Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5206
Full metadata record
DC FieldValueLanguage
dc.contributor.authorKundu, M.R.-
dc.contributor.authorSarma, N.V.G.-
dc.contributor.authorGerard, E.-
dc.date.accessioned2012-08-06T09:48:18Z-
dc.date.available2012-08-06T09:48:18Z-
dc.date.issued1976-
dc.identifier.citationAstrophysical Letters, 1976, Vol.18, p41-47en
dc.identifier.urihttp://hdl.handle.net/2289/5206-
dc.descriptionRestricted Access.en
dc.description.abstractDuring the 1974 fly-by of Jupiter by the Pioneer 11 spacecraft, radio observations were carried out daily at 327 and 1410 MHz for a period of 60 days centered on December 3, 1974, the day of closest approach to Jupiter. The 1410-MHz data reveal two significant short-term variations in the Jovian radio emission; the largest one is probably present also at 327 MHz although Faraday rotation in earth's ionosphere could have affected the data. The two radio bursts appear to be correlated with two long-duration electron bursts observed in the energy ranges from 2 to 7 and 6 to 30 MeV.en
dc.language.isoenen
dc.publisherTaylor & Francisen
dc.relation.urihttp://adsabs.harvard.edu/abs/1976ApL....18...41Ken
dc.rights1976 Taylor & Francisen
dc.subjectjupiter (planet)en
dc.subjectmicrowave emissionen
dc.subjectplanetary radiationen
dc.subjectradiant flux densityen
dc.subjectradio burstsen
dc.subjectradio observationen
dc.subjectelectron flux densityen
dc.subjectflyby missionsen
dc.subjectpioneer 11 space probeen
dc.titleObservations of Jupiter's radio emission at 327 MHz and 1410 MHz during the Pioneer 11 fly-byen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1976_Astrophysical Letters_p18_p41.pdf
  Restricted Access
Restricted Access313.91 kBAdobe PDFView/Open Request a copy


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.