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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2561
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dc.contributor.authorCornwell, T.J.-
dc.contributor.authorAnantharamaiah, K.R.-
dc.contributor.authorNarayan, R.-
dc.date.accessioned2007-06-04T07:59:10Z-
dc.date.available2007-06-04T07:59:10Z-
dc.date.issued1990-
dc.identifier.citationURSI/IAU Symposium on Radio Astronomical Seeing, Beijing, People's Republic of China, May 15-19, 1989, Proceedings. Beijing/Oxford, International Academic Publishers/Pergamon Press, 1990, p239-242en
dc.identifier.urihttp://hdl.handle.net/2289/2561-
dc.descriptionRestricted Access.en
dc.description.abstractAlthough scattering is widespread in radio-astronomy, there has been little investigation of the 'speckle' phenomenon found in optical scattering. Using the VLA, the existence of speckles have been demonstrated in interplanetary scintillation scattering disks when observed with high temporal and angular resolution. Such speckles lead to a number of conceptual and practical difficulties in schemes for the correction of radio-astronomical seeing. These various aspects of radio-speckles are discussed and some examples drawn from the VLA IPS observations are shown.en
dc.format.extent214632 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherPergamon Pressen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1990ursi.symp..239Cen
dc.rights1990 Pergamon Pressen
dc.subjectINTERPLANETARY MEDIUMen
dc.subjectLIGHT SCATTERINGen
dc.subjectRADIO ASTRONOMYen
dc.subjectSCINTILLATIONen
dc.subjectSPECKLE PATTERNSen
dc.subjectVERY LARGE ARRAY (VLA)en
dc.subjectPOINT SPREAD FUNCTIONSen
dc.subjectRADIO TELESCOPESen
dc.subjectSEEING (ASTRONOMY)en
dc.subjectSIGNAL TO NOISE RATIOSen
dc.subjectSOLAR WINDen
dc.titleSpeckle phenomena in inter-planetary scintillationen
dc.typeArticleen
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