NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Optical diameters of stars measured with the Mt. Wilson Mark III interferometerReliable stellar angular diameters can now be determined using the Mark III Optical Interferometer located on Mt. Wilson, California. The Mark III is a Michelson Interferometer capable of measuring the interferometric fringe visibility for stars using interferometer baselines varying from 3 to 31.5 meters in length. Angular diameters measured with the Mark III Optical Interferometer are presented for 12 stars at wavelengths of 450 and 800 nm.
Document ID
19910046081
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Simon, R. S. (Interferometrics, Inc. Vienna, VA, United States)
Mozurkewich, D. (Interferometers, Inc. Vienna, VA, United States)
Johnston, K. J. (Interferometers, Inc. Vienna, VA, United States)
Gaume, Ralph (U.S. Navy, Naval Research Laboratory, Washington DC, United States)
Hutter, D. J. (U.S. Naval Observatory Washington, DC, United States)
Bowers, P. F. (Sachs/Freeman Associates, Inc. Landover, MD, United States)
Colavita, M. M. (Interferometers, Inc. Vienna, VA, United States)
Shao, M. (JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Astronomy
Meeting Information
Meeting: Amplitude and intensity spatial interferometry
Location: Tucson, AZ
Country: United States
Start Date: February 14, 1990
End Date: February 16, 1990
Sponsors: JPL, American Astronomical Society, SPIE
Accession Number
91A30704
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available