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Mariner 9 Michelson interferometer.The Michelson interferometer on Mariner 9 measures the thermal emission spectrum of Mars between 200 and 2000 per cm (between 5 and 50 microns) with a spectral resolution of 2.4 per cm in the apodized mode. A noise equivalent radiance of 0.5 x 10 to the minus 7th W/sq cm/ster/cm is deduced from data recorded in orbit around Mars. The Mariner interferometer deviates in design from the Nimbus 3 and 4 interferometers in several areas, notably, by a cesium iodide beam splitter and certain aspects of the digital information processing. Special attention has been given to the problem of external vibration. The instrument performance is demonstrated by calibration data and samples of Mars spectra.
Document ID
19730026426
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hanel, R.
Schlachman, B.
(NASA Goddard Space Flight Center Greenbelt, Md., United States)
Rodgers, D.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Breihan, E.
Bywaters, R.
Chapman, F.
Rhodes, M.
Vanous, D.
Date Acquired
August 7, 2013
Publication Date
November 1, 1972
Publication Information
Publication: Applied Optics
Volume: 11
Subject Category
Instrumentation And Photography
Accession Number
73A11228
Distribution Limits
Public
Copyright
Other

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