Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/4238
Title: | Low frequency imaging and the non-isoplanatic atmosphere |
Authors: | Subrahmanya, C.R. |
Keywords: | Atmospheric Effects Instrument Compensation Ionospheric Propagation Radio Telescopes Sky Brightness Brightness Distribution Field Of View Fourier Transformation Low Frequencies Very Large Array (Vla) |
Issue Date: | 1991 |
Publisher: | Astronomical Society of the Pacific |
Citation: | Radio interferometry: Theory, techniques, and applications; Proceedings of the 131st IAU Colloquium, Socorro, NM, Oct. 8-12, 1990 |
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. |
Description: | Restricted Access. |
URI: | http://hdl.handle.net/2289/4238 |
Alternative Location: | http://adsabs.harvard.edu/abs/1991ASPC...19..218S |
Copyright: | 1991 Astronomical Society of the Pacific |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1991_ASPC_19_p218.pdf Restricted Access | Restricted access | 100.46 kB | Adobe PDF | View/Open Request a copy |
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