A search for p-mode oscillations of Jupiter - Serendipitous observations of nonacoustic thermal wave structure

Details A search for p-mode oscillations of Jupiter - Serendipitous observations of nonacoustic thermal wave structure A search for p-mode oscillations of Jupiter - Serendipitous observations of nonacoustic thermal wave structure

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...343..456d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 343, Aug. 1, 1989, p. 456-467.

Computer Science

Sound

60

Coriolis Effect, Jupiter Atmosphere, Modal Response, Planetary Radiation, Brightness Temperature, Hydrodynamics, Solar Oscillations, Sound Waves, Jupiter, Oscillations, Waves, Structure, Frequencies, Infrared, Spectra, Wavelengths, Intensity, Amplitude, Brightness, Hydrodynamics, Turbulence, Motion, Earth-Based Observations, Power, Thermal Properties, Temperature, Comparisons, Calculations

Scientific paper

Frequencies for the p-mode oscillations of Jupiter have been determined, and infrared brightness temperature fluctuations are used to search for the modes. Measurements of the infrared intensity of the Jovian disk were obtained in a broad bandwidth using a 20-element linear array. No p-mode oscillations were observed at the 0.07-K level in the 8-13-micron brightness temperature. The results suggest that Jovian p modes are not likely to have observable amplitudes. A prominent nonacoustic wave-like structure in the 8-13-micron brightness temperature is found both at 20 deg N and at the equator.

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