Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array
Descripción del Articulo
Jupiter radiates electromagnetic radiation in a broad spectrum. We are concerned here with the center part, usually referred as the decimetric radiation, a relatively flat part of the spectrum going from about 39.5 MHz merging into the thermal radiation at about 4GHz. The source of this radiation is...
| Autores: | , |
|---|---|
| Formato: | objeto de conferencia |
| Fecha de Publicación: | 2013 |
| Institución: | Instituto Geofísico del Perú |
| Repositorio: | IGP-Institucional |
| Lenguaje: | inglés |
| OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/2134 |
| Enlace del recurso: | http://hdl.handle.net/20.500.12816/2134 |
| Nivel de acceso: | acceso abierto |
| Materia: | Radiation Magnetic field Electromagnetism Space science http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.05.00 |
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| dc.title.es_ES.fl_str_mv |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| title |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| spellingShingle |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array Woodman Pollitt, Ronald Francisco Radiation Magnetic field Electromagnetism Space science http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.05.00 |
| title_short |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| title_full |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| title_fullStr |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| title_full_unstemmed |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| title_sort |
Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array |
| author |
Woodman Pollitt, Ronald Francisco |
| author_facet |
Woodman Pollitt, Ronald Francisco Villanueva R., Fernando |
| author_role |
author |
| author2 |
Villanueva R., Fernando |
| author2_role |
author |
| dc.contributor.author.fl_str_mv |
Woodman Pollitt, Ronald Francisco Villanueva R., Fernando |
| dc.subject.es_ES.fl_str_mv |
Radiation Magnetic field Electromagnetism Space science |
| topic |
Radiation Magnetic field Electromagnetism Space science http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.05.00 |
| dc.subject.ocde.es_ES.fl_str_mv |
http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.05.00 |
| description |
Jupiter radiates electromagnetic radiation in a broad spectrum. We are concerned here with the center part, usually referred as the decimetric radiation, a relatively flat part of the spectrum going from about 39.5 MHz merging into the thermal radiation at about 4GHz. The source of this radiation is synchrotron radiation emitted by energetic electrons, trapped in Jupiter's Van Allen radiation belt, gyrating around its magnetic field. The flux density of this radiation has been measured at many frequencies, the lowest being at around 80 MHZ. |
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2013 |
| dc.date.accessioned.none.fl_str_mv |
2018-07-31T17:34:08Z |
| dc.date.available.none.fl_str_mv |
2018-07-31T17:34:08Z |
| dc.date.issued.fl_str_mv |
2013-05 |
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info:eu-repo/semantics/conferenceObject |
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http://hdl.handle.net/20.500.12816/2134 |
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http://hdl.handle.net/20.500.12816/2134 |
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eng |
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eng |
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https://creativecommons.org/licences/by/4.0/ |
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Woodman Pollitt, Ronald FranciscoVillanueva R., Fernando2018-07-31T17:34:08Z2018-07-31T17:34:08Z2013-05http://hdl.handle.net/20.500.12816/2134Jupiter radiates electromagnetic radiation in a broad spectrum. We are concerned here with the center part, usually referred as the decimetric radiation, a relatively flat part of the spectrum going from about 39.5 MHz merging into the thermal radiation at about 4GHz. The source of this radiation is synchrotron radiation emitted by energetic electrons, trapped in Jupiter's Van Allen radiation belt, gyrating around its magnetic field. The flux density of this radiation has been measured at many frequencies, the lowest being at around 80 MHZ.application/pdfengInstituto Geofísico del Perúinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/RadiationMagnetic fieldElectromagnetismSpace sciencehttp://purl.org/pe-repo/ocde/ford#1.05.01http://purl.org/pe-repo/ocde/ford#1.05.00Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca arrayinfo:eu-repo/semantics/conferenceObjectreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-2-0-1376318876.pdfIGP-1-2-0-1376318876.pdfapplication/pdf1989949https://repositorio.igp.gob.pe/bitstreams/ef5adea5-87d9-4c17-9437-466fccc78b87/downloadcb00641b7f7cb914e12e7eb4a19b340dMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/4db563b2-ce87-4bd5-aedb-fd7db4f8e157/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILIGP-1-2-0-1376318876.pdf.jpgIGP-1-2-0-1376318876.pdf.jpgIM Thumbnailimage/jpeg123578https://repositorio.igp.gob.pe/bitstreams/d51428ae-c011-470c-886c-7c3ab581a953/download342a0c3a704cff98253f8d42a86cacebMD53TEXTIGP-1-2-0-1376318876.pdf.txtIGP-1-2-0-1376318876.pdf.txtExtracted texttext/plain6692https://repositorio.igp.gob.pe/bitstreams/8e8f0fbb-1609-4774-ac31-f799aafeac31/download6adeb71f861bec85fb47e38a02e966d4MD5420.500.12816/2134oai:repositorio.igp.gob.pe:20.500.12816/21342021-03-10 12:01:46.652https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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 |
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La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).