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NASA NTRS · 19870008796

Technology for satellite power conversion

Abstract

The work is this reporting period was concentrated on electronically calibrating the bolometer detectors. The calibration is necessary for two reasons: first, the power delivered to the rectifying circuit must be known in order to choose a diode with the appropriate barrier height, and second, the power captured by the antenna must be measured if the efficiency of the rectenna is to be divided into antenna efficiency and rectification efficiency. The millimeter wave region operation of the bolometers was simulated with a VHF (10 to 90 MHz) test signal. These detectors are accurate to within roughly 10%. The typical responsivity of the bolometers is 10 volts/watt and the NEP at 20 Hz is 5 times 10 to the minus 9th power W(Hz)-1/2.

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BibTeXRIS

Gouker, M. A., Campbell, D. P., Gallagher, J. J.. 1987-02-27. Technology for satellite power conversion. https://ntrs.nasa.gov/citations/19870008796

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