Fringe pattern of an infrared rotating, rotationally shearing interferometer generated by a star-planet source

Details Fringe pattern of an infrared rotating, rotationally shearing interferometer generated by a star-planet source Fringe pattern of an infrared rotating, rotationally shearing interferometer generated by a star-planet source

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995spie.2553...38s&link_type=abstract

Proc. SPIE Vol. 2553, p. 38-45, Infrared Spaceborne Remote Sensing III, Marija S. Scholl; Bjorn F. Andresen; Eds.

Computer Science

Scientific paper

An infrared, rotating, rotationally-shearing interferometer is proposed for the detection of a planet around a nearby star. The fringe visibility pattern is shown to depend only on the planet parameters. The expression for the interferometric pattern generated by a star and its faint companion detected by a rotationally-shearing interferometer shows that the planet may be detected only if the aperture rotates. Additionally, we show that the shearing interferometer does not suppress the star light--the interferometric pattern is proportional to the star intensity.

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