| 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 |