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Quantitative assessment of the science return from an orbiting, imaging, optical interferometerImaging simulations were performed with the filled Mills cross orbiting, imaging, optical interferometer proposed by Synnott et al. (1990) in order to determine its capabilities in the area of spatial resolution, dynamic range, and sensitivity. Astronomical objects have been chosen as candidate program sources to determine whether this interferometer design can accomplish research goals relating to the objects.
Document ID
19920073819
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Meier, David L. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Synnott, Stephen P. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Dumont, Philip J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jones, Dayton L. (JPL Pasadena, CA, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Subject Category
Astronomy
Meeting Information
Meeting: IAU Colloquium on Radio Interferometry: Theory, Techniques and Applications
Location: Socorro, NM
Country: United States
Start Date: October 8, 1990
End Date: October 12, 1990
Accession Number
92A56443
Distribution Limits
Public
Copyright
Other

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