Slowly moving thermal features on Jupiter

Details Slowly moving thermal features on Jupiter Slowly moving thermal features on Jupiter

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.337..444m&link_type=abstract

Nature (ISSN 0028-0836), vol. 337, Feb. 2, 1989, p. 444-447.

Physics

28

Cloud Physics, Jupiter (Planet), Planetary Atmospheres, Image Analysis, Infrared Spectroscopy, Temperature Distribution, Velocity Distribution, Voyager 1 Spacecraft, Voyager 2 Spacecraft, Jupiter, Thermal Properties, Features, Atmosphere, Structure, Winds, Depth, Troposphere, Temperature, Voyager Missions, Iris Instrument, Spacecraft Observations, Spectra, Motion, Velocity, Meteorology, Hypotheses, Anomalies, Techniques, Dynamics

Scientific paper

Maps of the Jovian upper troposphere temperatures derived from Voyager 1 and Voyager 2 infrared interferometer spectrometer (IRIS) spectra show large-scale features which move very slowly. The motion is very different from the inferred local fluid velocity. It is suggested that these features may indicate a deeply-rooted fluid dynamical regime beneath the surface meteorology.

Affiliated with

Also associated with

No associations

Rating

Slowly moving thermal features on Jupiter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Slowly moving thermal features on Jupiter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Slowly moving thermal features on Jupiter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885331