JIME - the Enhanced Jovian Ionospheric Model

Details JIME - the Enhanced Jovian Ionospheric Model JIME - the Enhanced Jovian Ionospheric Model

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....3777w&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #3777

Physics

Scientific paper

JIME is an evolution of the time-dependent Jovian Ionospheric Model developed by the Atmospheric Physics Group at University College London. Features such as the ability to vary stellar radiation input and H3+ cooling were added in order to better allow JIME to simulate the expected conditions in recently detected 51-Peg type exoplanets orbiting close to their parent star. Using this model a comparison of ionospheric composition was undertaken between a rotating and tidally locked planet at varying orbital radii down to 0.1AU, allowing the effects of intense planetary irradiation to be observed.

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