Seeing timescales for large-aperture optical/infrared interferometers from simulations

Details Seeing timescales for large-aperture optical/infrared interferometers from simulations Seeing timescales for large-aperture optical/infrared interferometers from simulations

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004spie.5491.1240t&link_type=abstract

New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The Intern

Computer Science

2

Scientific paper

Numerical simulations of interferometers with spatial filters and large apertures are presented. These simulations are particularly aimed at measuring the fringe (or OPD) motion caused by atmospherically induced wavefront corrugations (high order Zernike modes) across the telescope apertures. This component of the fringe motion results from the coupling in a spatial filter of high-order Zernike modes to the fringe motion. The Piston Mode component is found to be an inadequate approximation to the OPD in an interferometer with large apertures, spatial filters and tip-tilt correction. The fringe motion at

Affiliated with

Also associated with

No associations

Rating

Seeing timescales for large-aperture optical/infrared interferometers from simulations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Seeing timescales for large-aperture optical/infrared interferometers from simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Seeing timescales for large-aperture optical/infrared interferometers from simulations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1810446