Mapping the temperature and composition of Saturn's stratosphere from Cassini/CIRS observations

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5210 Planetary Atmospheres, Clouds, And Hazes (0343), 5704 Atmospheres (0343, 1060), 5739 Meteorology (3346), 6275 Saturn

Scientific paper

Using the limb observations provided by the Composite Infrared Spectrometer aboard the Cassini spacecraft, we obtained an unprecedended map of the temperature between 20~hPa to 0.003~hPa, and of the composition (ethane and acetylene) between 10~hPa and 0.01~hPa, with a vertical resolution of 1.5 times a scale height. The statospheric temperature structure and the derived thermal wind structure show the presence of an equatorial oscillation similar to the terrestrial QBO and jovian QQO. At extratropical latitudes, the temperature structure exhibits a smoother increase with altitude. However, in the upper stratosphere, the radiative cooling rates at mid-latitudes in northern and southern hemispheres does not balance with the local solar heating rates. This desiquilibrium can be explained by a meridional circulation from the southern to the northern hemisphere. The composition of the stratosphere, with enhancement of hydrocarbon abundance in the northern hemisphere at high altitudes constitutes another evidence for a meridional circulation.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Mapping the temperature and composition of Saturn's stratosphere from Cassini/CIRS observations 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 Mapping the temperature and composition of Saturn's stratosphere from Cassini/CIRS observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mapping the temperature and composition of Saturn's stratosphere from Cassini/CIRS observations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1406124

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.