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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4139
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dc.contributor.authorBhardwaj, A.-
dc.contributor.authorIshwara-Chandra, C.H.-
dc.contributor.authorUdaya Shankar, N.-
dc.contributor.authorMisawa, H.-
dc.contributor.authorImai, K.-
dc.contributor.authorMiyoshi, Y.-
dc.contributor.authorTsuchiya, F.-
dc.contributor.authorKondo, T.-
dc.contributor.authorMorioka, A.-
dc.date.accessioned2011-08-24T05:24:41Z-
dc.date.available2011-08-24T05:24:41Z-
dc.date.issued2009-09-
dc.identifier.citationASP Conference Series, 2009, Vol.407, p369en
dc.identifier.urihttp://hdl.handle.net/2289/4139-
dc.descriptionRestricted Access. Proceedings of the conference held 8-12 December 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India. Edited by D. J. Saikia, D. A. Green, Y. Gupta, and T. Venturi. San Francisco: Astronomical Society of the Pacific.en
dc.description.abstractThe non-thermal decimeteric radio emission from Jupiter is dominated by synchrotron emission originating from high-energy electrons trapped in Jupiter's inner radiation belt (<5 Jovian radii). We observed Jupiter during February 24 -- March 3, 2003 with the GMRT to study its day-to-day variability. Each day's observations lasted for ˜10 hours (the rotation period of Jupiter). These observations suggest a correlation between the Jupiter radio flux density and the solar radio flux density at 10.7 cm (which is a proxy for solar EUV flux). Short-term variability (flux density change by ~20%) seen at 610 MHz in 6-day observation seems to be due to enhanced solar EUV activity. This is the first result reporting the short-term variability in Jupiter synchrotron radiation at 610 MHz. The results have implications for Jovian radiation belt dynamics and upper atmospheric processes.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/2009ASPC..407..369Ben
dc.rights2009 Astronomical Society of the Pacific.en
dc.titleGMRT observations of jupiter's synchrotron radio emission at 610 MHzen
dc.typeArticleen
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