Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007dps....39.1913m&link_type=abstract
American Astronomical Society, DPS meeting #39, #19.13; Bulletin of the American Astronomical Society, Vol. 39, p.446
Astronomy and Astrophysics
Astronomy
Scientific paper
Using a one-dimensional version of the Saturn Thermosphere Ionosphere Model (STIM), we perform calculations of the ion and electron temperatures in the ionosphere of Saturn. There are no direct measurements of plasma temperatures in Saturn's atmosphere published to date, but they are often estimated from the topside plasma scale heights of radio occultation measurements of electron density. Based on Pioneer, Voyager, and now Cassini data, those estimates range from 625 K to 1700 K. Our preliminary calculations reproduce the lower level of that range, with an electron temperature peak value of just over 600 K at midlatitudes near dawn and dusk. Our calculations also suggest a diurnal variation of more than 200 K. Finally, our results allow an assessment of the reliability of estimating plasma temperatures from altitude profiles of electron density, which are also computed in STIM. By applying a range of background conditions (e.g., neutral atmosphere, solar flux) we explore the parameter space of possible variability of plasma temperatures on Saturn.
STIM development at Boston University was funded by the NASA Planetary Atmospheres program. LM acknowledges support from a NASA Graduate Student Researchers Program fellowship, IM-W is supported by a British Royal Society Fellowship.
Galand Marina
Mendillo Michael
Moore Luke
Müller-Wodarg Ingo
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