1 May 1991 High accuracy image centroiding with a moving Ronchi ruling
George N. Lawrence, Chunsheng Huang, Eugene H. Levy, Robert S. McMillan
Author Affiliations +
Abstract
A moving Ronchi ruling at the focal plane of a telescope has been employed to measure the relative motions of stars with great accuracy. The method has long-term stability and exceptional linearity over a relatively large field-of-view. This measurement technique may prove useful in other applications where such capabilities are required. This paper employs Fourier optics to describe the operation of the device, explore performance at very long and very short periods, and consider ruling profiles and other means of optimizing performance.
George N. Lawrence, Chunsheng Huang, Eugene H. Levy, and Robert S. McMillan "High accuracy image centroiding with a moving Ronchi ruling," Optical Engineering 30(5), (1 May 1991). https://doi.org/10.1117/12.55840
Published: 1 May 1991
Lens.org Logo
CITATIONS
Cited by 5 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Signal to noise ratio

Ronchi rulings

Phase transfer function

Sensors

Monochromatic aberrations

Stars

Modulation transfer functions

RELATED CONTENT

Improvements in OTF measurement technique
Proceedings of SPIE (January 01 1993)
Portable intensity interferometry
Proceedings of SPIE (September 12 2012)
Compact diode laser homodyne vibrometers
Proceedings of SPIE (April 29 2010)
Status of PRIMA for the VLTI or the quest for...
Proceedings of SPIE (July 21 2010)
A status update of the VLTI control system
Proceedings of SPIE (September 15 2004)

Back to Top