Author: Criscuoli S. Moro D. Bonet J. Márquez I.
Publisher: Springer Publishing Company
ISSN: 0038-0938
Source: Solar Physics, Vol.228, Iss.1-2, 2005-05, pp. : 177-189
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Phase diversity techniques are robust post-processing tools for image enhancement and correction of telescopic and atmospheric induced aberrations. We present results obtained applying the Partitioned Phase-Diverse Speckle (PPDS) technique to images acquired at THEMIS. We also present an image quality estimator based on image power spectrum content we developed in order to automatically evaluate the results of large amount of data.
Related content
Themis, BBSO, MDI and trace observations of a filament eruption
By Contarino L. Romano P. Yurchyshyn V.B. Zuccarello F.
Solar Physics, Vol. 216, Iss. 1-2, 2003-09 ,pp. :
-ATLAS: first data release of the Science Demonstration Phase source catalogues
By Rigby E. E. Maddox S. J. Dunne L. Negrello M. Smith D. J. B. González-Nuevo J. Herranz D. López-Caniego M. Auld R. Buttiglione S. Baes M. Cava A. Cooray A. Clements D. L. Dariush A. De Zotti G. Dye S. Eales S. Frayer D. Fritz J. Hopwood R. Ibar E. Ivison R. J. Jarvis M. Panuzzo P. Pascale E. Pohlen M. Rodighiero G. Serjeant S. Temi P. Thompson M. A.
Monthly Notices of the Royal Astronomical Society, Vol. 415, Iss. 3, 2011-08 ,pp. :