RRI Banner

Low frequency imaging and the non-isoplanatic atmosphere

Simple item page
dc.contributor.authorSubrahmanya, C.R.
dc.date.accessioned2011-12-15T06:05:30Z
dc.date.available2011-12-15T06:05:30Z
dc.date.issued1991
dc.descriptionRestricted Access.en
dc.description.abstractA method for image reconstruction in radio telescopes using self-calibration is presented for the case of a nonisoplanatic atmosphere. While computation intensive, most of the computations consist of calculating the model visibilities and the solution of nonlinear equations, and the method is suitable for implementation on parallel processors.en
dc.identifier.citationRadio interferometry: Theory, techniques, and applications; Proceedings of the 131st IAU Colloquium, Socorro, NM, Oct. 8-12, 1990en
dc.identifier.urihttp://hdl.handle.net/2289/4238
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/1991ASPC...19..218Sen
dc.rights1991 Astronomical Society of the Pacificen
dc.subjectAtmospheric Effectsen
dc.subjectInstrument Compensationen
dc.subjectIonospheric Propagationen
dc.subjectRadio Telescopesen
dc.subjectSky Brightnessen
dc.subjectBrightness Distributionen
dc.subjectField Of Viewen
dc.subjectFourier Transformationen
dc.subjectLow Frequenciesen
dc.subjectVery Large Array (Vla)en
dc.titleLow frequency imaging and the non-isoplanatic atmosphereen
dc.typeArticleen

Files

Collections

Research Papers (A&A)