dc.contributor.author |
Saxena, A. K |
|
dc.contributor.author |
Lancelot, J. P |
|
dc.contributor.author |
Samson, J. P |
|
dc.date.accessioned |
2011-09-26T10:59:41Z |
|
dc.date.available |
2011-09-26T10:59:41Z |
|
dc.date.issued |
1993-12 |
|
dc.identifier.citation |
Proceedings of SPIE; Vol. 2003, pp. 88-97 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/5580 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
India is planning to build a large Optical/Infrared Telescope of 4 to 5 M in size. This telescope will adopt most of the features of the New Technology Telescope including active and adoptive optics corrections for achieving improved image quality. Keeping this in view a prototype active optics system for a 27 inch thin mirror is being developed at Indian Institute of Astrophysics. A new digital polarization shearing interferometer will be used for wavefront sensing. The paper describes in detail the procedure for wavefront sensing and the approach for the active correction. |
en |
dc.language.iso |
en |
en |
dc.publisher |
SPIE-The International Society for Optical Engineering |
en |
dc.relation.ispartofseries |
Proceedings of SPIE; Vol. 2003 |
|
dc.relation.uri |
http://dx.doi.org/10.1117/12.165442 |
en |
dc.rights |
© SPIE-The International Society for Optical Engineering |
en |
dc.title |
Development of an active-optics system for 27-inch thin mirror |
en |
dc.type |
Article |
en |