Jupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca array

dc.contributor.authorWoodman Pollitt, Ronald Francisco
dc.contributor.authorVillanueva R., Fernando
dc.date.accessioned2018-07-31T17:34:08Z
dc.date.available2018-07-31T17:34:08Z
dc.date.issued2013-05
dc.description.abstractJupiter 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.es_ES
dc.formatapplication/pdfes_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/2134
dc.language.isoenges_ES
dc.publisherInstituto Geofísico del Perúes_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttps://creativecommons.org/licences/by/4.0/es_ES
dc.subjectRadiationes_ES
dc.subjectMagnetic fieldes_ES
dc.subjectElectromagnetismes_ES
dc.subjectSpace sciencees_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.00es_ES
dc.titleJupiter's synchrotron radiation at 50 MHZ measured by the large 50MHZ Jicamarca arrayes_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES

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