Low frequency imaging and the non-isoplanatic atmosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4238

Full metadata record

DC Field	Value	Language
dc.contributor.author	Subrahmanya, C.R.	-
dc.date.accessioned	2011-12-15T06:05:30Z	-
dc.date.available	2011-12-15T06:05:30Z	-
dc.date.issued	1991	-
dc.identifier.citation	Radio interferometry: Theory, techniques, and applications; Proceedings of the 131st IAU Colloquium, Socorro, NM, Oct. 8-12, 1990	en
dc.identifier.uri	http://hdl.handle.net/2289/4238	-
dc.description	Restricted Access.	en
dc.description.abstract	A 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.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1991ASPC...19..218S	en
dc.rights	1991 Astronomical Society of the Pacific	en
dc.subject	Atmospheric Effects	en
dc.subject	Instrument Compensation	en
dc.subject	Ionospheric Propagation	en
dc.subject	Radio Telescopes	en
dc.subject	Sky Brightness	en
dc.subject	Brightness Distribution	en
dc.subject	Field Of View	en
dc.subject	Fourier Transformation	en
dc.subject	Low Frequencies	en
dc.subject	Very Large Array (Vla)	en
dc.title	Low frequency imaging and the non-isoplanatic atmosphere	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

Files in This Item:

File	Description	Size	Format
1991_ASPC_19_p218.pdf Restricted Access	Restricted access	100.46 kB	Adobe PDF	View/Open Request a copy