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An Adaptive Steerable Imaging Array

Published online by Cambridge University Press:  19 July 2016

E.K. Hege ,
J.R.P. Angel ,
A.D. Gleckler ,
K.P. Pflibsen  and
B.L. Ulich
E.K. Hege
Affiliation:
Steward Observatory, University of Arizona, Tucson AZ 85721, USA
J.R.P. Angel
Affiliation:
Steward Observatory, University of Arizona, Tucson AZ 85721, USA
A.D. Gleckler
Affiliation:
Kaman Aerospace Corporation, 3480 East Britannia, Tucson AZ 85706-5007, USA
K.P. Pflibsen
Affiliation:
Kaman Aerospace Corporation, 3480 East Britannia, Tucson AZ 85706-5007, USA
B.L. Ulich
Affiliation:
Kaman Aerospace Corporation, 3480 East Britannia, Tucson AZ 85706-5007, USA

Abstract

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We propose an optimized design for the redeployment of the Multiple Mirror Telescope (MMT) primary optics as a 25 m Adaptive Steerable Imaging Array (ASIA) providing direct focal plane image formation. The design incorporates concepts of active telescope alignment and adaptive optics proven in the existing MMT. Basing predictions on contemporary radio telescope mount technology, 45 m to 100 m optical baselines may be practical.

Keywords

Telescope designHigh angular resolutionAdaptive optics
Type
Optical and Infrared Interferometers and Arrays
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 167 - 170
Copyright
Copyright © Kluwer 1994 

References

Angel, J.R.P., Wizinowich, P.L., Lloyd-Hart, M. and Sandler, D.: 1990, Nature 348, 221 CrossRefGoogle Scholar
Cornwell, T.: 1988, IEEE Trans. A. P. 36, 1165–1167 CrossRefGoogle Scholar
Ellerbroek, B.L.: 1992, in Real Time and Post-Facto Solar Image Correction, Radick, R.R., ed(s)., 13 th Sacramento Peak Summer Workshop, Sunspot, NM, In press Google Scholar
Gleckler, A.D. Markason, D.J. and Ames, G.H.: 1991, in Active and Adaptive Optical Components, Ealey, M.A., ed(s)., SPIE Proceedings 1542: Bellingham, WA, 176–189 Google Scholar
Hege, E.K.: 1988, in Very Large Telescopes and their Instrumentation, Ulrich, M.-H., ed(s)., ESO: Garching, 805–814 Google Scholar
Hege, E.K.: 1992, in High Resolution Imaging by Interferometry II, Merkle, F., ed(s)., ESO: Garching,Google Scholar
Lloyd-Hart, M., Dekany, R., McLeod, B., Wittman, D., Colucci, D., McCarthy, D. and Angel, R.: 1993, Astrophys J. Letters 402, L81–L84 CrossRefGoogle Scholar
Ulich, B.L. and Rather, J.D.G.: 1990a, in Advanced Technology Optical Telescopes IV, Barr, L.D., ed(s)., SPIE Proceedings 1236: Bellingham, WA, 985–995 Google Scholar
Ulich, B.L., Pflibsen, K., Sheppard, C. and Calmes, L.: 1990b, ibid, 768–776 Google Scholar
Wizinowich, P., McLeod, B., Lloyd-Hart, M., Angel, J.R.P., Colucci, D., Dekany, R., McCarthy, D., Wittman, D. and Scott-Fleming, I.: 1992, Appl. Opt. 31, 6036–6046 CrossRefGoogle Scholar