Aeronomy of Saturn and Titan

Details Aeronomy of Saturn and Titan Aeronomy of Saturn and Titan

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978nascp2068..185s&link_type=abstract

In JPL The Saturn System p 185-194 (SEE N79-16758 07-91)

Computer Science

3

Atmospheric Composition, Photochemical Reactions, Saturn Atmosphere, Titan, Aeronomy, Atmospheric Models, Helium, Hydrocarbons, Hydrogen, Methane, Phosphines, Planetary Atmospheres

Scientific paper

The Saturn system presents exciting and unique objects for planetary aeronomy. The photochemistry of H2 and He leads to the formation of an ionosphere. Methane photolysis results in the formation of spectroscopically detectable amounts of C2H6 and C2H2 and in the case of Titan, C2H4. Density profiles of C2H6, C2H2, and PH3 should be indicative of the strength of atmospheric mixing processes.

Affiliated with

Also associated with

No associations

Rating

Aeronomy of Saturn and Titan 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 Aeronomy of Saturn and Titan, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Aeronomy of Saturn and Titan will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-889271