The Pierre Auger Observatory
- Autores
- Dova, María Teresa
- Año de publicación
- 2003
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- One of the foremost issues in astrophysics today is that of the origin of the ultra high energy cosmic rays. The Pierre Auger Observatory (PAO), currently under construction in the Province of Mendoza, Argentina, is a broadly based international effort to make a high statistic study of the upper-end of the cosmic ray spectrum. The PAO is the first experiment designed to work in a hybrid detection mode. It consists of an array of 1600 particle detectors spread over 3000 km2 and four fluorescence telescopes placed on the boundaries of the surface array. The concept of the experiment as well as the current status and future prospects are presented.
Facultad de Ciencias Exactas - Materia
-
Ciencias Exactas
Pierre Auger Observatory
astrophysics
cosmic rays spectrum
Física - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/78179
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The Pierre Auger ObservatoryDova, María TeresaCiencias ExactasPierre Auger Observatoryastrophysicscosmic rays spectrumFísicaOne of the foremost issues in astrophysics today is that of the origin of the ultra high energy cosmic rays. The Pierre Auger Observatory (PAO), currently under construction in the Province of Mendoza, Argentina, is a broadly based international effort to make a high statistic study of the upper-end of the cosmic ray spectrum. The PAO is the first experiment designed to work in a hybrid detection mode. It consists of an array of 1600 particle detectors spread over 3000 km2 and four fluorescence telescopes placed on the boundaries of the surface array. The concept of the experiment as well as the current status and future prospects are presented.Facultad de Ciencias Exactas2003-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf170-178http://sedici.unlp.edu.ar/handle/10915/78179enginfo:eu-repo/semantics/altIdentifier/issn/0550-3213info:eu-repo/semantics/altIdentifier/doi/10.1016/S0920-5632(03)80373-0info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:44:34Zoai:sedici.unlp.edu.ar:10915/78179Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:44:34.534SEDICI (UNLP) - Universidad Nacional de La Platafalse |
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The Pierre Auger Observatory |
| title |
The Pierre Auger Observatory |
| spellingShingle |
The Pierre Auger Observatory Dova, María Teresa Ciencias Exactas Pierre Auger Observatory astrophysics cosmic rays spectrum Física |
| title_short |
The Pierre Auger Observatory |
| title_full |
The Pierre Auger Observatory |
| title_fullStr |
The Pierre Auger Observatory |
| title_full_unstemmed |
The Pierre Auger Observatory |
| title_sort |
The Pierre Auger Observatory |
| dc.creator.none.fl_str_mv |
Dova, María Teresa |
| author |
Dova, María Teresa |
| author_facet |
Dova, María Teresa |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Ciencias Exactas Pierre Auger Observatory astrophysics cosmic rays spectrum Física |
| topic |
Ciencias Exactas Pierre Auger Observatory astrophysics cosmic rays spectrum Física |
| dc.description.none.fl_txt_mv |
One of the foremost issues in astrophysics today is that of the origin of the ultra high energy cosmic rays. The Pierre Auger Observatory (PAO), currently under construction in the Province of Mendoza, Argentina, is a broadly based international effort to make a high statistic study of the upper-end of the cosmic ray spectrum. The PAO is the first experiment designed to work in a hybrid detection mode. It consists of an array of 1600 particle detectors spread over 3000 km2 and four fluorescence telescopes placed on the boundaries of the surface array. The concept of the experiment as well as the current status and future prospects are presented. Facultad de Ciencias Exactas |
| description |
One of the foremost issues in astrophysics today is that of the origin of the ultra high energy cosmic rays. The Pierre Auger Observatory (PAO), currently under construction in the Province of Mendoza, Argentina, is a broadly based international effort to make a high statistic study of the upper-end of the cosmic ray spectrum. The PAO is the first experiment designed to work in a hybrid detection mode. It consists of an array of 1600 particle detectors spread over 3000 km2 and four fluorescence telescopes placed on the boundaries of the surface array. The concept of the experiment as well as the current status and future prospects are presented. |
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2003 |
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2003-07 |
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eng |
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