Computer Science
Scientific paper
Aug 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...47..159b&link_type=abstract
Icarus, vol. 47, Aug. 1981, p. 159-165.
Computer Science
28
Albedo, Atmospheric Circulation, Diurnal Variations, Infrared Radiation, Neptune Atmosphere, Upper Atmosphere, Atmospheric Effects, Atmospheric Scattering, Haze, Light Curve, Uranus (Planet), Neptune, Atmosphere, Rotation, Infrared, Brightness, Comparisons, Data, Amplitude, Spectrum, Wavelengths, Photometry, Flux, Uranus, Magnitude, Geometry, Light Curve, Particles, Period
Scientific paper
The variations in the near-infrared brightness of Neptune observed during July and August 1980 show a well-defined, large-amplitude variation in Neptune's J-K color, with a period of 17.73 + or - 0.1 hour. These results are interpreted as diurnal variations resulting from the 17.73-hour rotation period of the Neptune upper atmosphere in the presence of inhomogeneous weather, and are found to qualitatively corroborate those of Cruikshank (1978). It is also noted that Smith and Slavsky (1980) report a 17.7-hour component as a secondary periodicity in their data. Variations were observed in the 5-0-micron spectral region which are in phase with the variations seen at shorter wavelengths.
Brown Harvey R.
Cruikshank Dale P.
Tokunaga Alan T.
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