JEM-EUSO: Meteor and nuclearite observations

Autores
Bertaina, M.; Cellino, A.; Ronga, F.; Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; Andreev, V.; Anzalone, A.; Arai, Y.; Asano, K.; Ave Pernas, M.; Baragatti, P.; Barrillon, P.; Batsch, T.; Bayer, J.; Bechini, R.; Belenguer, T.; Bellotti, R.; Belov, K.; Berlind, A. A.; Biermann, P. L.; Biktemerova, S.; Blaksley, C.; Blanc, N.; Blecki, J.; Blin Bondil, S.; Supanitsky, Alberto Daniel; The JEM-EUSO Collaboration
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Meteor and fireball observations are key to the derivation of both the inventory and physical characterization of small solar system bodies orbiting in the vicinity of the Earth. For several decades, observation of these phenomena has only been possible via ground-based instruments. The proposed JEM-EUSO mission has the potential to become the first operational space-based platform to share this capability. In comparison to the observation of extremely energetic cosmic ray events, which is the primary objective of JEM-EUSO, meteor phenomena are very slow, since their typical speeds are of the order of a few tens of km/sec (whereas cosmic rays travel at light speed). The observing strategy developed to detect meteors may also be applied to the detection of nuclearites, which have higher velocities, a wider range of possible trajectories, but move well below the speed of light and can therefore be considered as slow events for JEM-EUSO. The possible detection of nuclearites greatly enhances the scientific rationale behind the JEM-EUSO mission.
Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Cellino, A.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Ronga, F.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, 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 Alcalá; 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 Tubingen; Alemania
Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA; 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: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); 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: 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
Meteors
Nuclearites
Jem-Euso
Space Detectors
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/18312
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/18312
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling JEM-EUSO: Meteor and nuclearite observationsBertaina, M.Cellino, A.Ronga, F.Adams, J. H.Ahmad, S.Albert, J. N.Allard, D.Anchordoqui, L.Andreev, V.Anzalone, A.Arai, Y.Asano, K.Ave Pernas, M.Baragatti, P.Barrillon, P.Batsch, T.Bayer, J.Bechini, R.Belenguer, T.Bellotti, R.Belov, K.Berlind, A. A.Biermann, P. L.Biktemerova, S.Blaksley, C.Blanc, N.Blecki, J.Blin Bondil, S.Supanitsky, Alberto DanielThe JEM-EUSO CollaborationMeteorsNuclearitesJem-EusoSpace Detectorshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Meteor and fireball observations are key to the derivation of both the inventory and physical characterization of small solar system bodies orbiting in the vicinity of the Earth. For several decades, observation of these phenomena has only been possible via ground-based instruments. The proposed JEM-EUSO mission has the potential to become the first operational space-based platform to share this capability. In comparison to the observation of extremely energetic cosmic ray events, which is the primary objective of JEM-EUSO, meteor phenomena are very slow, since their typical speeds are of the order of a few tens of km/sec (whereas cosmic rays travel at light speed). The observing strategy developed to detect meteors may also be applied to the detection of nuclearites, which have higher velocities, a wider range of possible trajectories, but move well below the speed of light and can therefore be considered as slow events for JEM-EUSO. The possible detection of nuclearites greatly enhances the scientific rationale behind the JEM-EUSO mission.Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Cellino, A.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Ronga, F.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Adams, J. H.. University of Alabama in Huntsville; Estados UnidosFil: Ahmad, 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 Alcalá; 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 Tubingen; AlemaniaFil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA; EspañaFil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Belov, K.. University of California; Estados UnidosFil: Berlind, A. A.. Vanderbilt University; Estados UnidosFil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); 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: 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/11336/18312Bertaina, M.; Cellino, A.; Ronga, F.; Adams, J. H.; Ahmad, S.; et al.; JEM-EUSO: Meteor and nuclearite observations; Springer; Experimental Astronomy; 40; 1; 11-2015; 253-2790922-6435CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-014-9375-4info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs10686-014-9375-4info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:16:43Zoai:ri.conicet.gov.ar:11336/18312instacron: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:34982025-10-22 12:16:43.343CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv JEM-EUSO: Meteor and nuclearite observations
title JEM-EUSO: Meteor and nuclearite observations
spellingShingle JEM-EUSO: Meteor and nuclearite observations
Bertaina, M.
Meteors
Nuclearites
Jem-Euso
Space Detectors
title_short JEM-EUSO: Meteor and nuclearite observations
title_full JEM-EUSO: Meteor and nuclearite observations
title_fullStr JEM-EUSO: Meteor and nuclearite observations
title_full_unstemmed JEM-EUSO: Meteor and nuclearite observations
title_sort JEM-EUSO: Meteor and nuclearite observations
dc.creator.none.fl_str_mv Bertaina, M.
Cellino, A.
Ronga, F.
Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Baragatti, P.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin Bondil, S.
Supanitsky, Alberto Daniel
The JEM-EUSO Collaboration
author Bertaina, M.
author_facet Bertaina, M.
Cellino, A.
Ronga, F.
Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Baragatti, P.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin Bondil, S.
Supanitsky, Alberto Daniel
The JEM-EUSO Collaboration
author_role author
author2 Cellino, A.
Ronga, F.
Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Baragatti, P.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin Bondil, S.
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
dc.subject.none.fl_str_mv Meteors
Nuclearites
Jem-Euso
Space Detectors
topic Meteors
Nuclearites
Jem-Euso
Space Detectors
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Meteor and fireball observations are key to the derivation of both the inventory and physical characterization of small solar system bodies orbiting in the vicinity of the Earth. For several decades, observation of these phenomena has only been possible via ground-based instruments. The proposed JEM-EUSO mission has the potential to become the first operational space-based platform to share this capability. In comparison to the observation of extremely energetic cosmic ray events, which is the primary objective of JEM-EUSO, meteor phenomena are very slow, since their typical speeds are of the order of a few tens of km/sec (whereas cosmic rays travel at light speed). The observing strategy developed to detect meteors may also be applied to the detection of nuclearites, which have higher velocities, a wider range of possible trajectories, but move well below the speed of light and can therefore be considered as slow events for JEM-EUSO. The possible detection of nuclearites greatly enhances the scientific rationale behind the JEM-EUSO mission.
Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Cellino, A.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Ronga, F.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, 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 Alcalá; 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 Tubingen; Alemania
Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA; 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: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); 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: 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 Meteor and fireball observations are key to the derivation of both the inventory and physical characterization of small solar system bodies orbiting in the vicinity of the Earth. For several decades, observation of these phenomena has only been possible via ground-based instruments. The proposed JEM-EUSO mission has the potential to become the first operational space-based platform to share this capability. In comparison to the observation of extremely energetic cosmic ray events, which is the primary objective of JEM-EUSO, meteor phenomena are very slow, since their typical speeds are of the order of a few tens of km/sec (whereas cosmic rays travel at light speed). The observing strategy developed to detect meteors may also be applied to the detection of nuclearites, which have higher velocities, a wider range of possible trajectories, but move well below the speed of light and can therefore be considered as slow events for JEM-EUSO. The possible detection of nuclearites greatly enhances the scientific rationale behind the JEM-EUSO mission.
publishDate 2015
dc.date.none.fl_str_mv 2015-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/18312
Bertaina, M.; Cellino, A.; Ronga, F.; Adams, J. H.; Ahmad, S.; et al.; JEM-EUSO: Meteor and nuclearite observations; Springer; Experimental Astronomy; 40; 1; 11-2015; 253-279
0922-6435
CONICET Digital
CONICET
url http://hdl.handle.net/11336/18312
identifier_str_mv Bertaina, M.; Cellino, A.; Ronga, F.; Adams, J. H.; Ahmad, S.; et al.; JEM-EUSO: Meteor and nuclearite observations; Springer; Experimental Astronomy; 40; 1; 11-2015; 253-279
0922-6435
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-014-9375-4
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs10686-014-9375-4
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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