| dc.contributor.author | Yeswanth, L | |
| dc.date.accessioned | 2013-05-03T16:59:14Z | |
| dc.date.available | 2013-05-03T16:59:14Z | |
| dc.date.issued | 2013-05-03 | |
| dc.identifier.citation | IIA Technical Report Series No. 12 | en | 
| dc.identifier.uri | http://hdl.handle.net/2248/6052 | |
| dc.description | Open Access | en | 
| dc.description.abstract | A rotational shearing interferometer is a modification of the Michelson’s interferometer to obtain the spatial coherence of the light waves. It is mainly used for obtaining diffraction limited images of astronomical objects; through the turbulent atmosphere of the Earth. The fabrication of a solid rotational shearing interferometer with a fixed rotational shear of 180º is described. Also the use of the interferometer, for testing the aberrations of a telescope is described. | en | 
| dc.language.iso | en | en | 
| dc.publisher | Indian Institute of Astrophysics | en | 
| dc.relation.ispartofseries | IIA-TRS-1213 | |
| dc.rights | © Indian Institute of Astrophysics | en | 
| dc.subject | Interferometer | en | 
| dc.subject | Michelson Interferometer | en | 
| dc.subject | Fizeau Interferogram | en | 
| dc.subject | Path Length Equalization | en | 
| dc.title | Rotational shearing interferomater | en | 
| dc.type | Technical Report | en |