Astronomical image reconstruction via space slit aperture telescope

Details Astronomical image reconstruction via space slit aperture telescope Astronomical image reconstruction via space slit aperture telescope

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986spie..643..189m&link_type=abstract

IN: Infrared, adaptive, and synthetic aperture optical systems; Proceedings of the Meetings, Arlington, VA, Apr. 8, 1985 and Orl

Astronomy and Astrophysics

Astronomy

1

Image Reconstruction, Slot Antennas, Speckle Interferometry, Synthetic Apertures, Telescopes, Angular Resolution, Michelson Interferometers, Spaceborne Telescopes

Scientific paper

High angular resolution observations by speckle-interferometric techniques invite the development of ground-based split aperture telescopy (SAT) employing a long, thin pupil. Such devices lie halfway between the Michelson stellar interferometer and the standard telescope with circular aperture. Attention is presently given to a space-based SAT's astronomical image reconstruction. A full coverage of the two-dimensional Fourier plane can be derived through rotation of the SAT around its optical axis. The reconstructed image appears simultaneously in several wavelengths.

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