Seite 45-60 |
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| Übergeordnetes Werk: |
volume:40 ; year:2014 ; number:1 ; day:23 ; month:07 ; pages:45-60 |
| Links: |
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| DOI / URN: |
10.1007/s10686-014-9378-1 |
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| Katalog-ID: |
OLC2042944602 |
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| 100 | 1 | |a Adams, J. H. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a The atmospheric monitoring system of the JEM-EUSO instrument |
| 264 | 1 | |c 2014 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 500 | |a © Springer Science+Business Media Dordrecht 2014 | ||
| 520 | |a Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. | ||
| 650 | 4 | |a Ultra high energy cosmic rays | |
| 650 | 4 | |a Atmospheric monitoring | |
| 650 | 4 | |a IR camera | |
| 650 | 4 | |a LIDAR | |
| 700 | 1 | |a Ahmad, S. |4 aut | |
| 700 | 1 | |a Albert, J. -N. |4 aut | |
| 700 | 1 | |a Allard, D. |4 aut | |
| 700 | 1 | |a Anchordoqui, L. |4 aut | |
| 700 | 1 | |a Andreev, V. |4 aut | |
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| 700 | 1 | |a Bellotti, R. |4 aut | |
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| 700 | 1 | |a Bonamente, M. |4 aut | |
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| 773 | 0 | 8 | |i Enthalten in |t Experimental astronomy |d Springer Netherlands, 1989 |g 40(2014), 1 vom: 23. Juli, Seite 45-60 |w (DE-627)130767123 |w (DE-600)1001704-5 |w (DE-576)023036176 |x 0922-6435 |7 nnns |
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10.1007/s10686-014-9378-1 doi (DE-627)OLC2042944602 (DE-He213)s10686-014-9378-1-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Adams, J. H. verfasserin aut The atmospheric monitoring system of the JEM-EUSO instrument 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. Ultra high energy cosmic rays Atmospheric monitoring IR camera LIDAR Ahmad, S. aut Albert, J. -N. aut Allard, D. aut Anchordoqui, L. aut Andreev, V. aut Anzalone, A. aut Arai, Y. aut Asano, K. aut Ave Pernas, M. aut Baragatti, P. aut Barrillon, P. aut Batsch, T. aut Bayer, J. aut Bechini, R. aut Belenguer, T. aut Bellotti, R. aut Belov, K. aut Berlind, A. A. aut Bertaina, M. aut Biermann, P. L. aut Biktemerova, S. aut Blaksley, C. aut Blanc, N. aut Błȩcki, J. aut Blin-Bondil, S. aut Blümer, J. aut Bobik, P. aut Bogomilov, M. aut Bonamente, M. aut Briggs, M. S. aut Briz, S. aut Bruno, A. aut Cafagna, F. aut Campana, D. aut Capdevielle, J. -N. aut Caruso, R. aut Casolino, M. aut Cassardo, C. aut Castellinic, G. aut Catalano, C. aut Catalano, G. aut Cellino, A. aut Chikawa, M. aut Christl, M. J. aut Cline, D. aut Connaughton, V. aut Conti, L. aut Cordero, G. aut Crawford, H. J. aut Cremonini, R. aut Csorna, S. aut Dagoret-Campagne, S. aut de Castro, A. J. aut De Donato, C. aut de la Taille, C. aut De Santis, C. aut del Peral, L. aut Dell’Oro, A. aut De Simone, N. aut Di Martino, M. aut Distratis, G. aut Dulucq, F. aut Dupieux, M. aut Ebersoldt, A. aut Ebisuzaki, T. aut Engel, R. aut Falk, S. aut Fang, K. aut Fenu, F. aut Fernández-Gómez, I. aut Ferrarese, S. aut Finco, D. aut Flamini, M. aut Fornaro, C. aut Franceschi, A. aut Fujimoto, J. aut Fukushima, M. aut Galeotti, P. aut Garipov, G. aut Geary, J. aut Gelmini, G. aut Giraudo, G. aut Gonchar, M. aut González Alvarado, C. aut Gorodetzky, P. aut Guarino, F. aut Guzmán, A. aut Hachisu, Y. aut Harlov, B. aut Haungs, A. aut Hernández Carretero, J. aut Higashide, K. aut Ikeda, D. aut Ikeda, H. aut Inoue, N. aut Inoue, S. aut Insolia, A. aut Isgrò, F. aut Itow, Y. aut Joven, E. aut Judd, E. G. aut Jung, A. aut Kajino, F. aut Kajino, T. aut Kaneko, I. aut Karadzhov, Y. aut Karczmarczyk, J. aut Karus, M. aut Katahira, K. aut Kawai, K. aut Kawasaki, Y. aut Keilhauer, B. aut Khrenov, B. A. aut Kim, J. -S. aut Kim, S. -W. aut Kim, S. -W. aut Kleifges, M. aut Klimov, P. A. aut Kolev, D. aut Kreykenbohm, I. aut Kudela, K. aut Kurihara, Y. aut Kusenko, A. aut Kuznetsov, E. aut Lacombe, M. aut Lachaud, C. aut Lee, J. aut Licandro, J. aut Lim, H. aut López, F. aut Maccarone, M. C. aut Mannheim, K. aut Maravilla, D. aut Marcelli, L. aut Marini, A. aut Martinez, O. aut Masciantonio, G. aut Mase, K. aut Matev, R. aut Medina-Tanco, G. aut Mernik, T. aut Miyamoto, H. aut Miyazaki, Y. aut Mizumoto, Y. aut Modestino, G. aut Monaco, A. aut Monnier-Ragaigne, D. aut Morales de los Ríos, J. A. aut Moretto, C. aut Morozenko, V. S. aut Mot, B. aut Murakami, T. aut Murakami, M. Nagano aut Nagata, M. aut Nagataki, S. aut Nakamura, T. aut Napolitano, T. aut Naumov, D. aut Nava, R. aut Neronov, A. aut Nomoto, K. aut Nonaka, T. aut Ogawa, T. aut Ogio, S. aut Ohmori, H. aut Olinto, A. V. aut Orleański, P. aut Osteria, G. aut Panasyuk, M. I. aut Parizot, E. aut Park, I. H. aut Park, H. W. aut Pastircak, B. aut Patzak, T. aut Paul, T. aut Pennypacker, C. aut Perez Cano, S. aut Peter, T. aut Picozza, P. aut Pierog, T. aut Piotrowski, L. W. aut Piraino, S. aut Plebaniak, Z. aut Pollini, A. aut Prat, P. aut Prévôt, G. aut Prieto, H. aut Putis, M. aut Reardon, P. aut Reyes, M. aut Ricci, M. aut Rodríguez, I. aut Rodríguez Frías, M. D. aut Ronga, F. aut Roth, M. aut Rothkaehl, H. aut Roudil, G. aut Rusinov, I. aut Rybczyński, M. aut Sabau, M. D. aut Sáez-Cano, G. aut Sagawa, H. aut Saito, A. aut Sakaki, N. aut Sakata, M. aut Salazar, H. aut Sánchez, S. aut Santangelo, A. aut Santiago Crúz, L. aut Sanz Palomino, M. aut Saprykin, O. aut Sarazin, F. aut Sato, H. aut Sato, M. aut Schanz, T. aut Schieler, H. aut Scotti, V. aut Segreto, A. aut Selmane, S. aut Semikoz, D. aut Serra, M. aut Sharakin, S. aut Shibata, T. aut Shimizu, H. M. aut Shinozaki, K. aut Shirahama, T. aut Siemieniec-Oziȩbło, G. aut Silva López, H. H. aut Sledd, J. aut Słomińska, K. aut Sobey, A. aut Sugiyama, T. aut Supanitsky, D. aut Suzuki, M. aut Szabelska, B. aut Szabelski, J. aut Tajima, F. aut Tajima, N. aut Tajima, T. aut Takahashi, Y. aut Takami, H. aut Takeda, M. aut Takizawa, Y. aut Tenzer, C. aut Tibolla, O. aut Tkachev, L. aut Tokuno, H. aut Tomida, T. aut Tone, N. aut Toscano, S. aut Trillaud, F. aut Tsenov, R. aut Tsunesada, Y. aut Tsuno, K. aut Tymieniecka, T. aut Uchihori, Y. aut Unger, M. aut Vaduvescu, O. aut Valdés-Galicia, J. F. aut Vallania, P. aut Valore, L. aut Vankova, G. aut Vigorito, C. aut Villaseñor, L. aut von Ballmoos, P. aut Wada, S. aut Watanabe, J. aut Watanabe, S. aut Watts, J. aut Weber, M. aut Weiler, T. J. aut Wibig, T. aut Wiencke, L. aut Wille, M. aut Wilms, J. aut Włodarczyk, Z. aut Yamamoto, T. aut Yamamoto, Y. aut Yang, J. aut Yano, H. aut Yashin, I. V. aut Yonetoku, D. aut Yoshida, K. aut Yoshida, S. aut Young, R. aut Zotov, M. Yu. aut Zuccaro Marchi, A. aut Enthalten in Experimental astronomy Springer Netherlands, 1989 40(2014), 1 vom: 23. Juli, Seite 45-60 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:40 year:2014 number:1 day:23 month:07 pages:45-60 https://doi.org/10.1007/s10686-014-9378-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_4012 39.00 VZ AR 40 2014 1 23 07 45-60 |
| spelling |
10.1007/s10686-014-9378-1 doi (DE-627)OLC2042944602 (DE-He213)s10686-014-9378-1-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Adams, J. H. verfasserin aut The atmospheric monitoring system of the JEM-EUSO instrument 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. Ultra high energy cosmic rays Atmospheric monitoring IR camera LIDAR Ahmad, S. aut Albert, J. -N. aut Allard, D. aut Anchordoqui, L. aut Andreev, V. aut Anzalone, A. aut Arai, Y. aut Asano, K. aut Ave Pernas, M. aut Baragatti, P. aut Barrillon, P. aut Batsch, T. aut Bayer, J. aut Bechini, R. aut Belenguer, T. aut Bellotti, R. aut Belov, K. aut Berlind, A. A. aut Bertaina, M. aut Biermann, P. L. aut Biktemerova, S. aut Blaksley, C. aut Blanc, N. aut Błȩcki, J. aut Blin-Bondil, S. aut Blümer, J. aut Bobik, P. aut Bogomilov, M. aut Bonamente, M. aut Briggs, M. S. aut Briz, S. aut Bruno, A. aut Cafagna, F. aut Campana, D. aut Capdevielle, J. -N. aut Caruso, R. aut Casolino, M. aut Cassardo, C. aut Castellinic, G. aut Catalano, C. aut Catalano, G. aut Cellino, A. aut Chikawa, M. aut Christl, M. J. aut Cline, D. aut Connaughton, V. aut Conti, L. aut Cordero, G. aut Crawford, H. J. aut Cremonini, R. aut Csorna, S. aut Dagoret-Campagne, S. aut de Castro, A. J. aut De Donato, C. aut de la Taille, C. aut De Santis, C. aut del Peral, L. aut Dell’Oro, A. aut De Simone, N. aut Di Martino, M. aut Distratis, G. aut Dulucq, F. aut Dupieux, M. aut Ebersoldt, A. aut Ebisuzaki, T. aut Engel, R. aut Falk, S. aut Fang, K. aut Fenu, F. aut Fernández-Gómez, I. aut Ferrarese, S. aut Finco, D. aut Flamini, M. aut Fornaro, C. aut Franceschi, A. aut Fujimoto, J. aut Fukushima, M. aut Galeotti, P. aut Garipov, G. aut Geary, J. aut Gelmini, G. aut Giraudo, G. aut Gonchar, M. aut González Alvarado, C. aut Gorodetzky, P. aut Guarino, F. aut Guzmán, A. aut Hachisu, Y. aut Harlov, B. aut Haungs, A. aut Hernández Carretero, J. aut Higashide, K. aut Ikeda, D. aut Ikeda, H. aut Inoue, N. aut Inoue, S. aut Insolia, A. aut Isgrò, F. aut Itow, Y. aut Joven, E. aut Judd, E. G. aut Jung, A. aut Kajino, F. aut Kajino, T. aut Kaneko, I. aut Karadzhov, Y. aut Karczmarczyk, J. aut Karus, M. aut Katahira, K. aut Kawai, K. aut Kawasaki, Y. aut Keilhauer, B. aut Khrenov, B. A. aut Kim, J. -S. aut Kim, S. -W. aut Kim, S. -W. aut Kleifges, M. aut Klimov, P. A. aut Kolev, D. aut Kreykenbohm, I. aut Kudela, K. aut Kurihara, Y. aut Kusenko, A. aut Kuznetsov, E. aut Lacombe, M. aut Lachaud, C. aut Lee, J. aut Licandro, J. aut Lim, H. aut López, F. aut Maccarone, M. C. aut Mannheim, K. aut Maravilla, D. aut Marcelli, L. aut Marini, A. aut Martinez, O. aut Masciantonio, G. aut Mase, K. aut Matev, R. aut Medina-Tanco, G. aut Mernik, T. aut Miyamoto, H. aut Miyazaki, Y. aut Mizumoto, Y. aut Modestino, G. aut Monaco, A. aut Monnier-Ragaigne, D. aut Morales de los Ríos, J. A. aut Moretto, C. aut Morozenko, V. S. aut Mot, B. aut Murakami, T. aut Murakami, M. Nagano aut Nagata, M. aut Nagataki, S. aut Nakamura, T. aut Napolitano, T. aut Naumov, D. aut Nava, R. aut Neronov, A. aut Nomoto, K. aut Nonaka, T. aut Ogawa, T. aut Ogio, S. aut Ohmori, H. aut Olinto, A. V. aut Orleański, P. aut Osteria, G. aut Panasyuk, M. I. aut Parizot, E. aut Park, I. H. aut Park, H. W. aut Pastircak, B. aut Patzak, T. aut Paul, T. aut Pennypacker, C. aut Perez Cano, S. aut Peter, T. aut Picozza, P. aut Pierog, T. aut Piotrowski, L. W. aut Piraino, S. aut Plebaniak, Z. aut Pollini, A. aut Prat, P. aut Prévôt, G. aut Prieto, H. aut Putis, M. aut Reardon, P. aut Reyes, M. aut Ricci, M. aut Rodríguez, I. aut Rodríguez Frías, M. D. aut Ronga, F. aut Roth, M. aut Rothkaehl, H. aut Roudil, G. aut Rusinov, I. aut Rybczyński, M. aut Sabau, M. D. aut Sáez-Cano, G. aut Sagawa, H. aut Saito, A. aut Sakaki, N. aut Sakata, M. aut Salazar, H. aut Sánchez, S. aut Santangelo, A. aut Santiago Crúz, L. aut Sanz Palomino, M. aut Saprykin, O. aut Sarazin, F. aut Sato, H. aut Sato, M. aut Schanz, T. aut Schieler, H. aut Scotti, V. aut Segreto, A. aut Selmane, S. aut Semikoz, D. aut Serra, M. aut Sharakin, S. aut Shibata, T. aut Shimizu, H. M. aut Shinozaki, K. aut Shirahama, T. aut Siemieniec-Oziȩbło, G. aut Silva López, H. H. aut Sledd, J. aut Słomińska, K. aut Sobey, A. aut Sugiyama, T. aut Supanitsky, D. aut Suzuki, M. aut Szabelska, B. aut Szabelski, J. aut Tajima, F. aut Tajima, N. aut Tajima, T. aut Takahashi, Y. aut Takami, H. aut Takeda, M. aut Takizawa, Y. aut Tenzer, C. aut Tibolla, O. aut Tkachev, L. aut Tokuno, H. aut Tomida, T. aut Tone, N. aut Toscano, S. aut Trillaud, F. aut Tsenov, R. aut Tsunesada, Y. aut Tsuno, K. aut Tymieniecka, T. aut Uchihori, Y. aut Unger, M. aut Vaduvescu, O. aut Valdés-Galicia, J. F. aut Vallania, P. aut Valore, L. aut Vankova, G. aut Vigorito, C. aut Villaseñor, L. aut von Ballmoos, P. aut Wada, S. aut Watanabe, J. aut Watanabe, S. aut Watts, J. aut Weber, M. aut Weiler, T. J. aut Wibig, T. aut Wiencke, L. aut Wille, M. aut Wilms, J. aut Włodarczyk, Z. aut Yamamoto, T. aut Yamamoto, Y. aut Yang, J. aut Yano, H. aut Yashin, I. V. aut Yonetoku, D. aut Yoshida, K. aut Yoshida, S. aut Young, R. aut Zotov, M. Yu. aut Zuccaro Marchi, A. aut Enthalten in Experimental astronomy Springer Netherlands, 1989 40(2014), 1 vom: 23. Juli, Seite 45-60 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:40 year:2014 number:1 day:23 month:07 pages:45-60 https://doi.org/10.1007/s10686-014-9378-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_4012 39.00 VZ AR 40 2014 1 23 07 45-60 |
| allfields_unstemmed |
10.1007/s10686-014-9378-1 doi (DE-627)OLC2042944602 (DE-He213)s10686-014-9378-1-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Adams, J. H. verfasserin aut The atmospheric monitoring system of the JEM-EUSO instrument 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. Ultra high energy cosmic rays Atmospheric monitoring IR camera LIDAR Ahmad, S. aut Albert, J. -N. aut Allard, D. aut Anchordoqui, L. aut Andreev, V. aut Anzalone, A. aut Arai, Y. aut Asano, K. aut Ave Pernas, M. aut Baragatti, P. aut Barrillon, P. aut Batsch, T. aut Bayer, J. aut Bechini, R. aut Belenguer, T. aut Bellotti, R. aut Belov, K. aut Berlind, A. A. aut Bertaina, M. aut Biermann, P. L. aut Biktemerova, S. aut Blaksley, C. aut Blanc, N. aut Błȩcki, J. aut Blin-Bondil, S. aut Blümer, J. aut Bobik, P. aut Bogomilov, M. aut Bonamente, M. aut Briggs, M. S. aut Briz, S. aut Bruno, A. aut Cafagna, F. aut Campana, D. aut Capdevielle, J. -N. aut Caruso, R. aut Casolino, M. aut Cassardo, C. aut Castellinic, G. aut Catalano, C. aut Catalano, G. aut Cellino, A. aut Chikawa, M. aut Christl, M. J. aut Cline, D. aut Connaughton, V. aut Conti, L. aut Cordero, G. aut Crawford, H. J. aut Cremonini, R. aut Csorna, S. aut Dagoret-Campagne, S. aut de Castro, A. J. aut De Donato, C. aut de la Taille, C. aut De Santis, C. aut del Peral, L. aut Dell’Oro, A. aut De Simone, N. aut Di Martino, M. aut Distratis, G. aut Dulucq, F. aut Dupieux, M. aut Ebersoldt, A. aut Ebisuzaki, T. aut Engel, R. aut Falk, S. aut Fang, K. aut Fenu, F. aut Fernández-Gómez, I. aut Ferrarese, S. aut Finco, D. aut Flamini, M. aut Fornaro, C. aut Franceschi, A. aut Fujimoto, J. aut Fukushima, M. aut Galeotti, P. aut Garipov, G. aut Geary, J. aut Gelmini, G. aut Giraudo, G. aut Gonchar, M. aut González Alvarado, C. aut Gorodetzky, P. aut Guarino, F. aut Guzmán, A. aut Hachisu, Y. aut Harlov, B. aut Haungs, A. aut Hernández Carretero, J. aut Higashide, K. aut Ikeda, D. aut Ikeda, H. aut Inoue, N. aut Inoue, S. aut Insolia, A. aut Isgrò, F. aut Itow, Y. aut Joven, E. aut Judd, E. G. aut Jung, A. aut Kajino, F. aut Kajino, T. aut Kaneko, I. aut Karadzhov, Y. aut Karczmarczyk, J. aut Karus, M. aut Katahira, K. aut Kawai, K. aut Kawasaki, Y. aut Keilhauer, B. aut Khrenov, B. A. aut Kim, J. -S. aut Kim, S. -W. aut Kim, S. -W. aut Kleifges, M. aut Klimov, P. A. aut Kolev, D. aut Kreykenbohm, I. aut Kudela, K. aut Kurihara, Y. aut Kusenko, A. aut Kuznetsov, E. aut Lacombe, M. aut Lachaud, C. aut Lee, J. aut Licandro, J. aut Lim, H. aut López, F. aut Maccarone, M. C. aut Mannheim, K. aut Maravilla, D. aut Marcelli, L. aut Marini, A. aut Martinez, O. aut Masciantonio, G. aut Mase, K. aut Matev, R. aut Medina-Tanco, G. aut Mernik, T. aut Miyamoto, H. aut Miyazaki, Y. aut Mizumoto, Y. aut Modestino, G. aut Monaco, A. aut Monnier-Ragaigne, D. aut Morales de los Ríos, J. A. aut Moretto, C. aut Morozenko, V. S. aut Mot, B. aut Murakami, T. aut Murakami, M. Nagano aut Nagata, M. aut Nagataki, S. aut Nakamura, T. aut Napolitano, T. aut Naumov, D. aut Nava, R. aut Neronov, A. aut Nomoto, K. aut Nonaka, T. aut Ogawa, T. aut Ogio, S. aut Ohmori, H. aut Olinto, A. V. aut Orleański, P. aut Osteria, G. aut Panasyuk, M. I. aut Parizot, E. aut Park, I. H. aut Park, H. W. aut Pastircak, B. aut Patzak, T. aut Paul, T. aut Pennypacker, C. aut Perez Cano, S. aut Peter, T. aut Picozza, P. aut Pierog, T. aut Piotrowski, L. W. aut Piraino, S. aut Plebaniak, Z. aut Pollini, A. aut Prat, P. aut Prévôt, G. aut Prieto, H. aut Putis, M. aut Reardon, P. aut Reyes, M. aut Ricci, M. aut Rodríguez, I. aut Rodríguez Frías, M. D. aut Ronga, F. aut Roth, M. aut Rothkaehl, H. aut Roudil, G. aut Rusinov, I. aut Rybczyński, M. aut Sabau, M. D. aut Sáez-Cano, G. aut Sagawa, H. aut Saito, A. aut Sakaki, N. aut Sakata, M. aut Salazar, H. aut Sánchez, S. aut Santangelo, A. aut Santiago Crúz, L. aut Sanz Palomino, M. aut Saprykin, O. aut Sarazin, F. aut Sato, H. aut Sato, M. aut Schanz, T. aut Schieler, H. aut Scotti, V. aut Segreto, A. aut Selmane, S. aut Semikoz, D. aut Serra, M. aut Sharakin, S. aut Shibata, T. aut Shimizu, H. M. aut Shinozaki, K. aut Shirahama, T. aut Siemieniec-Oziȩbło, G. aut Silva López, H. H. aut Sledd, J. aut Słomińska, K. aut Sobey, A. aut Sugiyama, T. aut Supanitsky, D. aut Suzuki, M. aut Szabelska, B. aut Szabelski, J. aut Tajima, F. aut Tajima, N. aut Tajima, T. aut Takahashi, Y. aut Takami, H. aut Takeda, M. aut Takizawa, Y. aut Tenzer, C. aut Tibolla, O. aut Tkachev, L. aut Tokuno, H. aut Tomida, T. aut Tone, N. aut Toscano, S. aut Trillaud, F. aut Tsenov, R. aut Tsunesada, Y. aut Tsuno, K. aut Tymieniecka, T. aut Uchihori, Y. aut Unger, M. aut Vaduvescu, O. aut Valdés-Galicia, J. F. aut Vallania, P. aut Valore, L. aut Vankova, G. aut Vigorito, C. aut Villaseñor, L. aut von Ballmoos, P. aut Wada, S. aut Watanabe, J. aut Watanabe, S. aut Watts, J. aut Weber, M. aut Weiler, T. J. aut Wibig, T. aut Wiencke, L. aut Wille, M. aut Wilms, J. aut Włodarczyk, Z. aut Yamamoto, T. aut Yamamoto, Y. aut Yang, J. aut Yano, H. aut Yashin, I. V. aut Yonetoku, D. aut Yoshida, K. aut Yoshida, S. aut Young, R. aut Zotov, M. Yu. aut Zuccaro Marchi, A. aut Enthalten in Experimental astronomy Springer Netherlands, 1989 40(2014), 1 vom: 23. Juli, Seite 45-60 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:40 year:2014 number:1 day:23 month:07 pages:45-60 https://doi.org/10.1007/s10686-014-9378-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_4012 39.00 VZ AR 40 2014 1 23 07 45-60 |
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10.1007/s10686-014-9378-1 doi (DE-627)OLC2042944602 (DE-He213)s10686-014-9378-1-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Adams, J. H. verfasserin aut The atmospheric monitoring system of the JEM-EUSO instrument 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. Ultra high energy cosmic rays Atmospheric monitoring IR camera LIDAR Ahmad, S. aut Albert, J. -N. aut Allard, D. aut Anchordoqui, L. aut Andreev, V. aut Anzalone, A. aut Arai, Y. aut Asano, K. aut Ave Pernas, M. aut Baragatti, P. aut Barrillon, P. aut Batsch, T. aut Bayer, J. aut Bechini, R. aut Belenguer, T. aut Bellotti, R. aut Belov, K. aut Berlind, A. A. aut Bertaina, M. aut Biermann, P. L. aut Biktemerova, S. aut Blaksley, C. aut Blanc, N. aut Błȩcki, J. aut Blin-Bondil, S. aut Blümer, J. aut Bobik, P. aut Bogomilov, M. aut Bonamente, M. aut Briggs, M. S. aut Briz, S. aut Bruno, A. aut Cafagna, F. aut Campana, D. aut Capdevielle, J. -N. aut Caruso, R. aut Casolino, M. aut Cassardo, C. aut Castellinic, G. aut Catalano, C. aut Catalano, G. aut Cellino, A. aut Chikawa, M. aut Christl, M. J. aut Cline, D. aut Connaughton, V. aut Conti, L. aut Cordero, G. aut Crawford, H. J. aut Cremonini, R. aut Csorna, S. aut Dagoret-Campagne, S. aut de Castro, A. J. aut De Donato, C. aut de la Taille, C. aut De Santis, C. aut del Peral, L. aut Dell’Oro, A. aut De Simone, N. aut Di Martino, M. aut Distratis, G. aut Dulucq, F. aut Dupieux, M. aut Ebersoldt, A. aut Ebisuzaki, T. aut Engel, R. aut Falk, S. aut Fang, K. aut Fenu, F. aut Fernández-Gómez, I. aut Ferrarese, S. aut Finco, D. aut Flamini, M. aut Fornaro, C. aut Franceschi, A. aut Fujimoto, J. aut Fukushima, M. aut Galeotti, P. aut Garipov, G. aut Geary, J. aut Gelmini, G. aut Giraudo, G. aut Gonchar, M. aut González Alvarado, C. aut Gorodetzky, P. aut Guarino, F. aut Guzmán, A. aut Hachisu, Y. aut Harlov, B. aut Haungs, A. aut Hernández Carretero, J. aut Higashide, K. aut Ikeda, D. aut Ikeda, H. aut Inoue, N. aut Inoue, S. aut Insolia, A. aut Isgrò, F. aut Itow, Y. aut Joven, E. aut Judd, E. G. aut Jung, A. aut Kajino, F. aut Kajino, T. aut Kaneko, I. aut Karadzhov, Y. aut Karczmarczyk, J. aut Karus, M. aut Katahira, K. aut Kawai, K. aut Kawasaki, Y. aut Keilhauer, B. aut Khrenov, B. A. aut Kim, J. -S. aut Kim, S. -W. aut Kim, S. -W. aut Kleifges, M. aut Klimov, P. A. aut Kolev, D. aut Kreykenbohm, I. aut Kudela, K. aut Kurihara, Y. aut Kusenko, A. aut Kuznetsov, E. aut Lacombe, M. aut Lachaud, C. aut Lee, J. aut Licandro, J. aut Lim, H. aut López, F. aut Maccarone, M. C. aut Mannheim, K. aut Maravilla, D. aut Marcelli, L. aut Marini, A. aut Martinez, O. aut Masciantonio, G. aut Mase, K. aut Matev, R. aut Medina-Tanco, G. aut Mernik, T. aut Miyamoto, H. aut Miyazaki, Y. aut Mizumoto, Y. aut Modestino, G. aut Monaco, A. aut Monnier-Ragaigne, D. aut Morales de los Ríos, J. A. aut Moretto, C. aut Morozenko, V. S. aut Mot, B. aut Murakami, T. aut Murakami, M. Nagano aut Nagata, M. aut Nagataki, S. aut Nakamura, T. aut Napolitano, T. aut Naumov, D. aut Nava, R. aut Neronov, A. aut Nomoto, K. aut Nonaka, T. aut Ogawa, T. aut Ogio, S. aut Ohmori, H. aut Olinto, A. V. aut Orleański, P. aut Osteria, G. aut Panasyuk, M. I. aut Parizot, E. aut Park, I. H. aut Park, H. W. aut Pastircak, B. aut Patzak, T. aut Paul, T. aut Pennypacker, C. aut Perez Cano, S. aut Peter, T. aut Picozza, P. aut Pierog, T. aut Piotrowski, L. W. aut Piraino, S. aut Plebaniak, Z. aut Pollini, A. aut Prat, P. aut Prévôt, G. aut Prieto, H. aut Putis, M. aut Reardon, P. aut Reyes, M. aut Ricci, M. aut Rodríguez, I. aut Rodríguez Frías, M. D. aut Ronga, F. aut Roth, M. aut Rothkaehl, H. aut Roudil, G. aut Rusinov, I. aut Rybczyński, M. aut Sabau, M. D. aut Sáez-Cano, G. aut Sagawa, H. aut Saito, A. aut Sakaki, N. aut Sakata, M. aut Salazar, H. aut Sánchez, S. aut Santangelo, A. aut Santiago Crúz, L. aut Sanz Palomino, M. aut Saprykin, O. aut Sarazin, F. aut Sato, H. aut Sato, M. aut Schanz, T. aut Schieler, H. aut Scotti, V. aut Segreto, A. aut Selmane, S. aut Semikoz, D. aut Serra, M. aut Sharakin, S. aut Shibata, T. aut Shimizu, H. M. aut Shinozaki, K. aut Shirahama, T. aut Siemieniec-Oziȩbło, G. aut Silva López, H. H. aut Sledd, J. aut Słomińska, K. aut Sobey, A. aut Sugiyama, T. aut Supanitsky, D. aut Suzuki, M. aut Szabelska, B. aut Szabelski, J. aut Tajima, F. aut Tajima, N. aut Tajima, T. aut Takahashi, Y. aut Takami, H. aut Takeda, M. aut Takizawa, Y. aut Tenzer, C. aut Tibolla, O. aut Tkachev, L. aut Tokuno, H. aut Tomida, T. aut Tone, N. aut Toscano, S. aut Trillaud, F. aut Tsenov, R. aut Tsunesada, Y. aut Tsuno, K. aut Tymieniecka, T. aut Uchihori, Y. aut Unger, M. aut Vaduvescu, O. aut Valdés-Galicia, J. F. aut Vallania, P. aut Valore, L. aut Vankova, G. aut Vigorito, C. aut Villaseñor, L. aut von Ballmoos, P. aut Wada, S. aut Watanabe, J. aut Watanabe, S. aut Watts, J. aut Weber, M. aut Weiler, T. J. aut Wibig, T. aut Wiencke, L. aut Wille, M. aut Wilms, J. aut Włodarczyk, Z. aut Yamamoto, T. aut Yamamoto, Y. aut Yang, J. aut Yano, H. aut Yashin, I. V. aut Yonetoku, D. aut Yoshida, K. aut Yoshida, S. aut Young, R. aut Zotov, M. Yu. aut Zuccaro Marchi, A. aut Enthalten in Experimental astronomy Springer Netherlands, 1989 40(2014), 1 vom: 23. Juli, Seite 45-60 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:40 year:2014 number:1 day:23 month:07 pages:45-60 https://doi.org/10.1007/s10686-014-9378-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_4012 39.00 VZ AR 40 2014 1 23 07 45-60 |
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10.1007/s10686-014-9378-1 doi (DE-627)OLC2042944602 (DE-He213)s10686-014-9378-1-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Adams, J. H. verfasserin aut The atmospheric monitoring system of the JEM-EUSO instrument 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2014 Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. Ultra high energy cosmic rays Atmospheric monitoring IR camera LIDAR Ahmad, S. aut Albert, J. -N. aut Allard, D. aut Anchordoqui, L. aut Andreev, V. aut Anzalone, A. aut Arai, Y. aut Asano, K. aut Ave Pernas, M. aut Baragatti, P. aut Barrillon, P. aut Batsch, T. aut Bayer, J. aut Bechini, R. aut Belenguer, T. aut Bellotti, R. aut Belov, K. aut Berlind, A. A. aut Bertaina, M. aut Biermann, P. L. aut Biktemerova, S. aut Blaksley, C. aut Blanc, N. aut Błȩcki, J. aut Blin-Bondil, S. aut Blümer, J. aut Bobik, P. aut Bogomilov, M. aut Bonamente, M. aut Briggs, M. S. aut Briz, S. aut Bruno, A. aut Cafagna, F. aut Campana, D. aut Capdevielle, J. -N. aut Caruso, R. aut Casolino, M. aut Cassardo, C. aut Castellinic, G. aut Catalano, C. aut Catalano, G. aut Cellino, A. aut Chikawa, M. aut Christl, M. J. aut Cline, D. aut Connaughton, V. aut Conti, L. aut Cordero, G. aut Crawford, H. J. aut Cremonini, R. aut Csorna, S. aut Dagoret-Campagne, S. aut de Castro, A. J. aut De Donato, C. aut de la Taille, C. aut De Santis, C. aut del Peral, L. aut Dell’Oro, A. aut De Simone, N. aut Di Martino, M. aut Distratis, G. aut Dulucq, F. aut Dupieux, M. aut Ebersoldt, A. aut Ebisuzaki, T. aut Engel, R. aut Falk, S. aut Fang, K. aut Fenu, F. aut Fernández-Gómez, I. aut Ferrarese, S. aut Finco, D. aut Flamini, M. aut Fornaro, C. aut Franceschi, A. aut Fujimoto, J. aut Fukushima, M. aut Galeotti, P. aut Garipov, G. aut Geary, J. aut Gelmini, G. aut Giraudo, G. aut Gonchar, M. aut González Alvarado, C. aut Gorodetzky, P. aut Guarino, F. aut Guzmán, A. aut Hachisu, Y. aut Harlov, B. aut Haungs, A. aut Hernández Carretero, J. aut Higashide, K. aut Ikeda, D. aut Ikeda, H. aut Inoue, N. aut Inoue, S. aut Insolia, A. aut Isgrò, F. aut Itow, Y. aut Joven, E. aut Judd, E. G. aut Jung, A. aut Kajino, F. aut Kajino, T. aut Kaneko, I. aut Karadzhov, Y. aut Karczmarczyk, J. aut Karus, M. aut Katahira, K. aut Kawai, K. aut Kawasaki, Y. aut Keilhauer, B. aut Khrenov, B. A. aut Kim, J. -S. aut Kim, S. -W. aut Kim, S. -W. aut Kleifges, M. aut Klimov, P. A. aut Kolev, D. aut Kreykenbohm, I. aut Kudela, K. aut Kurihara, Y. aut Kusenko, A. aut Kuznetsov, E. aut Lacombe, M. aut Lachaud, C. aut Lee, J. aut Licandro, J. aut Lim, H. aut López, F. aut Maccarone, M. C. aut Mannheim, K. aut Maravilla, D. aut Marcelli, L. aut Marini, A. aut Martinez, O. aut Masciantonio, G. aut Mase, K. aut Matev, R. aut Medina-Tanco, G. aut Mernik, T. aut Miyamoto, H. aut Miyazaki, Y. aut Mizumoto, Y. aut Modestino, G. aut Monaco, A. aut Monnier-Ragaigne, D. aut Morales de los Ríos, J. A. aut Moretto, C. aut Morozenko, V. S. aut Mot, B. aut Murakami, T. aut Murakami, M. Nagano aut Nagata, M. aut Nagataki, S. aut Nakamura, T. aut Napolitano, T. aut Naumov, D. aut Nava, R. aut Neronov, A. aut Nomoto, K. aut Nonaka, T. aut Ogawa, T. aut Ogio, S. aut Ohmori, H. aut Olinto, A. V. aut Orleański, P. aut Osteria, G. aut Panasyuk, M. I. aut Parizot, E. aut Park, I. H. aut Park, H. W. aut Pastircak, B. aut Patzak, T. aut Paul, T. aut Pennypacker, C. aut Perez Cano, S. aut Peter, T. aut Picozza, P. aut Pierog, T. aut Piotrowski, L. W. aut Piraino, S. aut Plebaniak, Z. aut Pollini, A. aut Prat, P. aut Prévôt, G. aut Prieto, H. aut Putis, M. aut Reardon, P. aut Reyes, M. aut Ricci, M. aut Rodríguez, I. aut Rodríguez Frías, M. D. aut Ronga, F. aut Roth, M. aut Rothkaehl, H. aut Roudil, G. aut Rusinov, I. aut Rybczyński, M. aut Sabau, M. D. aut Sáez-Cano, G. aut Sagawa, H. aut Saito, A. aut Sakaki, N. aut Sakata, M. aut Salazar, H. aut Sánchez, S. aut Santangelo, A. aut Santiago Crúz, L. aut Sanz Palomino, M. aut Saprykin, O. aut Sarazin, F. aut Sato, H. aut Sato, M. aut Schanz, T. aut Schieler, H. aut Scotti, V. aut Segreto, A. aut Selmane, S. aut Semikoz, D. aut Serra, M. aut Sharakin, S. aut Shibata, T. aut Shimizu, H. M. aut Shinozaki, K. aut Shirahama, T. aut Siemieniec-Oziȩbło, G. aut Silva López, H. H. aut Sledd, J. aut Słomińska, K. aut Sobey, A. aut Sugiyama, T. aut Supanitsky, D. aut Suzuki, M. aut Szabelska, B. aut Szabelski, J. aut Tajima, F. aut Tajima, N. aut Tajima, T. aut Takahashi, Y. aut Takami, H. aut Takeda, M. aut Takizawa, Y. aut Tenzer, C. aut Tibolla, O. aut Tkachev, L. aut Tokuno, H. aut Tomida, T. aut Tone, N. aut Toscano, S. aut Trillaud, F. aut Tsenov, R. aut Tsunesada, Y. aut Tsuno, K. aut Tymieniecka, T. aut Uchihori, Y. aut Unger, M. aut Vaduvescu, O. aut Valdés-Galicia, J. F. aut Vallania, P. aut Valore, L. aut Vankova, G. aut Vigorito, C. aut Villaseñor, L. aut von Ballmoos, P. aut Wada, S. aut Watanabe, J. aut Watanabe, S. aut Watts, J. aut Weber, M. aut Weiler, T. J. aut Wibig, T. aut Wiencke, L. aut Wille, M. aut Wilms, J. aut Włodarczyk, Z. aut Yamamoto, T. aut Yamamoto, Y. aut Yang, J. aut Yano, H. aut Yashin, I. V. aut Yonetoku, D. aut Yoshida, K. aut Yoshida, S. aut Young, R. aut Zotov, M. Yu. aut Zuccaro Marchi, A. aut Enthalten in Experimental astronomy Springer Netherlands, 1989 40(2014), 1 vom: 23. Juli, Seite 45-60 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:40 year:2014 number:1 day:23 month:07 pages:45-60 https://doi.org/10.1007/s10686-014-9378-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_4012 39.00 VZ AR 40 2014 1 23 07 45-60 |
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Adams, J. H. @@aut@@ Ahmad, S. @@aut@@ Albert, J. -N. @@aut@@ Allard, D. @@aut@@ Anchordoqui, L. @@aut@@ Andreev, V. @@aut@@ Anzalone, A. @@aut@@ Arai, Y. @@aut@@ Asano, K. @@aut@@ Ave Pernas, M. @@aut@@ Baragatti, P. @@aut@@ Barrillon, P. @@aut@@ Batsch, T. @@aut@@ Bayer, J. @@aut@@ Bechini, R. @@aut@@ Belenguer, T. @@aut@@ Bellotti, R. @@aut@@ Belov, K. @@aut@@ Berlind, A. A. @@aut@@ Bertaina, M. @@aut@@ Biermann, P. L. @@aut@@ Biktemerova, S. @@aut@@ Blaksley, C. @@aut@@ Blanc, N. @@aut@@ Błȩcki, J. @@aut@@ Blin-Bondil, S. @@aut@@ Blümer, J. @@aut@@ Bobik, P. @@aut@@ Bogomilov, M. @@aut@@ Bonamente, M. @@aut@@ Briggs, M. S. @@aut@@ Briz, S. @@aut@@ Bruno, A. @@aut@@ Cafagna, F. @@aut@@ Campana, D. @@aut@@ Capdevielle, J. -N. @@aut@@ Caruso, R. @@aut@@ Casolino, M. @@aut@@ Cassardo, C. @@aut@@ Castellinic, G. @@aut@@ Catalano, C. @@aut@@ Catalano, G. @@aut@@ Cellino, A. @@aut@@ Chikawa, M. @@aut@@ Christl, M. J. @@aut@@ Cline, D. @@aut@@ Connaughton, V. @@aut@@ Conti, L. @@aut@@ Cordero, G. @@aut@@ Crawford, H. J. @@aut@@ Cremonini, R. @@aut@@ Csorna, S. @@aut@@ Dagoret-Campagne, S. @@aut@@ de Castro, A. J. @@aut@@ De Donato, C. @@aut@@ de la Taille, C. @@aut@@ De Santis, C. @@aut@@ del Peral, L. @@aut@@ Dell’Oro, A. @@aut@@ De Simone, N. @@aut@@ Di Martino, M. @@aut@@ Distratis, G. @@aut@@ Dulucq, F. @@aut@@ Dupieux, M. @@aut@@ Ebersoldt, A. @@aut@@ Ebisuzaki, T. @@aut@@ Engel, R. @@aut@@ Falk, S. @@aut@@ Fang, K. @@aut@@ Fenu, F. @@aut@@ Fernández-Gómez, I. @@aut@@ Ferrarese, S. @@aut@@ Finco, D. @@aut@@ Flamini, M. @@aut@@ Fornaro, C. @@aut@@ Franceschi, A. @@aut@@ Fujimoto, J. @@aut@@ Fukushima, M. @@aut@@ Galeotti, P. @@aut@@ Garipov, G. @@aut@@ Geary, J. @@aut@@ Gelmini, G. @@aut@@ Giraudo, G. @@aut@@ Gonchar, M. @@aut@@ González Alvarado, C. @@aut@@ Gorodetzky, P. @@aut@@ Guarino, F. @@aut@@ Guzmán, A. @@aut@@ Hachisu, Y. @@aut@@ Harlov, B. @@aut@@ Haungs, A. @@aut@@ Hernández Carretero, J. @@aut@@ Higashide, K. @@aut@@ Ikeda, D. @@aut@@ Ikeda, H. @@aut@@ Inoue, N. @@aut@@ Inoue, S. @@aut@@ Insolia, A. @@aut@@ Isgrò, F. @@aut@@ Itow, Y. @@aut@@ Joven, E. @@aut@@ Judd, E. G. @@aut@@ Jung, A. @@aut@@ Kajino, F. @@aut@@ Kajino, T. @@aut@@ Kaneko, I. @@aut@@ Karadzhov, Y. @@aut@@ Karczmarczyk, J. @@aut@@ Karus, M. @@aut@@ Katahira, K. @@aut@@ Kawai, K. @@aut@@ Kawasaki, Y. @@aut@@ Keilhauer, B. @@aut@@ Khrenov, B. A. @@aut@@ Kim, J. -S. @@aut@@ Kim, S. -W. @@aut@@ Kleifges, M. @@aut@@ Klimov, P. A. @@aut@@ Kolev, D. @@aut@@ Kreykenbohm, I. @@aut@@ Kudela, K. @@aut@@ Kurihara, Y. @@aut@@ Kusenko, A. @@aut@@ Kuznetsov, E. @@aut@@ Lacombe, M. @@aut@@ Lachaud, C. @@aut@@ Lee, J. @@aut@@ Licandro, J. @@aut@@ Lim, H. @@aut@@ López, F. @@aut@@ Maccarone, M. C. @@aut@@ Mannheim, K. @@aut@@ Maravilla, D. @@aut@@ Marcelli, L. @@aut@@ Marini, A. @@aut@@ Martinez, O. @@aut@@ Masciantonio, G. @@aut@@ Mase, K. @@aut@@ Matev, R. @@aut@@ Medina-Tanco, G. @@aut@@ Mernik, T. @@aut@@ Miyamoto, H. @@aut@@ Miyazaki, Y. @@aut@@ Mizumoto, Y. @@aut@@ Modestino, G. @@aut@@ Monaco, A. @@aut@@ Monnier-Ragaigne, D. @@aut@@ Morales de los Ríos, J. A. @@aut@@ Moretto, C. @@aut@@ Morozenko, V. S. @@aut@@ Mot, B. @@aut@@ Murakami, T. @@aut@@ Murakami, M. Nagano @@aut@@ Nagata, M. @@aut@@ Nagataki, S. @@aut@@ Nakamura, T. @@aut@@ Napolitano, T. @@aut@@ Naumov, D. @@aut@@ Nava, R. @@aut@@ Neronov, A. @@aut@@ Nomoto, K. @@aut@@ Nonaka, T. @@aut@@ Ogawa, T. @@aut@@ Ogio, S. @@aut@@ Ohmori, H. @@aut@@ Olinto, A. V. @@aut@@ Orleański, P. @@aut@@ Osteria, G. @@aut@@ Panasyuk, M. I. @@aut@@ Parizot, E. @@aut@@ Park, I. H. @@aut@@ Park, H. W. @@aut@@ Pastircak, B. @@aut@@ Patzak, T. @@aut@@ Paul, T. @@aut@@ Pennypacker, C. @@aut@@ Perez Cano, S. @@aut@@ Peter, T. @@aut@@ Picozza, P. @@aut@@ Pierog, T. @@aut@@ Piotrowski, L. W. @@aut@@ Piraino, S. @@aut@@ Plebaniak, Z. @@aut@@ Pollini, A. @@aut@@ Prat, P. @@aut@@ Prévôt, G. @@aut@@ Prieto, H. @@aut@@ Putis, M. @@aut@@ Reardon, P. @@aut@@ Reyes, M. @@aut@@ Ricci, M. @@aut@@ Rodríguez, I. @@aut@@ Rodríguez Frías, M. D. @@aut@@ Ronga, F. @@aut@@ Roth, M. @@aut@@ Rothkaehl, H. @@aut@@ Roudil, G. @@aut@@ Rusinov, I. @@aut@@ Rybczyński, M. @@aut@@ Sabau, M. D. @@aut@@ Sáez-Cano, G. @@aut@@ Sagawa, H. @@aut@@ Saito, A. @@aut@@ Sakaki, N. @@aut@@ Sakata, M. @@aut@@ Salazar, H. @@aut@@ Sánchez, S. @@aut@@ Santangelo, A. @@aut@@ Santiago Crúz, L. @@aut@@ Sanz Palomino, M. @@aut@@ Saprykin, O. @@aut@@ Sarazin, F. @@aut@@ Sato, H. @@aut@@ Sato, M. @@aut@@ Schanz, T. @@aut@@ Schieler, H. @@aut@@ Scotti, V. @@aut@@ Segreto, A. @@aut@@ Selmane, S. @@aut@@ Semikoz, D. @@aut@@ Serra, M. @@aut@@ Sharakin, S. @@aut@@ Shibata, T. @@aut@@ Shimizu, H. M. @@aut@@ Shinozaki, K. @@aut@@ Shirahama, T. @@aut@@ Siemieniec-Oziȩbło, G. @@aut@@ Silva López, H. H. @@aut@@ Sledd, J. @@aut@@ Słomińska, K. @@aut@@ Sobey, A. @@aut@@ Sugiyama, T. @@aut@@ Supanitsky, D. @@aut@@ Suzuki, M. @@aut@@ Szabelska, B. @@aut@@ Szabelski, J. @@aut@@ Tajima, F. @@aut@@ Tajima, N. @@aut@@ Tajima, T. @@aut@@ Takahashi, Y. @@aut@@ Takami, H. @@aut@@ Takeda, M. @@aut@@ Takizawa, Y. @@aut@@ Tenzer, C. @@aut@@ Tibolla, O. @@aut@@ Tkachev, L. @@aut@@ Tokuno, H. @@aut@@ Tomida, T. @@aut@@ Tone, N. @@aut@@ Toscano, S. @@aut@@ Trillaud, F. @@aut@@ Tsenov, R. @@aut@@ Tsunesada, Y. @@aut@@ Tsuno, K. @@aut@@ Tymieniecka, T. @@aut@@ Uchihori, Y. @@aut@@ Unger, M. @@aut@@ Vaduvescu, O. @@aut@@ Valdés-Galicia, J. F. @@aut@@ Vallania, P. @@aut@@ Valore, L. @@aut@@ Vankova, G. @@aut@@ Vigorito, C. @@aut@@ Villaseñor, L. @@aut@@ von Ballmoos, P. @@aut@@ Wada, S. @@aut@@ Watanabe, J. @@aut@@ Watanabe, S. @@aut@@ Watts, J. @@aut@@ Weber, M. @@aut@@ Weiler, T. J. @@aut@@ Wibig, T. @@aut@@ Wiencke, L. @@aut@@ Wille, M. @@aut@@ Wilms, J. @@aut@@ Włodarczyk, Z. @@aut@@ Yamamoto, T. @@aut@@ Yamamoto, Y. @@aut@@ Yang, J. @@aut@@ Yano, H. @@aut@@ Yashin, I. V. @@aut@@ Yonetoku, D. @@aut@@ Yoshida, K. @@aut@@ Yoshida, S. @@aut@@ Young, R. @@aut@@ Zotov, M. Yu. @@aut@@ Zuccaro Marchi, A. @@aut@@ |
| publishDateDaySort_date |
2014-07-23T00:00:00Z |
| hierarchy_top_id |
130767123 |
| dewey-sort |
3520 |
| id |
OLC2042944602 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2042944602</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230503055233.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2014 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10686-014-9378-1</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2042944602</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10686-014-9378-1-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Adams, J. H.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The atmospheric monitoring system of the JEM-EUSO instrument</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media Dordrecht 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Ultra high energy cosmic rays</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Atmospheric monitoring</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">IR camera</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">LIDAR</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ahmad, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Albert, J. -N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Allard, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anchordoqui, L.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Andreev, V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anzalone, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Arai, Y.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Asano, K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ave Pernas, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Baragatti, P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Barrillon, P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Batsch, T.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bayer, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bechini, R.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Belenguer, T.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bellotti, R.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Belov, K.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Berlind, A. 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Adams, J. H. Ahmad, S. Albert, J. -N. Allard, D. Anchordoqui, L. Andreev, V. Anzalone, A. Arai, Y. Asano, K. Ave Pernas, M. Baragatti, P. Barrillon, P. Batsch, T. Bayer, J. Bechini, R. Belenguer, T. Bellotti, R. Belov, K. Berlind, A. A. Bertaina, M. Biermann, P. L. Biktemerova, S. Blaksley, C. Blanc, N. Błȩcki, J. Blin-Bondil, S. Blümer, J. Bobik, P. Bogomilov, M. Bonamente, M. Briggs, M. S. Briz, S. Bruno, A. Cafagna, F. Campana, D. Capdevielle, J. -N. Caruso, R. Casolino, M. Cassardo, C. Castellinic, G. Catalano, C. Catalano, G. Cellino, A. Chikawa, M. Christl, M. J. Cline, D. Connaughton, V. Conti, L. Cordero, G. Crawford, H. J. Cremonini, R. Csorna, S. Dagoret-Campagne, S. de Castro, A. J. De Donato, C. de la Taille, C. De Santis, C. del Peral, L. Dell’Oro, A. De Simone, N. Di Martino, M. Distratis, G. Dulucq, F. Dupieux, M. Ebersoldt, A. Ebisuzaki, T. Engel, R. Falk, S. Fang, K. Fenu, F. Fernández-Gómez, I. Ferrarese, S. Finco, D. Flamini, M. Fornaro, C. Franceschi, A. Fujimoto, J. Fukushima, M. Galeotti, P. Garipov, G. Geary, J. Gelmini, G. Giraudo, G. Gonchar, M. González Alvarado, C. Gorodetzky, P. Guarino, F. Guzmán, A. Hachisu, Y. Harlov, B. Haungs, A. Hernández Carretero, J. Higashide, K. Ikeda, D. Ikeda, H. Inoue, N. Inoue, S. Insolia, A. Isgrò, F. Itow, Y. Joven, E. Judd, E. G. Jung, A. Kajino, F. Kajino, T. Kaneko, I. Karadzhov, Y. Karczmarczyk, J. Karus, M. Katahira, K. Kawai, K. Kawasaki, Y. Keilhauer, B. Khrenov, B. A. Kim, J. -S. Kim, S. -W. Kleifges, M. Klimov, P. A. Kolev, D. Kreykenbohm, I. Kudela, K. Kurihara, Y. Kusenko, A. Kuznetsov, E. Lacombe, M. Lachaud, C. Lee, J. Licandro, J. Lim, H. López, F. Maccarone, M. C. Mannheim, K. Maravilla, D. Marcelli, L. Marini, A. Martinez, O. Masciantonio, G. Mase, K. Matev, R. Medina-Tanco, G. Mernik, T. Miyamoto, H. Miyazaki, Y. Mizumoto, Y. Modestino, G. Monaco, A. Monnier-Ragaigne, D. Morales de los Ríos, J. A. Moretto, C. Morozenko, V. S. Mot, B. Murakami, T. Murakami, M. Nagano Nagata, M. Nagataki, S. Nakamura, T. Napolitano, T. Naumov, D. Nava, R. Neronov, A. Nomoto, K. Nonaka, T. Ogawa, T. Ogio, S. Ohmori, H. Olinto, A. V. Orleański, P. Osteria, G. Panasyuk, M. I. Parizot, E. Park, I. H. Park, H. W. Pastircak, B. Patzak, T. Paul, T. Pennypacker, C. Perez Cano, S. Peter, T. Picozza, P. Pierog, T. Piotrowski, L. W. Piraino, S. Plebaniak, Z. Pollini, A. Prat, P. Prévôt, G. Prieto, H. Putis, M. Reardon, P. Reyes, M. Ricci, M. Rodríguez, I. Rodríguez Frías, M. D. Ronga, F. Roth, M. Rothkaehl, H. Roudil, G. Rusinov, I. Rybczyński, M. Sabau, M. D. Sáez-Cano, G. Sagawa, H. Saito, A. Sakaki, N. Sakata, M. Salazar, H. Sánchez, S. Santangelo, A. Santiago Crúz, L. Sanz Palomino, M. Saprykin, O. Sarazin, F. Sato, H. Sato, M. Schanz, T. Schieler, H. Scotti, V. Segreto, A. Selmane, S. Semikoz, D. Serra, M. Sharakin, S. Shibata, T. Shimizu, H. M. Shinozaki, K. Shirahama, T. Siemieniec-Oziȩbło, G. Silva López, H. H. Sledd, J. Słomińska, K. Sobey, A. Sugiyama, T. Supanitsky, D. Suzuki, M. Szabelska, B. Szabelski, J. Tajima, F. Tajima, N. Tajima, T. Takahashi, Y. Takami, H. Takeda, M. Takizawa, Y. Tenzer, C. Tibolla, O. Tkachev, L. Tokuno, H. Tomida, T. Tone, N. Toscano, S. Trillaud, F. Tsenov, R. Tsunesada, Y. Tsuno, K. Tymieniecka, T. Uchihori, Y. Unger, M. Vaduvescu, O. Valdés-Galicia, J. F. Vallania, P. Valore, L. Vankova, G. Vigorito, C. Villaseñor, L. von Ballmoos, P. Wada, S. Watanabe, J. Watanabe, S. Watts, J. Weber, M. Weiler, T. J. Wibig, T. Wiencke, L. Wille, M. Wilms, J. Włodarczyk, Z. Yamamoto, T. Yamamoto, Y. Yang, J. Yano, H. Yashin, I. V. Yonetoku, D. Yoshida, K. Yoshida, S. Young, R. Zotov, M. Yu. Zuccaro Marchi, A. |
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Adams, J. H. |
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the atmospheric monitoring system of the jem-euso instrument |
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The atmospheric monitoring system of the JEM-EUSO instrument |
| abstract |
Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. © Springer Science+Business Media Dordrecht 2014 |
| abstractGer |
Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. © Springer Science+Business Media Dordrecht 2014 |
| abstract_unstemmed |
Abstract The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m. © Springer Science+Business Media Dordrecht 2014 |
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The atmospheric monitoring system of the JEM-EUSO instrument |
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