A lower limit on the top of Jupiter's haze layer

Details A lower limit on the top of Jupiter's haze layer A lower limit on the top of Jupiter's haze layer

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.280..780c&link_type=abstract

Nature, vol. 280, Aug. 30, 1979, p. 780-793. Research supported by the Science Research Council;

Physics

Haze, Jupiter Atmosphere, Satellite-Borne Photography, High Resolution, Image Processing, Infrared Spectra, Mesosphere, Remote Sensors, Stratosphere, Textures, Ultraviolet Spectra, Voyager Project

Scientific paper

Remote sensing observations of the Jovian atmosphere at wavelengths ranging from UV to the IR are affected by the presence of haze layers above the visible clouds. These layers are difficult to detect as they generally contain submicron particles. In the present paper, a sequence of Voyager images of high-latitude haze, which extends through the Jovian stratosphere into the mesosphere is presented and discussed.

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