Meteor studies in the framework of the JEM-EUSO program
We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect mete...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Abdellaoui, G [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Übergeordnetes Werk: |
Enthalten in: Planetary and space science - New York, NY : Elsevier, 1959, 143(2016), Seite 245 |
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| Übergeordnetes Werk: |
volume:143 ; year:2016 ; pages:245 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.pss.2016.12.001 |
|---|
| Katalog-ID: |
OLC1997534487 |
|---|
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| 520 | |a We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. | ||
| 700 | 1 | |a Abe, S |4 oth | |
| 700 | 1 | |a Acheli, A |4 oth | |
| 700 | 1 | |a Adams, J.H |4 oth | |
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10.1016/j.pss.2016.12.001 doi PQ20171228 (DE-627)OLC1997534487 (DE-599)GBVOLC1997534487 (PRQ)c1826-7db330e07dd8f0526b5b1c63ca463035c23596d2628e8dcd2a179237fb8c62670 (KEY)0077938520160000143000000245meteorstudiesintheframeworkofthejemeusoprogram DE-627 ger DE-627 rakwb eng 620 DNB 39.00 bkl 50.93 bkl Abdellaoui, G verfasserin aut Meteor studies in the framework of the JEM-EUSO program 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. 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, A oth Belov, K 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 Cordero, 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 Fouka, M oth Franceschi, A oth Franchini, S oth Fuglesang, C oth ... oth Enthalten in Planetary and space science New York, NY : Elsevier, 1959 143(2016), Seite 245 (DE-627)129602205 (DE-600)241527-6 (DE-576)015095932 0032-0633 nnns volume:143 year:2016 pages:245 http://dx.doi.org/10.1016/j.pss.2016.12.001 Volltext http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-211312 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_70 GBV_ILN_2279 39.00 AVZ 50.93 AVZ AR 143 2016 245 |
| spelling |
10.1016/j.pss.2016.12.001 doi PQ20171228 (DE-627)OLC1997534487 (DE-599)GBVOLC1997534487 (PRQ)c1826-7db330e07dd8f0526b5b1c63ca463035c23596d2628e8dcd2a179237fb8c62670 (KEY)0077938520160000143000000245meteorstudiesintheframeworkofthejemeusoprogram DE-627 ger DE-627 rakwb eng 620 DNB 39.00 bkl 50.93 bkl Abdellaoui, G verfasserin aut Meteor studies in the framework of the JEM-EUSO program 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. 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, A oth Belov, K 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 Cordero, 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 Fouka, M oth Franceschi, A oth Franchini, S oth Fuglesang, C oth ... oth Enthalten in Planetary and space science New York, NY : Elsevier, 1959 143(2016), Seite 245 (DE-627)129602205 (DE-600)241527-6 (DE-576)015095932 0032-0633 nnns volume:143 year:2016 pages:245 http://dx.doi.org/10.1016/j.pss.2016.12.001 Volltext http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-211312 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_70 GBV_ILN_2279 39.00 AVZ 50.93 AVZ AR 143 2016 245 |
| allfields_unstemmed |
10.1016/j.pss.2016.12.001 doi PQ20171228 (DE-627)OLC1997534487 (DE-599)GBVOLC1997534487 (PRQ)c1826-7db330e07dd8f0526b5b1c63ca463035c23596d2628e8dcd2a179237fb8c62670 (KEY)0077938520160000143000000245meteorstudiesintheframeworkofthejemeusoprogram DE-627 ger DE-627 rakwb eng 620 DNB 39.00 bkl 50.93 bkl Abdellaoui, G verfasserin aut Meteor studies in the framework of the JEM-EUSO program 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. 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, A oth Belov, K 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 Cordero, 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 Fouka, M oth Franceschi, A oth Franchini, S oth Fuglesang, C oth ... oth Enthalten in Planetary and space science New York, NY : Elsevier, 1959 143(2016), Seite 245 (DE-627)129602205 (DE-600)241527-6 (DE-576)015095932 0032-0633 nnns volume:143 year:2016 pages:245 http://dx.doi.org/10.1016/j.pss.2016.12.001 Volltext http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-211312 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_70 GBV_ILN_2279 39.00 AVZ 50.93 AVZ AR 143 2016 245 |
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10.1016/j.pss.2016.12.001 doi PQ20171228 (DE-627)OLC1997534487 (DE-599)GBVOLC1997534487 (PRQ)c1826-7db330e07dd8f0526b5b1c63ca463035c23596d2628e8dcd2a179237fb8c62670 (KEY)0077938520160000143000000245meteorstudiesintheframeworkofthejemeusoprogram DE-627 ger DE-627 rakwb eng 620 DNB 39.00 bkl 50.93 bkl Abdellaoui, G verfasserin aut Meteor studies in the framework of the JEM-EUSO program 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. 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, A oth Belov, K 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 Cordero, 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 Fouka, M oth Franceschi, A oth Franchini, S oth Fuglesang, C oth ... oth Enthalten in Planetary and space science New York, NY : Elsevier, 1959 143(2016), Seite 245 (DE-627)129602205 (DE-600)241527-6 (DE-576)015095932 0032-0633 nnns volume:143 year:2016 pages:245 http://dx.doi.org/10.1016/j.pss.2016.12.001 Volltext http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-211312 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_70 GBV_ILN_2279 39.00 AVZ 50.93 AVZ AR 143 2016 245 |
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10.1016/j.pss.2016.12.001 doi PQ20171228 (DE-627)OLC1997534487 (DE-599)GBVOLC1997534487 (PRQ)c1826-7db330e07dd8f0526b5b1c63ca463035c23596d2628e8dcd2a179237fb8c62670 (KEY)0077938520160000143000000245meteorstudiesintheframeworkofthejemeusoprogram DE-627 ger DE-627 rakwb eng 620 DNB 39.00 bkl 50.93 bkl Abdellaoui, G verfasserin aut Meteor studies in the framework of the JEM-EUSO program 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. 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, A oth Belov, K 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 Cordero, 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 Fouka, M oth Franceschi, A oth Franchini, S oth Fuglesang, C oth ... oth Enthalten in Planetary and space science New York, NY : Elsevier, 1959 143(2016), Seite 245 (DE-627)129602205 (DE-600)241527-6 (DE-576)015095932 0032-0633 nnns volume:143 year:2016 pages:245 http://dx.doi.org/10.1016/j.pss.2016.12.001 Volltext http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-211312 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_70 GBV_ILN_2279 39.00 AVZ 50.93 AVZ AR 143 2016 245 |
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Abdellaoui, G @@aut@@ 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, A @@oth@@ Belov, K @@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@@ Cordero, 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@@ Fouka, M @@oth@@ Franceschi, A @@oth@@ Franchini, S @@oth@@ Fuglesang, C @@oth@@ ... @@oth@@ |
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meteor studies in the framework of the jem-euso program |
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Meteor studies in the framework of the JEM-EUSO program |
| abstract |
We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. |
| abstractGer |
We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. |
| abstract_unstemmed |
We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This means that JEM-EUSO should be able to record a statistically significant flux of meteors, including both sporadic ones, and events produced by different meteor streams. Being unaffected by adverse weather conditions, JEM-EUSO can also be a very important facility for the detection of bright meteors and fireballs, as these events can be detected even in conditions of very high sky background. In the case of bright events, moreover, exhibiting some persistence of the meteor train, preliminary simulations show that it should be possible to exploit the motion of the ISS itself and derive at least a rough 3D reconstruction of the meteor trajectory. Moreover, the observing strategy developed to detect meteors may also be applied to the detection of nuclearites, exotic particles whose existence has been suggested by some theoretical investigations. Nuclearites are expected to move at higher velocities than meteoroids, and to exhibit a wider range of possible trajectories, including particles moving upward after crossing the Earth. Some pilot studies, including the approved Mini-EUSO mission, a precursor of JEM-EUSO, are currently operational or in preparation. We are doing simulations to assess the performance of Mini-EUSO for meteor studies, while a few meteor events have been already detected using the ground-based facility EUSO-TA. |
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| title_short |
Meteor studies in the framework of the JEM-EUSO program |
| url |
http://dx.doi.org/10.1016/j.pss.2016.12.001 http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-211312 |
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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, A Belov, K 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 Cordero, 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 Fouka, M Franceschi, A Franchini, S Fuglesang, C . |
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