Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project
Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detect...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Abbrescia, M. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Berlin : Springer, 2011, 129(2014), 8 vom: 11. Aug. |
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| Übergeordnetes Werk: |
volume:129 ; year:2014 ; number:8 ; day:11 ; month:08 |
| Links: |
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| DOI / URN: |
10.1140/epjp/i2014-14166-3 |
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| Katalog-ID: |
SPR031455433 |
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| 100 | 1 | |a Abbrescia, M. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project |
| 264 | 1 | |c 2014 | |
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| 520 | |a Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. | ||
| 650 | 4 | |a Observation Level |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Coincidence Event |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Primary Proton |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Muon Component |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Shower Core |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Agocs, A. |4 aut | |
| 700 | 1 | |a Aiola, S. |4 aut | |
| 700 | 1 | |a Antolini, R. |4 aut | |
| 700 | 1 | |a Avanzini, C. |4 aut | |
| 700 | 1 | |a Baldini Ferroli, R. |4 aut | |
| 700 | 1 | |a Bencivenni, G. |4 aut | |
| 700 | 1 | |a Bossini, E. |4 aut | |
| 700 | 1 | |a Bressan, E. |4 aut | |
| 700 | 1 | |a Chiavassa, A. |4 aut | |
| 700 | 1 | |a Cicalò, C. |4 aut | |
| 700 | 1 | |a Cifarelli, L. |4 aut | |
| 700 | 1 | |a Coccia, E. |4 aut | |
| 700 | 1 | |a De Gruttola, D. |4 aut | |
| 700 | 1 | |a De Pasquale, S. |4 aut | |
| 700 | 1 | |a Di Giovanni, A. |4 aut | |
| 700 | 1 | |a D’Incecco, M. |4 aut | |
| 700 | 1 | |a Dreucci, M. |4 aut | |
| 700 | 1 | |a Fabbri, F. L. |4 aut | |
| 700 | 1 | |a Frolov, V. |4 aut | |
| 700 | 1 | |a Garbini, M. |4 aut | |
| 700 | 1 | |a Gemme, G. |4 aut | |
| 700 | 1 | |a Gnesi, I. |4 aut | |
| 700 | 1 | |a Gustavino, C. |4 aut | |
| 700 | 1 | |a Hatzifotiadou, D. |4 aut | |
| 700 | 1 | |a La Rocca, P. |4 aut | |
| 700 | 1 | |a Li, S. |4 aut | |
| 700 | 1 | |a Librizzi, F. |4 aut | |
| 700 | 1 | |a Maggiora, A. |4 aut | |
| 700 | 1 | |a Massai, M. |4 aut | |
| 700 | 1 | |a Miozzi, S. |4 aut | |
| 700 | 1 | |a Panareo, M. |4 aut | |
| 700 | 1 | |a Paoletti, R. |4 aut | |
| 700 | 1 | |a Perasso, L. |4 aut | |
| 700 | 1 | |a Pilo, F. |4 aut | |
| 700 | 1 | |a Piragino, G. |4 aut | |
| 700 | 1 | |a Regano, A. |4 aut | |
| 700 | 1 | |a Riggi, F. |4 aut | |
| 700 | 1 | |a Righini, G. C. |4 aut | |
| 700 | 1 | |a Sartorelli, G. |4 aut | |
| 700 | 1 | |a Scapparone, E. |4 aut | |
| 700 | 1 | |a Scribano, A. |4 aut | |
| 700 | 1 | |a Selvi, M. |4 aut | |
| 700 | 1 | |a Serci, S. |4 aut | |
| 700 | 1 | |a Siddi, E. |4 aut | |
| 700 | 1 | |a Spandre, G. |4 aut | |
| 700 | 1 | |a Squarcia, S. |4 aut | |
| 700 | 1 | |a Taiuti, M. |4 aut | |
| 700 | 1 | |a Tosello, F. |4 aut | |
| 700 | 1 | |a Votano, L. |4 aut | |
| 700 | 1 | |a Williams, M. C. S. |4 aut | |
| 700 | 1 | |a Yánez, G. |4 aut | |
| 700 | 1 | |a Zichichi, A. |4 aut | |
| 700 | 1 | |a Zuyeuski, R. |4 aut | |
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10.1140/epjp/i2014-14166-3 doi (DE-627)SPR031455433 (SPR)i2014-14166-3-e DE-627 ger DE-627 rakwb eng Abbrescia, M. verfasserin aut Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. Observation Level (dpeaa)DE-He213 Coincidence Event (dpeaa)DE-He213 Primary Proton (dpeaa)DE-He213 Muon Component (dpeaa)DE-He213 Shower Core (dpeaa)DE-He213 Agocs, A. aut Aiola, S. aut Antolini, R. aut Avanzini, C. aut Baldini Ferroli, R. aut Bencivenni, G. aut Bossini, E. aut Bressan, E. aut Chiavassa, A. aut Cicalò, C. aut Cifarelli, L. aut Coccia, E. aut De Gruttola, D. aut De Pasquale, S. aut Di Giovanni, A. aut D’Incecco, M. aut Dreucci, M. aut Fabbri, F. L. aut Frolov, V. aut Garbini, M. aut Gemme, G. aut Gnesi, I. aut Gustavino, C. aut Hatzifotiadou, D. aut La Rocca, P. aut Li, S. aut Librizzi, F. aut Maggiora, A. aut Massai, M. aut Miozzi, S. aut Panareo, M. aut Paoletti, R. aut Perasso, L. aut Pilo, F. aut Piragino, G. aut Regano, A. aut Riggi, F. aut Righini, G. C. aut Sartorelli, G. aut Scapparone, E. aut Scribano, A. aut Selvi, M. aut Serci, S. aut Siddi, E. aut Spandre, G. aut Squarcia, S. aut Taiuti, M. aut Tosello, F. aut Votano, L. aut Williams, M. C. S. aut Yánez, G. aut Zichichi, A. aut Zuyeuski, R. aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 8 vom: 11. Aug. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:8 day:11 month:08 https://dx.doi.org/10.1140/epjp/i2014-14166-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 129 2014 8 11 08 |
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10.1140/epjp/i2014-14166-3 doi (DE-627)SPR031455433 (SPR)i2014-14166-3-e DE-627 ger DE-627 rakwb eng Abbrescia, M. verfasserin aut Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. Observation Level (dpeaa)DE-He213 Coincidence Event (dpeaa)DE-He213 Primary Proton (dpeaa)DE-He213 Muon Component (dpeaa)DE-He213 Shower Core (dpeaa)DE-He213 Agocs, A. aut Aiola, S. aut Antolini, R. aut Avanzini, C. aut Baldini Ferroli, R. aut Bencivenni, G. aut Bossini, E. aut Bressan, E. aut Chiavassa, A. aut Cicalò, C. aut Cifarelli, L. aut Coccia, E. aut De Gruttola, D. aut De Pasquale, S. aut Di Giovanni, A. aut D’Incecco, M. aut Dreucci, M. aut Fabbri, F. L. aut Frolov, V. aut Garbini, M. aut Gemme, G. aut Gnesi, I. aut Gustavino, C. aut Hatzifotiadou, D. aut La Rocca, P. aut Li, S. aut Librizzi, F. aut Maggiora, A. aut Massai, M. aut Miozzi, S. aut Panareo, M. aut Paoletti, R. aut Perasso, L. aut Pilo, F. aut Piragino, G. aut Regano, A. aut Riggi, F. aut Righini, G. C. aut Sartorelli, G. aut Scapparone, E. aut Scribano, A. aut Selvi, M. aut Serci, S. aut Siddi, E. aut Spandre, G. aut Squarcia, S. aut Taiuti, M. aut Tosello, F. aut Votano, L. aut Williams, M. C. S. aut Yánez, G. aut Zichichi, A. aut Zuyeuski, R. aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 8 vom: 11. Aug. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:8 day:11 month:08 https://dx.doi.org/10.1140/epjp/i2014-14166-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 129 2014 8 11 08 |
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10.1140/epjp/i2014-14166-3 doi (DE-627)SPR031455433 (SPR)i2014-14166-3-e DE-627 ger DE-627 rakwb eng Abbrescia, M. verfasserin aut Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. Observation Level (dpeaa)DE-He213 Coincidence Event (dpeaa)DE-He213 Primary Proton (dpeaa)DE-He213 Muon Component (dpeaa)DE-He213 Shower Core (dpeaa)DE-He213 Agocs, A. aut Aiola, S. aut Antolini, R. aut Avanzini, C. aut Baldini Ferroli, R. aut Bencivenni, G. aut Bossini, E. aut Bressan, E. aut Chiavassa, A. aut Cicalò, C. aut Cifarelli, L. aut Coccia, E. aut De Gruttola, D. aut De Pasquale, S. aut Di Giovanni, A. aut D’Incecco, M. aut Dreucci, M. aut Fabbri, F. L. aut Frolov, V. aut Garbini, M. aut Gemme, G. aut Gnesi, I. aut Gustavino, C. aut Hatzifotiadou, D. aut La Rocca, P. aut Li, S. aut Librizzi, F. aut Maggiora, A. aut Massai, M. aut Miozzi, S. aut Panareo, M. aut Paoletti, R. aut Perasso, L. aut Pilo, F. aut Piragino, G. aut Regano, A. aut Riggi, F. aut Righini, G. C. aut Sartorelli, G. aut Scapparone, E. aut Scribano, A. aut Selvi, M. aut Serci, S. aut Siddi, E. aut Spandre, G. aut Squarcia, S. aut Taiuti, M. aut Tosello, F. aut Votano, L. aut Williams, M. C. S. aut Yánez, G. aut Zichichi, A. aut Zuyeuski, R. aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 8 vom: 11. Aug. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:8 day:11 month:08 https://dx.doi.org/10.1140/epjp/i2014-14166-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 129 2014 8 11 08 |
| allfieldsGer |
10.1140/epjp/i2014-14166-3 doi (DE-627)SPR031455433 (SPR)i2014-14166-3-e DE-627 ger DE-627 rakwb eng Abbrescia, M. verfasserin aut Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. Observation Level (dpeaa)DE-He213 Coincidence Event (dpeaa)DE-He213 Primary Proton (dpeaa)DE-He213 Muon Component (dpeaa)DE-He213 Shower Core (dpeaa)DE-He213 Agocs, A. aut Aiola, S. aut Antolini, R. aut Avanzini, C. aut Baldini Ferroli, R. aut Bencivenni, G. aut Bossini, E. aut Bressan, E. aut Chiavassa, A. aut Cicalò, C. aut Cifarelli, L. aut Coccia, E. aut De Gruttola, D. aut De Pasquale, S. aut Di Giovanni, A. aut D’Incecco, M. aut Dreucci, M. aut Fabbri, F. L. aut Frolov, V. aut Garbini, M. aut Gemme, G. aut Gnesi, I. aut Gustavino, C. aut Hatzifotiadou, D. aut La Rocca, P. aut Li, S. aut Librizzi, F. aut Maggiora, A. aut Massai, M. aut Miozzi, S. aut Panareo, M. aut Paoletti, R. aut Perasso, L. aut Pilo, F. aut Piragino, G. aut Regano, A. aut Riggi, F. aut Righini, G. C. aut Sartorelli, G. aut Scapparone, E. aut Scribano, A. aut Selvi, M. aut Serci, S. aut Siddi, E. aut Spandre, G. aut Squarcia, S. aut Taiuti, M. aut Tosello, F. aut Votano, L. aut Williams, M. C. S. aut Yánez, G. aut Zichichi, A. aut Zuyeuski, R. aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 8 vom: 11. Aug. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:8 day:11 month:08 https://dx.doi.org/10.1140/epjp/i2014-14166-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 129 2014 8 11 08 |
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Abbrescia, M. @@aut@@ Agocs, A. @@aut@@ Aiola, S. @@aut@@ Antolini, R. @@aut@@ Avanzini, C. @@aut@@ Baldini Ferroli, R. @@aut@@ Bencivenni, G. @@aut@@ Bossini, E. @@aut@@ Bressan, E. @@aut@@ Chiavassa, A. @@aut@@ Cicalò, C. @@aut@@ Cifarelli, L. @@aut@@ Coccia, E. @@aut@@ De Gruttola, D. @@aut@@ De Pasquale, S. @@aut@@ Di Giovanni, A. @@aut@@ D’Incecco, M. @@aut@@ Dreucci, M. @@aut@@ Fabbri, F. L. @@aut@@ Frolov, V. @@aut@@ Garbini, M. @@aut@@ Gemme, G. @@aut@@ Gnesi, I. @@aut@@ Gustavino, C. @@aut@@ Hatzifotiadou, D. @@aut@@ La Rocca, P. @@aut@@ Li, S. @@aut@@ Librizzi, F. @@aut@@ Maggiora, A. @@aut@@ Massai, M. @@aut@@ Miozzi, S. @@aut@@ Panareo, M. @@aut@@ Paoletti, R. @@aut@@ Perasso, L. @@aut@@ Pilo, F. @@aut@@ Piragino, G. @@aut@@ Regano, A. @@aut@@ Riggi, F. @@aut@@ Righini, G. C. @@aut@@ Sartorelli, G. @@aut@@ Scapparone, E. @@aut@@ Scribano, A. @@aut@@ Selvi, M. @@aut@@ Serci, S. @@aut@@ Siddi, E. @@aut@@ Spandre, G. @@aut@@ Squarcia, S. @@aut@@ Taiuti, M. @@aut@@ Tosello, F. @@aut@@ Votano, L. @@aut@@ Williams, M. C. S. @@aut@@ Yánez, G. @@aut@@ Zichichi, A. @@aut@@ Zuyeuski, R. @@aut@@ |
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Abbrescia, M. |
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Abbrescia, M. misc Observation Level misc Coincidence Event misc Primary Proton misc Muon Component misc Shower Core Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project |
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Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project Observation Level (dpeaa)DE-He213 Coincidence Event (dpeaa)DE-He213 Primary Proton (dpeaa)DE-He213 Muon Component (dpeaa)DE-He213 Shower Core (dpeaa)DE-He213 |
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Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project |
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Abbrescia, M. Agocs, A. Aiola, S. Antolini, R. Avanzini, C. Baldini Ferroli, R. Bencivenni, G. Bossini, E. Bressan, E. Chiavassa, A. Cicalò, C. Cifarelli, L. Coccia, E. De Gruttola, D. De Pasquale, S. Di Giovanni, A. D’Incecco, M. Dreucci, M. Fabbri, F. L. Frolov, V. Garbini, M. Gemme, G. Gnesi, I. Gustavino, C. Hatzifotiadou, D. La Rocca, P. Li, S. Librizzi, F. Maggiora, A. Massai, M. Miozzi, S. Panareo, M. Paoletti, R. Perasso, L. Pilo, F. Piragino, G. Regano, A. Riggi, F. Righini, G. C. Sartorelli, G. Scapparone, E. Scribano, A. Selvi, M. Serci, S. Siddi, E. Spandre, G. Squarcia, S. Taiuti, M. Tosello, F. Votano, L. Williams, M. C. S. Yánez, G. Zichichi, A. Zuyeuski, R. |
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Elektronische Aufsätze |
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Abbrescia, M. |
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10.1140/epjp/i2014-14166-3 |
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cosmic rays monte carlo simulations for the extreme energy events project |
| title_auth |
Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project |
| abstract |
Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 |
| abstractGer |
Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 |
| abstract_unstemmed |
Abstract The Extreme Energy Events Project (EEE Project) is an innovative experiment to study very high energy cosmic rays by means of the detection of the associated air shower muon component. It consists of a network of tracking detectors installed inside Italian High Schools. Each tracking detector, called EEE telescope, is composed of three Multigap Resistive Plate Chambers (MRPCs). At present, 43 telescopes are installed and taking data, opening the way for the detection of far away coincidences over a total area of about 3 × $ 10^{5} $ $ km^{2} $. In this paper we present the Monte Carlo simulations that have been performed to predict the expected coincidence rate between distant EEE telescopes. © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 |
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Cosmic rays Monte Carlo simulations for the Extreme Energy Events Project |
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https://dx.doi.org/10.1140/epjp/i2014-14166-3 |
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Agocs, A. Aiola, S. Antolini, R. Avanzini, C. Baldini Ferroli, R. Bencivenni, G. Bossini, E. Bressan, E. Chiavassa, A. Cicalò, C. Cifarelli, L. Coccia, E. De Gruttola, D. De Pasquale, S. Di Giovanni, A. D’Incecco, M. Dreucci, M. Fabbri, F. L. Frolov, V. Garbini, M. Gemme, G. Gnesi, I. Gustavino, C. Hatzifotiadou, D. La Rocca, P. Li, S. Librizzi, F. Maggiora, A. Massai, M. Miozzi, S. Panareo, M. Paoletti, R. Perasso, L. Pilo, F. Piragino, G. Regano, A. Riggi, F. Righini, G. C. Sartorelli, G. Scapparone, E. Scribano, A. Selvi, M. Serci, S. Siddi, E. Spandre, G. Squarcia, S. Taiuti, M. Tosello, F. Votano, L. Williams, M. C. S. Yánez, G. Zichichi, A. Zuyeuski, R. |
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Agocs, A. Aiola, S. Antolini, R. Avanzini, C. Baldini Ferroli, R. Bencivenni, G. Bossini, E. Bressan, E. Chiavassa, A. Cicalò, C. Cifarelli, L. Coccia, E. De Gruttola, D. De Pasquale, S. Di Giovanni, A. D’Incecco, M. Dreucci, M. Fabbri, F. L. Frolov, V. Garbini, M. Gemme, G. Gnesi, I. Gustavino, C. Hatzifotiadou, D. La Rocca, P. Li, S. Librizzi, F. Maggiora, A. Massai, M. Miozzi, S. Panareo, M. Paoletti, R. Perasso, L. Pilo, F. Piragino, G. Regano, A. Riggi, F. Righini, G. C. Sartorelli, G. Scapparone, E. Scribano, A. Selvi, M. Serci, S. Siddi, E. Spandre, G. Squarcia, S. Taiuti, M. Tosello, F. Votano, L. Williams, M. C. S. Yánez, G. Zichichi, A. Zuyeuski, R. |
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2024-07-03T23:48:21.729Z |
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| score |
7.399583 |