Cosmic ray oriented performance studies for the JEM-EUSO first level trigger
JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly spec...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Abdellaoui, G [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Rechteinformationen: |
Nutzungsrecht: © Elsevier B.V. © Distributed under a Creative Commons Attribution 4.0 International License |
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| Schlagwörter: |
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| Systematik: |
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| Übergeordnetes Werk: |
Enthalten in: Nuclear instruments & methods in physics research / A - Amsterdam : North-Holland Publ. Co., 1984, 866(2017), Seite 150-163 |
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| Übergeordnetes Werk: |
volume:866 ; year:2017 ; pages:150-163 |
| Links: |
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| DOI / URN: |
10.1016/j.nima.2017.05.043 |
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| Katalog-ID: |
OLC1999323572 |
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| 520 | |a JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. | ||
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10.1016/j.nima.2017.05.043 doi PQ20171228 (DE-627)OLC1999323572 (DE-599)GBVOLC1999323572 (PRQ)e1975-f327144c9f955dc3e78d83e54da920013db9ec3a6a9c685c87298c536978bb230 (KEY)0136675020170000866000000150cosmicrayorientedperformancestudiesforthejemeusofi DE-627 ger DE-627 rakwb eng 530 DE-600 UA 5680. AVZ rvk Abdellaoui, G verfasserin aut Cosmic ray oriented performance studies for the JEM-EUSO first level trigger 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. Nutzungsrecht: © Elsevier B.V. © Distributed under a Creative Commons Attribution 4.0 International License Nightglow background JEM-EUSO Trigger system FPGA Instrumentation and Detectors Physics Abe, S oth Acheli, A oth Adams, J.H oth Ahmad, S oth Ahriche, A oth Albert, J.-N oth Allard, D oth Alonso, G oth Anchordoqui, L oth Andreev, V oth Anzalone, A oth Aouimeur, W oth Arai, Y oth Arsene, N oth Asano, K oth Attallah, R oth Attoui, H oth Ave Pernas, M oth Bacholle, S oth Bakiri, M oth Baragatti, P oth Barrillon, P oth Bartocci, S oth Batsch, T oth Bayer, J oth Bechini, R oth Belenguer, T oth Bellotti, R oth Belov, K oth Belov, A oth Benadda, B oth Benmessai, K oth Berlind, A.A oth Bertaina, M oth Biermann, P.L oth Biktemerova, S oth Bisconti, F oth Blanc, N oth Błȩcki, J oth Blin-Bondil, S oth Bobik, P oth Bogomilov, M oth Bonamente, M oth Boudaoud, R oth Bozzo, E oth Briggs, M.S oth Bruno, A oth Caballero, K.S oth Cafagna, F oth Campana, D oth Capdevielle, J.-N oth Capel, F oth Caramete, A oth Caramete, L oth Carlson, P oth Caruso, R oth Casolino, M oth Cassardo, C oth Castellina, A oth Castellini, G oth Catalano, C oth Catalano, O oth Cellino, A oth Chikawa, M oth Chiritoi, G oth Christl, M.J oth Connaughton, V oth Conti, L oth Contino, G oth Cordero, G oth Cotto, G oth Crawford, H.J oth Cremonini, R oth Csorna, S oth Dagoret-Campagne, S oth De Donato, C oth de la Taille, C oth De Santis, C oth del Peral, L oth Di Martino, M oth Djemil, T oth Djenas, S.A oth Dulucq, F oth Dupieux, M oth Dutan, I oth Ebersoldt, A oth Ebisuzaki, T oth Engel, R oth Eser, J oth Fang, K oth Fenu, F oth Fernández-González, S oth Fernández-Soriano, J oth Ferrarese, S oth Finco, D oth Flamini, M oth Fornaro, C oth Forza, R oth Fouka, M oth ... oth Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 866(2017), Seite 150-163 (DE-627)129862134 (DE-600)283627-0 (DE-576)015173461 0167-5087 nnns volume:866 year:2017 pages:150-163 http://dx.doi.org/10.1016/j.nima.2017.05.043 Volltext https://www.sciencedirect.com/science/article/pii/S016890021730596X https://hal.archives-ouvertes.fr/hal-01555206 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214415 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_70 GBV_ILN_170 UA 5680. AR 866 2017 150-163 |
| spelling |
10.1016/j.nima.2017.05.043 doi PQ20171228 (DE-627)OLC1999323572 (DE-599)GBVOLC1999323572 (PRQ)e1975-f327144c9f955dc3e78d83e54da920013db9ec3a6a9c685c87298c536978bb230 (KEY)0136675020170000866000000150cosmicrayorientedperformancestudiesforthejemeusofi DE-627 ger DE-627 rakwb eng 530 DE-600 UA 5680. AVZ rvk Abdellaoui, G verfasserin aut Cosmic ray oriented performance studies for the JEM-EUSO first level trigger 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. Nutzungsrecht: © Elsevier B.V. © Distributed under a Creative Commons Attribution 4.0 International License Nightglow background JEM-EUSO Trigger system FPGA Instrumentation and Detectors Physics Abe, S oth Acheli, A oth Adams, J.H oth Ahmad, S oth Ahriche, A oth Albert, J.-N oth Allard, D oth Alonso, G oth Anchordoqui, L oth Andreev, V oth Anzalone, A oth Aouimeur, W oth Arai, Y oth Arsene, N oth Asano, K oth Attallah, R oth Attoui, H oth Ave Pernas, M oth Bacholle, S oth Bakiri, M oth Baragatti, P oth Barrillon, P oth Bartocci, S oth Batsch, T oth Bayer, J oth Bechini, R oth Belenguer, T oth Bellotti, R oth Belov, K oth Belov, A oth Benadda, B oth Benmessai, K oth Berlind, A.A oth Bertaina, M oth Biermann, P.L oth Biktemerova, S oth Bisconti, F oth Blanc, N oth Błȩcki, J oth Blin-Bondil, S oth Bobik, P oth Bogomilov, M oth Bonamente, M oth Boudaoud, R oth Bozzo, E oth Briggs, M.S oth Bruno, A oth Caballero, K.S oth Cafagna, F oth Campana, D oth Capdevielle, J.-N oth Capel, F oth Caramete, A oth Caramete, L oth Carlson, P oth Caruso, R oth Casolino, M oth Cassardo, C oth Castellina, A oth Castellini, G oth Catalano, C oth Catalano, O oth Cellino, A oth Chikawa, M oth Chiritoi, G oth Christl, M.J oth Connaughton, V oth Conti, L oth Contino, G oth Cordero, G oth Cotto, G oth Crawford, H.J oth Cremonini, R oth Csorna, S oth Dagoret-Campagne, S oth De Donato, C oth de la Taille, C oth De Santis, C oth del Peral, L oth Di Martino, M oth Djemil, T oth Djenas, S.A oth Dulucq, F oth Dupieux, M oth Dutan, I oth Ebersoldt, A oth Ebisuzaki, T oth Engel, R oth Eser, J oth Fang, K oth Fenu, F oth Fernández-González, S oth Fernández-Soriano, J oth Ferrarese, S oth Finco, D oth Flamini, M oth Fornaro, C oth Forza, R oth Fouka, M oth ... oth Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 866(2017), Seite 150-163 (DE-627)129862134 (DE-600)283627-0 (DE-576)015173461 0167-5087 nnns volume:866 year:2017 pages:150-163 http://dx.doi.org/10.1016/j.nima.2017.05.043 Volltext https://www.sciencedirect.com/science/article/pii/S016890021730596X https://hal.archives-ouvertes.fr/hal-01555206 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214415 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_70 GBV_ILN_170 UA 5680. AR 866 2017 150-163 |
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10.1016/j.nima.2017.05.043 doi PQ20171228 (DE-627)OLC1999323572 (DE-599)GBVOLC1999323572 (PRQ)e1975-f327144c9f955dc3e78d83e54da920013db9ec3a6a9c685c87298c536978bb230 (KEY)0136675020170000866000000150cosmicrayorientedperformancestudiesforthejemeusofi DE-627 ger DE-627 rakwb eng 530 DE-600 UA 5680. AVZ rvk Abdellaoui, G verfasserin aut Cosmic ray oriented performance studies for the JEM-EUSO first level trigger 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. Nutzungsrecht: © Elsevier B.V. © Distributed under a Creative Commons Attribution 4.0 International License Nightglow background JEM-EUSO Trigger system FPGA Instrumentation and Detectors Physics Abe, S oth Acheli, A oth Adams, J.H oth Ahmad, S oth Ahriche, A oth Albert, J.-N oth Allard, D oth Alonso, G oth Anchordoqui, L oth Andreev, V oth Anzalone, A oth Aouimeur, W oth Arai, Y oth Arsene, N oth Asano, K oth Attallah, R oth Attoui, H oth Ave Pernas, M oth Bacholle, S oth Bakiri, M oth Baragatti, P oth Barrillon, P oth Bartocci, S oth Batsch, T oth Bayer, J oth Bechini, R oth Belenguer, T oth Bellotti, R oth Belov, K oth Belov, A oth Benadda, B oth Benmessai, K oth Berlind, A.A oth Bertaina, M oth Biermann, P.L oth Biktemerova, S oth Bisconti, F oth Blanc, N oth Błȩcki, J oth Blin-Bondil, S oth Bobik, P oth Bogomilov, M oth Bonamente, M oth Boudaoud, R oth Bozzo, E oth Briggs, M.S oth Bruno, A oth Caballero, K.S oth Cafagna, F oth Campana, D oth Capdevielle, J.-N oth Capel, F oth Caramete, A oth Caramete, L oth Carlson, P oth Caruso, R oth Casolino, M oth Cassardo, C oth Castellina, A oth Castellini, G oth Catalano, C oth Catalano, O oth Cellino, A oth Chikawa, M oth Chiritoi, G oth Christl, M.J oth Connaughton, V oth Conti, L oth Contino, G oth Cordero, G oth Cotto, G oth Crawford, H.J oth Cremonini, R oth Csorna, S oth Dagoret-Campagne, S oth De Donato, C oth de la Taille, C oth De Santis, C oth del Peral, L oth Di Martino, M oth Djemil, T oth Djenas, S.A oth Dulucq, F oth Dupieux, M oth Dutan, I oth Ebersoldt, A oth Ebisuzaki, T oth Engel, R oth Eser, J oth Fang, K oth Fenu, F oth Fernández-González, S oth Fernández-Soriano, J oth Ferrarese, S oth Finco, D oth Flamini, M oth Fornaro, C oth Forza, R oth Fouka, M oth ... oth Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 866(2017), Seite 150-163 (DE-627)129862134 (DE-600)283627-0 (DE-576)015173461 0167-5087 nnns volume:866 year:2017 pages:150-163 http://dx.doi.org/10.1016/j.nima.2017.05.043 Volltext https://www.sciencedirect.com/science/article/pii/S016890021730596X https://hal.archives-ouvertes.fr/hal-01555206 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214415 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_70 GBV_ILN_170 UA 5680. AR 866 2017 150-163 |
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10.1016/j.nima.2017.05.043 doi PQ20171228 (DE-627)OLC1999323572 (DE-599)GBVOLC1999323572 (PRQ)e1975-f327144c9f955dc3e78d83e54da920013db9ec3a6a9c685c87298c536978bb230 (KEY)0136675020170000866000000150cosmicrayorientedperformancestudiesforthejemeusofi DE-627 ger DE-627 rakwb eng 530 DE-600 UA 5680. AVZ rvk Abdellaoui, G verfasserin aut Cosmic ray oriented performance studies for the JEM-EUSO first level trigger 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. Nutzungsrecht: © Elsevier B.V. © Distributed under a Creative Commons Attribution 4.0 International License Nightglow background JEM-EUSO Trigger system FPGA Instrumentation and Detectors Physics Abe, S oth Acheli, A oth Adams, J.H oth Ahmad, S oth Ahriche, A oth Albert, J.-N oth Allard, D oth Alonso, G oth Anchordoqui, L oth Andreev, V oth Anzalone, A oth Aouimeur, W oth Arai, Y oth Arsene, N oth Asano, K oth Attallah, R oth Attoui, H oth Ave Pernas, M oth Bacholle, S oth Bakiri, M oth Baragatti, P oth Barrillon, P oth Bartocci, S oth Batsch, T oth Bayer, J oth Bechini, R oth Belenguer, T oth Bellotti, R oth Belov, K oth Belov, A oth Benadda, B oth Benmessai, K oth Berlind, A.A oth Bertaina, M oth Biermann, P.L oth Biktemerova, S oth Bisconti, F oth Blanc, N oth Błȩcki, J oth Blin-Bondil, S oth Bobik, P oth Bogomilov, M oth Bonamente, M oth Boudaoud, R oth Bozzo, E oth Briggs, M.S oth Bruno, A oth Caballero, K.S oth Cafagna, F oth Campana, D oth Capdevielle, J.-N oth Capel, F oth Caramete, A oth Caramete, L oth Carlson, P oth Caruso, R oth Casolino, M oth Cassardo, C oth Castellina, A oth Castellini, G oth Catalano, C oth Catalano, O oth Cellino, A oth Chikawa, M oth Chiritoi, G oth Christl, M.J oth Connaughton, V oth Conti, L oth Contino, G oth Cordero, G oth Cotto, G oth Crawford, H.J oth Cremonini, R oth Csorna, S oth Dagoret-Campagne, S oth De Donato, C oth de la Taille, C oth De Santis, C oth del Peral, L oth Di Martino, M oth Djemil, T oth Djenas, S.A oth Dulucq, F oth Dupieux, M oth Dutan, I oth Ebersoldt, A oth Ebisuzaki, T oth Engel, R oth Eser, J oth Fang, K oth Fenu, F oth Fernández-González, S oth Fernández-Soriano, J oth Ferrarese, S oth Finco, D oth Flamini, M oth Fornaro, C oth Forza, R oth Fouka, M oth ... oth Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 866(2017), Seite 150-163 (DE-627)129862134 (DE-600)283627-0 (DE-576)015173461 0167-5087 nnns volume:866 year:2017 pages:150-163 http://dx.doi.org/10.1016/j.nima.2017.05.043 Volltext https://www.sciencedirect.com/science/article/pii/S016890021730596X https://hal.archives-ouvertes.fr/hal-01555206 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214415 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_70 GBV_ILN_170 UA 5680. AR 866 2017 150-163 |
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10.1016/j.nima.2017.05.043 doi PQ20171228 (DE-627)OLC1999323572 (DE-599)GBVOLC1999323572 (PRQ)e1975-f327144c9f955dc3e78d83e54da920013db9ec3a6a9c685c87298c536978bb230 (KEY)0136675020170000866000000150cosmicrayorientedperformancestudiesforthejemeusofi DE-627 ger DE-627 rakwb eng 530 DE-600 UA 5680. AVZ rvk Abdellaoui, G verfasserin aut Cosmic ray oriented performance studies for the JEM-EUSO first level trigger 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. Nutzungsrecht: © Elsevier B.V. © Distributed under a Creative Commons Attribution 4.0 International License Nightglow background JEM-EUSO Trigger system FPGA Instrumentation and Detectors Physics Abe, S oth Acheli, A oth Adams, J.H oth Ahmad, S oth Ahriche, A oth Albert, J.-N oth Allard, D oth Alonso, G oth Anchordoqui, L oth Andreev, V oth Anzalone, A oth Aouimeur, W oth Arai, Y oth Arsene, N oth Asano, K oth Attallah, R oth Attoui, H oth Ave Pernas, M oth Bacholle, S oth Bakiri, M oth Baragatti, P oth Barrillon, P oth Bartocci, S oth Batsch, T oth Bayer, J oth Bechini, R oth Belenguer, T oth Bellotti, R oth Belov, K oth Belov, A oth Benadda, B oth Benmessai, K oth Berlind, A.A oth Bertaina, M oth Biermann, P.L oth Biktemerova, S oth Bisconti, F oth Blanc, N oth Błȩcki, J oth Blin-Bondil, S oth Bobik, P oth Bogomilov, M oth Bonamente, M oth Boudaoud, R oth Bozzo, E oth Briggs, M.S oth Bruno, A oth Caballero, K.S oth Cafagna, F oth Campana, D oth Capdevielle, J.-N oth Capel, F oth Caramete, A oth Caramete, L oth Carlson, P oth Caruso, R oth Casolino, M oth Cassardo, C oth Castellina, A oth Castellini, G oth Catalano, C oth Catalano, O oth Cellino, A oth Chikawa, M oth Chiritoi, G oth Christl, M.J oth Connaughton, V oth Conti, L oth Contino, G oth Cordero, G oth Cotto, G oth Crawford, H.J oth Cremonini, R oth Csorna, S oth Dagoret-Campagne, S oth De Donato, C oth de la Taille, C oth De Santis, C oth del Peral, L oth Di Martino, M oth Djemil, T oth Djenas, S.A oth Dulucq, F oth Dupieux, M oth Dutan, I oth Ebersoldt, A oth Ebisuzaki, T oth Engel, R oth Eser, J oth Fang, K oth Fenu, F oth Fernández-González, S oth Fernández-Soriano, J oth Ferrarese, S oth Finco, D oth Flamini, M oth Fornaro, C oth Forza, R oth Fouka, M oth ... oth Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 866(2017), Seite 150-163 (DE-627)129862134 (DE-600)283627-0 (DE-576)015173461 0167-5087 nnns volume:866 year:2017 pages:150-163 http://dx.doi.org/10.1016/j.nima.2017.05.043 Volltext https://www.sciencedirect.com/science/article/pii/S016890021730596X https://hal.archives-ouvertes.fr/hal-01555206 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214415 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_70 GBV_ILN_170 UA 5680. AR 866 2017 150-163 |
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Cosmic ray oriented performance studies for the JEM-EUSO first level trigger |
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cosmic ray oriented performance studies for the jem-euso first level trigger |
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Cosmic ray oriented performance studies for the JEM-EUSO first level trigger |
| abstract |
JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. |
| abstractGer |
JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. |
| abstract_unstemmed |
JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos ( E>5⋅1019eV ) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics. |
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GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_70 GBV_ILN_170 |
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Cosmic ray oriented performance studies for the JEM-EUSO first level trigger |
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http://dx.doi.org/10.1016/j.nima.2017.05.043 https://www.sciencedirect.com/science/article/pii/S016890021730596X https://hal.archives-ouvertes.fr/hal-01555206 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-214415 |
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Abe, S Acheli, A Adams, J.H Ahmad, S Ahriche, A Albert, J.-N Allard, D Alonso, G Anchordoqui, L Andreev, V Anzalone, A Aouimeur, W Arai, Y Arsene, N Asano, K Attallah, R Attoui, H Ave Pernas, M Bacholle, S Bakiri, M Baragatti, P Barrillon, P Bartocci, S Batsch, T Bayer, J Bechini, R Belenguer, T Bellotti, R Belov, K Belov, A Benadda, B Benmessai, K Berlind, A.A Bertaina, M Biermann, P.L Biktemerova, S Bisconti, F Blanc, N Błȩcki, J Blin-Bondil, S Bobik, P Bogomilov, M Bonamente, M Boudaoud, R Bozzo, E Briggs, M.S Bruno, A Caballero, K.S Cafagna, F Campana, D Capdevielle, J.-N Capel, F Caramete, A Caramete, L Carlson, P Caruso, R Casolino, M Cassardo, C Castellina, A Castellini, G Catalano, C Catalano, O Cellino, A Chikawa, M Chiritoi, G Christl, M.J Connaughton, V Conti, L Contino, G Cordero, G Cotto, G Crawford, H.J Cremonini, R Csorna, S Dagoret-Campagne, S De Donato, C de la Taille, C De Santis, C del Peral, L Di Martino, M Djemil, T Djenas, S.A Dulucq, F Dupieux, M Dutan, I Ebersoldt, A Ebisuzaki, T Engel, R Eser, J Fang, K Fenu, F Fernández-González, S Fernández-Soriano, J Ferrarese, S Finco, D Flamini, M Fornaro, C Forza, R Fouka, M . |
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Abe, S Acheli, A Adams, J.H Ahmad, S Ahriche, A Albert, J.-N Allard, D Alonso, G Anchordoqui, L Andreev, V Anzalone, A Aouimeur, W Arai, Y Arsene, N Asano, K Attallah, R Attoui, H Ave Pernas, M Bacholle, S Bakiri, M Baragatti, P Barrillon, P Bartocci, S Batsch, T Bayer, J Bechini, R Belenguer, T Bellotti, R Belov, K Belov, A Benadda, B Benmessai, K Berlind, A.A Bertaina, M Biermann, P.L Biktemerova, S Bisconti, F Blanc, N Błȩcki, J Blin-Bondil, S Bobik, P Bogomilov, M Bonamente, M Boudaoud, R Bozzo, E Briggs, M.S Bruno, A Caballero, K.S Cafagna, F Campana, D Capdevielle, J.-N Capel, F Caramete, A Caramete, L Carlson, P Caruso, R Casolino, M Cassardo, C Castellina, A Castellini, G Catalano, C Catalano, O Cellino, A Chikawa, M Chiritoi, G Christl, M.J Connaughton, V Conti, L Contino, G Cordero, G Cotto, G Crawford, H.J Cremonini, R Csorna, S Dagoret-Campagne, S De Donato, C de la Taille, C De Santis, C del Peral, L Di Martino, M Djemil, T Djenas, S.A Dulucq, F Dupieux, M Dutan, I Ebersoldt, A Ebisuzaki, T Engel, R Eser, J Fang, K Fenu, F Fernández-González, S Fernández-Soriano, J Ferrarese, S Finco, D Flamini, M Fornaro, C Forza, R Fouka, M . |
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| doi_str |
10.1016/j.nima.2017.05.043 |
| up_date |
2024-07-03T13:48:33.333Z |
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