dc.contributor.author |
Vyas, A |
|
dc.contributor.author |
Roopashree, M. B |
|
dc.contributor.author |
Prasad, B. R |
|
dc.date.accessioned |
2011-08-02T10:30:45Z |
|
dc.date.available |
2011-08-02T10:30:45Z |
|
dc.date.issued |
2011-07 |
|
dc.identifier.citation |
Adaptive Optics: Methods, Analysis and Applications, OSA Technical Digest, ATuA4 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/5531 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
Wavefront reconstruction accuracy strongly depends on the way the wavefront distortion points match the wavefront sensing locations. A multi-dither sensor largely improves the wavefront reconstruction accuracy in large telescope AO systems. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Optical Society of America |
en |
dc.relation.uri |
http://www.opticsinfobase.org/abstract.cfm?URI=AO-2011-ATuA4 |
en |
dc.rights |
© Optical Society of America |
en |
dc.title |
Multi-dither Shack Hartmann sensor for large telescopes: A numerical performance evaluation |
en |
dc.type |
Article |
en |