Seasonal Changes in Titan's Polar Trace Gas Abundance Observed by Cassini

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Planets And Satellites: Atmospheres

Scientific paper

We use a six-year data set (2004-2010) of mid-infrared spectra measured by Cassini's Composite InfraRed Spectrometer to search for seasonal variations in Titan's atmospheric temperature and composition. During most of Cassini's mission Titan's northern hemisphere has been in winter, with an intense stratospheric polar vortex highly enriched in trace gases, and a single south-to-north circulation cell. Following northern spring equinox in mid-2009, dramatic changes in atmospheric temperature and composition were expected, but until now the temporal coverage of polar latitudes has been too sparse to discern trends. Here, we show that during equinox and post-equinox periods, abundances of trace gases at both poles have begun to increase. We propose that increases in north polar trace gases are due to a seasonal reduction in gas depletion by horizontal mixing across the vortex boundary. A simultaneous south polar abundance increase suggests that Titan is now entering, or is about to enter, a transitional circulation regime with two branches, rather than the single branch circulation pattern previously observed.

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

Seasonal Changes in Titan's Polar Trace Gas Abundance Observed by Cassini 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 Seasonal Changes in Titan's Polar Trace Gas Abundance Observed by Cassini, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Seasonal Changes in Titan's Polar Trace Gas Abundance Observed by Cassini will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1161871

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