Translator Disclaimer
Paper
21 February 2003 Optical delay for OHANA
Author Affiliations +
Abstract
The OHANA interferometric array will be implemented by linking existing Mauna Kea telescopes with optical fiber. No new facility construction on Mauna Kea is required or planned for OHANA. Fibers will be run through existing cableways. The maximum potential baselines are approximately 800 meters in length. Interferometric operation with good UV coverage will require within the instrument variable optical delay approaching 400 meters. It will be necessary to provide this length of delay within a modest amount of existing laboratory space. An obvious approach is the use of multiple passes within a short delay line space. This poster investigates possible multi-pass implementations and related issues of efficiency, cost, wavefront quality and diffraction. The required optical delay can be provided at reasonable efficiency and moderate cost. The simpler optical delay for OHANA Phase II, already under construction, is described.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephen T. Ridgway, Guy S. Perrin, Julien Woillez, Jean Guerin, and Olivier Lai "Optical delay for OHANA", Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); https://doi.org/10.1117/12.459141
PROCEEDINGS
7 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Self-Referencing Wavefront Sensor
Proceedings of SPIE (August 01 1983)
GRAVITY: metrology
Proceedings of SPIE (September 12 2012)
Visible nulling interferometer
Proceedings of SPIE (October 12 2004)

Back to Top