The Development of a Probabilistic Model for Tholin Aggregation in Titan's Atmosphere

Details The Development of a Probabilistic Model for Tholin Aggregation in Titan's Atmosphere The Development of a Probabilistic Model for Tholin Aggregation in Titan's Atmosphere

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2334h&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2334

Physics

Scientific paper

A numerical model of coagulation of tholin particles in Titan's
atmosphere includes the fractal geometry of the aggregates. Dipole
charge interactions during collisions cause particles to rotate
affecting the coagulation rate and the subsequent morphology of the
grains.

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