Jupiter H3+ Auroral Emission Model for Electron Energy Estimation

Details Jupiter H3+ Auroral Emission Model for Electron Energy Estimation Jupiter H3+ Auroral Emission Model for Electron Energy Estimation

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1831t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1831

Physics

Scientific paper

We investigate the feasibility of determining the properties of Jupiter's auroral electrons from infrared (IR) emission line intensities using an auroral emission model. The ratios of three H3 + IR emission line intensities are required to determine the electron energy and background temperature. We evaluate the accuracy of the estimates derived using this method as a function of the accuracy of the observations.

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