Radiometric observations of the 752.033-GHz rotational absorption line of H2O from a laboratory jet |
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Authors: | G. F. Dionne J. F. Fitzgerald T-S. Chang M. M. Litvak H. R. Fetterman |
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Affiliation: | (1) Lincoln Laboratory, Massachusetts Institute of Technology, 02173 Lexington, Massachusetts;(2) Present address: Jet Propulsion Laboratory, California Institute of Technology, 91103 Pasadena, California |
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Abstract: | The intensity and lineshape of the Doppler-broadened 752.033-GHz (211 202) rotational transition of H2O has been studied passively using a high-resolution two-stage heterodyne radiometer with single-sideband system noise temperature of 45,000 K. The purpose of the experiments was to demonstrate the observability at submillimeter wavelengths of a high-altitude rocket plume simulated by a laboratory H2O jet in a vacuum chamber. First-stage mixing was accomplished by means of a GaAs Schottky diode with first local-oscillator power supplied by a CO2-laser pumped formic-acid laser (761.61 GHz), generating and X-band IF signal. Second localoscillator power was provided by a tunable C-band source. One-MHz resolution capability was obtained by means of a 3-GHz waveguide cavity filter with only 9-dB insertion loss. In the H2O jet experiments, the center frequency of the line was determined to within 1 MHz of the previously reported value. A rotational temperature 75 K, a linewidth 5 MHz, and a Doppler shift 3 MHz (from a 45-degree rotation of the flow direction) were measured with the line-of-sight intersecting the jet axis at a distance downstream of 30 nozzle diameters. These absorption data were ogtained against continuum background radiation sources at temperatures of 1175 and 300 K. |
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Keywords: | heterodyne radiometry submillimeter-wave spectra water vapor rotational lines rocket plumes |
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