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The Millimeter-Wave Bolometric InterferometerThe Millimeter-wave Bolometric Interferometer (MBI) is a proposed ground-based instrument designed for a wide range of cosmological and astrophysical observations including studies of the polarization of the cosmic microwave background (CMB). MBI combines the advantages of two well-developed technologies - interferometers and bolometric detectors. Interferometers have many advantages over .filled-aperture telescopes and are particularly suitable for high resolution imaging. Cooled bolometers are the highest sensitivity detectors at millimeter and sub-millimeter wavelengths. The combination of these two technologies results in an instrument with both high sensitivity and high angular resolution.
Document ID
20040074298
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Ali, S.
(Wisconsin Univ. Madison, WI, United States)
Ade, P. A. R.
(Wales Univ. Inst. of Science and Technology Cardiff, United Kingdom)
Bock, J. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Novak, G.
(Northwestern Univ. Evanston, IL, United States)
Piccirillo, L.
(Wales Univ. Inst. of Science and Technology Cardiff, United Kingdom)
Timbie, P.
(Wisconsin Univ. Madison, WI, United States)
Tucker, G. S.
(Brown Univ. Providence, RI, United States)
Date Acquired
September 7, 2013
Publication Date
April 1, 2004
Publication Information
Publication: New Concepts for Far-Infrared and Submillimeter Space Astronomy
Subject Category
Instrumentation And Photography
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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