Towards an ESA strategy for optical interferometry outside the atmosphere

Details Towards an ESA strategy for optical interferometry outside the atmosphere Towards an ESA strategy for optical interferometry outside the atmosphere

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991spie.1494..344n&link_type=abstract

IN: Space astronomical telescopes and instruments; Proceedings of the Meeting, Orlando, FL, Apr. 1-4, 1991 (A92-45151 19-89). Be

Mathematics

Logic

European Space Agency, Faint Objects, Imaging Techniques, Spatial Resolution, Very Long Base Interferometry, Functional Design Specifications, Mission Planning, Technological Forecasting

Scientific paper

The conclusions, recommendations, and target design parameters for a 100-m class optical space interferometer that has been recommended by a study group of the ESA for launching around the year 2005 are summarized. The desirability of an interferometer on the moon, covering the entire wavelength range from UV to sub-mm, with a space interferometer as a possible intermediate step, is considered.

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