1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/980
Full metadata record
DC FieldValueLanguage
dc.contributor.authorGopala Rao, U. V-
dc.date.accessioned2006-04-19T11:06:06Z-
dc.date.available2006-04-19T11:06:06Z-
dc.date.issued1967-
dc.identifier.citationProceedings of the Indian Academy of Sciences, Vol. 65, No. 2, Sec. A, pp. 112-119en
dc.identifier.urihttp://hdl.handle.net/2248/980-
dc.description.abstractAn analysis of the influence of the satellite Io on Jupiter`s decametric radio emission was carried out utilizing observations recorded at Kodaikanal and Boulder. The influence is found to be complicated and is different at the three sources. It is suggested that the Io related emission can be due to Cerenkov radiation by fast electrons acting as a well-separated streamen
dc.format.extent1405767 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian National Science Academyen
dc.subjectJupiteren
dc.subjectSatellite Ioen
dc.titleInfluence of the satellite Io on Jupiter`s Decametric radio emissionen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
RAO.pdf1.37 MBAdobe PDFView/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.