A new approach to stellar image correction for atmospherically degraded images

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4892

Full metadata record

DC Field	Value	Language
dc.contributor.author	Chinnappan, V	-
dc.date.accessioned	2009-11-04T17:16:40Z	-
dc.date.available	2009-11-04T17:16:40Z	-
dc.date.issued	2006-08	-
dc.identifier.citation	Ph.D. Thesis, Bangalore University, Bangalore	en
dc.identifier.uri	http://hdl.handle.net/2248/4892	-
dc.description	Thesis Advisor`s Dr. A. K. Saxena & Dr. A. Sreenivasan	-
dc.description.abstract	Atmospheric turbulence is the main cause of image degradation and poor resolution at the focal plane of a perfectly made optical telescope. It is necessary to make corrective measures to improve the optical wave-front, thus, get improved resolution from the telescopes. This research work is an effort to understand the degradations caused by atmospheric turbulence, build an appropriate wave-front sensor to measure the errors in the wave-front and correct the wave-front in real time for our 2.34 M Vainu Bappu Telescope (VBT) at Vainu Bappu Observatory, Kavalur, keeping the cost as one of the main factors.	en
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.subject	Astronomical Images	en
dc.subject	Speckle Interferometer	en
dc.subject	CCDs	en
dc.subject	CMOS Imagers	en
dc.subject	Atmospheric Turbulence	en
dc.subject	Image Degradation	en
dc.subject	Optical Telescope	en
dc.subject	Optical Wave-Front	en
dc.subject	Wave-Front Sensor	en
dc.title	A new approach to stellar image correction for atmospherically degraded images	en
dc.type	Thesis	en
Appears in Collections:	IIAP Ph.D.Theses

Files in This Item:

File	Description	Size	Format
A new approach to stellar image	Open Access	4.38 MB	Adobe PDF	View/Open

DSpace JSPUI