dc.contributor.author |
Shevgaonkar, R. K |
|
dc.date.accessioned |
2008-09-23T14:25:12Z |
|
dc.date.available |
2008-09-23T14:25:12Z |
|
dc.date.issued |
1987-04 |
|
dc.identifier.citation |
Astronomy And Astrophysics, Vol. 176, No. 1, No. 159 -170 |
en |
dc.identifier.issn |
0004-6361 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3837 |
|
dc.description.abstract |
A simple maximum entropy method algorithm for deconvolving polarized images obtained from synthesis observations has been described here. A general purpose Fortran program is also developed. it demonstrated that although the a priori positivity conditions is imposed on the total intensity image only, the polarized component images also get improved remarkably. |
en |
dc.language.iso |
en |
en |
dc.publisher |
The European Southern Observatory |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1987A%26A...176..159S |
en |
dc.subject |
Image processing |
en |
dc.subject |
maximum entropy |
en |
dc.subject |
Radio astronomy |
en |
dc.subject |
Stokes parameters |
en |
dc.subject |
Polarized images |
en |
dc.title |
Maximum Entropy Method for Polarized Images |
en |
dc.type |
Article |
en |