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NASA NTRS · 20020071038

Design and Fabrication of a Two-Dimensional Superconducting Bolometer Array

Abstract

Large format, two dimensional arrays of close-packed bolometers will enable submillimeter cameras and spectrometers to obtain images and spectra orders of magnitude faster than present instruments. The South Pole Imaging Fabry-Perot Interferometer (SPIFI) for the AST/RO observatory and the Submillimeter and Far-InfraRed Experiment (SAFIRE) on the SOFIA airborne observatory will employ a large-format, two-dimensional, closepacked bolometer arrays. Both these instruments are imaging Fabry-Perot spectrometers operating at wavelengths between 100 micron and 700 micron. The array format is 16x32 pixels, using a 32-element multiplexer developed in part for this purpose. The low backgrounds achieved in spectroscopy require very sensitive detectors with NEPs of order 5x10(exp 18) W/square root of Hz. Superconducting detectors can be close-packed using the Pop-Up Detector (PUD) format, and SQUID multiplexers operating at the detector bas temperature can be intimately coupled to them. We have fabricated an engineering model array with this technology which features a very compact, modular approach for large format arrays.

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BibTeXRIS

Benford, Dominic, Voellmer, George M., Chervenak, Jay, Irwin, Kent, Moseley, S. Harvey, Shafer, Rick, Stacey, Gordon, Staguhn, J., Oegerle, William. 2002-01-01. Design and Fabrication of a Two-Dimensional Superconducting Bolometer Array. https://ntrs.nasa.gov/citations/20020071038

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