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NASA NTRS · 20040074298

The Millimeter-Wave Bolometric Interferometer

Abstract

The 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.

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BibTeXRIS

Ali, S., Ade, P. A. R., Bock, J. J., Novak, G., Piccirillo, L., Timbie, P., Tucker, G. S.. 2004-04-01. The Millimeter-Wave Bolometric Interferometer. https://ntrs.nasa.gov/citations/20040074298

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