The JEM-EUSO mission: An introduction
- Autores
- Adams, J. H.; Ahmad, S. 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.; Blecki, J.; Blin-Bondil, S.; Blumer, J.; Bobik, P.; Bogomilov, M.; Supanitsky, Alberto Daniel; The JEM-EUSO Collaboration
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The Extreme Universe Space Observatory on board the Japanese Experiment Module of the International Space Station, JEM-EUSO, is being designed tosearch from space ultra-high energy cosmic rays. These are charged particles with energies from a few 10^19 eV to beyond 10^20 eV, at the very end of the known cosmic ray energy spectrum. JEM-EUSO will also search for extreme energy neutrinos, photons, and exotic particles, providing a unique opportunity to explore largely unknown phenomena in our Universe. The mission, principally based on a wide field of view(60 degrees) near-UV telescope with a diameter of ~2.5 m, will monitor the earth?s atmosphere at night, pioneering the observation from space of the ultraviolet tracks (290-430 nm) associated with giant extensive air showers produced by ultra-high energy primaries propagating in the earth?s atmosphere. Observing from an orbital altitude of ~400 km, the mission is expected to reach an instantaneous geometrical aperture of A_geo >= 2 x 10^5 km^2 sr with an estimated duty cycle of ~20%. Sucha geometrical aperture allows unprecedented exposures, significantly larger than can be obtained with ground-based experiments. In this paper we briefly review the history of space-based search for ultra-high energy cosmic rays. We then introduce the special issue of Experimental Astronomy devoted to the various aspects of such a challenging enterprise. We also summarise the activities of the on-going JEM-EUSO program.
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, S. S.. Ecole Polytechnique; Francia
Fil: Albert, J. N.. Univ Paris-Sud; Francia
Fil: Allard, D.. Univ Paris Diderot; Francia
Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos
Fil: Andreev, V.. University of California; Estados Unidos
Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón
Fil: Asano, K.. Tokyo Institute of Technology; Japón
Fil: Ave Pernas, M.. Universidad de Alcala ; España
Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia
Fil: Barrillon, P.. Univ Paris-Sud; Francia
Fil: Batsch, T.. National Centre for Nuclear Research; Polonia
Fil: Bayer, J.. University of Tubinge; Alemania
Fil: Bechini, R.. Universita’ di Torino; Italia
Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial; España
Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare -; Italia
Fil: Belov, K.. University of California; Estados Unidos
Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos
Fil: Bertaina, M.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Biermann, P. L.. Karlsruhe Institute of Technology; Alemania
Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia
Fil: Blaksley, C.. Univ Paris Diderot; Francia
Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM),; Suiza
Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia
Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia
Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania
Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia
Fil: Bogomilov, M.. University of Sofia; Bulgaria
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: The JEM-EUSO Collaboration. - Materia
-
Ultra-High Energy Cosmic Rays
Neutrinos - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/18298
Ver los metadatos del registro completo
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The JEM-EUSO mission: An introductionAdams, J. H.Ahmad, S. 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.Blecki, J.Blin-Bondil, S.Blumer, J.Bobik, P.Bogomilov, M.Supanitsky, Alberto DanielThe JEM-EUSO CollaborationUltra-High Energy Cosmic RaysNeutrinoshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Extreme Universe Space Observatory on board the Japanese Experiment Module of the International Space Station, JEM-EUSO, is being designed tosearch from space ultra-high energy cosmic rays. These are charged particles with energies from a few 10^19 eV to beyond 10^20 eV, at the very end of the known cosmic ray energy spectrum. JEM-EUSO will also search for extreme energy neutrinos, photons, and exotic particles, providing a unique opportunity to explore largely unknown phenomena in our Universe. The mission, principally based on a wide field of view(60 degrees) near-UV telescope with a diameter of ~2.5 m, will monitor the earth?s atmosphere at night, pioneering the observation from space of the ultraviolet tracks (290-430 nm) associated with giant extensive air showers produced by ultra-high energy primaries propagating in the earth?s atmosphere. Observing from an orbital altitude of ~400 km, the mission is expected to reach an instantaneous geometrical aperture of A_geo >= 2 x 10^5 km^2 sr with an estimated duty cycle of ~20%. Sucha geometrical aperture allows unprecedented exposures, significantly larger than can be obtained with ground-based experiments. In this paper we briefly review the history of space-based search for ultra-high energy cosmic rays. We then introduce the special issue of Experimental Astronomy devoted to the various aspects of such a challenging enterprise. We also summarise the activities of the on-going JEM-EUSO program.Fil: Adams, J. H.. University of Alabama in Huntsville; Estados UnidosFil: Ahmad, S. S.. Ecole Polytechnique; FranciaFil: Albert, J. N.. Univ Paris-Sud; FranciaFil: Allard, D.. Univ Paris Diderot; FranciaFil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados UnidosFil: Andreev, V.. University of California; Estados UnidosFil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; ItaliaFil: Arai, Y.. High Energy Accelerator Research Organization (KEK); JapónFil: Asano, K.. Tokyo Institute of Technology; JapónFil: Ave Pernas, M.. Universidad de Alcala ; EspañaFil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; ItaliaFil: Barrillon, P.. Univ Paris-Sud; FranciaFil: Batsch, T.. National Centre for Nuclear Research; PoloniaFil: Bayer, J.. University of Tubinge; AlemaniaFil: Bechini, R.. Universita’ di Torino; ItaliaFil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial; EspañaFil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare -; ItaliaFil: Belov, K.. University of California; Estados UnidosFil: Berlind, A. A.. Vanderbilt University; Estados UnidosFil: Bertaina, M.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; ItaliaFil: Biermann, P. L.. Karlsruhe Institute of Technology; AlemaniaFil: Biktemerova, S.. Joint Institute for Nuclear Research; RusiaFil: Blaksley, C.. Univ Paris Diderot; FranciaFil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM),; SuizaFil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); PoloniaFil: Blin-Bondil, S.. Ecole Polytechnique; FranciaFil: Blumer, J.. Karlsruhe Institute of Technology (KIT); AlemaniaFil: Bobik, P.. Institute of Experimental Physics; EslovaquiaFil: Bogomilov, M.. University of Sofia; BulgariaFil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: The JEM-EUSO Collaboration.Springer2015-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/18298Adams, J. H.; Ahmad, S. S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; The JEM-EUSO mission: An introduction; Springer; Experimental Astronomy; 40; 1; 11-2015; 3-170922-6435CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-015-9482-xinfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10686-015-9482-xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:23:50Zoai:ri.conicet.gov.ar:11336/18298instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:23:50.675CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The JEM-EUSO mission: An introduction |
| title |
The JEM-EUSO mission: An introduction |
| spellingShingle |
The JEM-EUSO mission: An introduction Adams, J. H. Ultra-High Energy Cosmic Rays Neutrinos |
| title_short |
The JEM-EUSO mission: An introduction |
| title_full |
The JEM-EUSO mission: An introduction |
| title_fullStr |
The JEM-EUSO mission: An introduction |
| title_full_unstemmed |
The JEM-EUSO mission: An introduction |
| title_sort |
The JEM-EUSO mission: An introduction |
| dc.creator.none.fl_str_mv |
Adams, J. H. Ahmad, S. 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. Blecki, J. Blin-Bondil, S. Blumer, J. Bobik, P. Bogomilov, M. Supanitsky, Alberto Daniel The JEM-EUSO Collaboration |
| author |
Adams, J. H. |
| author_facet |
Adams, J. H. Ahmad, S. 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. Blecki, J. Blin-Bondil, S. Blumer, J. Bobik, P. Bogomilov, M. Supanitsky, Alberto Daniel The JEM-EUSO Collaboration |
| author_role |
author |
| author2 |
Ahmad, S. 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. Blecki, J. Blin-Bondil, S. Blumer, J. Bobik, P. Bogomilov, M. Supanitsky, Alberto Daniel The JEM-EUSO Collaboration |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Ultra-High Energy Cosmic Rays Neutrinos |
| topic |
Ultra-High Energy Cosmic Rays Neutrinos |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The Extreme Universe Space Observatory on board the Japanese Experiment Module of the International Space Station, JEM-EUSO, is being designed tosearch from space ultra-high energy cosmic rays. These are charged particles with energies from a few 10^19 eV to beyond 10^20 eV, at the very end of the known cosmic ray energy spectrum. JEM-EUSO will also search for extreme energy neutrinos, photons, and exotic particles, providing a unique opportunity to explore largely unknown phenomena in our Universe. The mission, principally based on a wide field of view(60 degrees) near-UV telescope with a diameter of ~2.5 m, will monitor the earth?s atmosphere at night, pioneering the observation from space of the ultraviolet tracks (290-430 nm) associated with giant extensive air showers produced by ultra-high energy primaries propagating in the earth?s atmosphere. Observing from an orbital altitude of ~400 km, the mission is expected to reach an instantaneous geometrical aperture of A_geo >= 2 x 10^5 km^2 sr with an estimated duty cycle of ~20%. Sucha geometrical aperture allows unprecedented exposures, significantly larger than can be obtained with ground-based experiments. In this paper we briefly review the history of space-based search for ultra-high energy cosmic rays. We then introduce the special issue of Experimental Astronomy devoted to the various aspects of such a challenging enterprise. We also summarise the activities of the on-going JEM-EUSO program. Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos Fil: Ahmad, S. S.. Ecole Polytechnique; Francia Fil: Albert, J. N.. Univ Paris-Sud; Francia Fil: Allard, D.. Univ Paris Diderot; Francia Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos Fil: Andreev, V.. University of California; Estados Unidos Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón Fil: Asano, K.. Tokyo Institute of Technology; Japón Fil: Ave Pernas, M.. Universidad de Alcala ; España Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia Fil: Barrillon, P.. Univ Paris-Sud; Francia Fil: Batsch, T.. National Centre for Nuclear Research; Polonia Fil: Bayer, J.. University of Tubinge; Alemania Fil: Bechini, R.. Universita’ di Torino; Italia Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial; España Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare -; Italia Fil: Belov, K.. University of California; Estados Unidos Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos Fil: Bertaina, M.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia Fil: Biermann, P. L.. Karlsruhe Institute of Technology; Alemania Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia Fil: Blaksley, C.. Univ Paris Diderot; Francia Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM),; Suiza Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia Fil: Bogomilov, M.. University of Sofia; Bulgaria Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: The JEM-EUSO Collaboration. |
| description |
The Extreme Universe Space Observatory on board the Japanese Experiment Module of the International Space Station, JEM-EUSO, is being designed tosearch from space ultra-high energy cosmic rays. These are charged particles with energies from a few 10^19 eV to beyond 10^20 eV, at the very end of the known cosmic ray energy spectrum. JEM-EUSO will also search for extreme energy neutrinos, photons, and exotic particles, providing a unique opportunity to explore largely unknown phenomena in our Universe. The mission, principally based on a wide field of view(60 degrees) near-UV telescope with a diameter of ~2.5 m, will monitor the earth?s atmosphere at night, pioneering the observation from space of the ultraviolet tracks (290-430 nm) associated with giant extensive air showers produced by ultra-high energy primaries propagating in the earth?s atmosphere. Observing from an orbital altitude of ~400 km, the mission is expected to reach an instantaneous geometrical aperture of A_geo >= 2 x 10^5 km^2 sr with an estimated duty cycle of ~20%. Sucha geometrical aperture allows unprecedented exposures, significantly larger than can be obtained with ground-based experiments. In this paper we briefly review the history of space-based search for ultra-high energy cosmic rays. We then introduce the special issue of Experimental Astronomy devoted to the various aspects of such a challenging enterprise. We also summarise the activities of the on-going JEM-EUSO program. |
| publishDate |
2015 |
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2015-11 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/18298 Adams, J. H.; Ahmad, S. S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; The JEM-EUSO mission: An introduction; Springer; Experimental Astronomy; 40; 1; 11-2015; 3-17 0922-6435 CONICET Digital CONICET |
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http://hdl.handle.net/11336/18298 |
| identifier_str_mv |
Adams, J. H.; Ahmad, S. S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; The JEM-EUSO mission: An introduction; Springer; Experimental Astronomy; 40; 1; 11-2015; 3-17 0922-6435 CONICET Digital CONICET |
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eng |
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