Modeling low density sulfur dioxide jets: Application to volcanoes on jupiter's moon Io

J. Zhang, D. B. Goldstein, N. E. Gimelshein, S. F. Gimelsheint, D. A. Levin, P. L. Varghese

Research output: Contribution to conferencePaperpeer-review

Abstract

Modeling results of volcanic plumes on Jupiter's moon lo are presented. Two types of low density axisymmetric SO2 plume flows are modeled using the direct simulation Monte Carlo method. Thermal radiation from all three vibrational bands and overall rotational bands of SO2 molecules are included in the simulations. The radiation features were examined both by calculating infrared emission spectra along several lines-of-sight through the plume and the DSMC modeled emission images of the whole flow field. A high resolution plume core flow was obtained by multi-domain sequential calculation to better study the radiation signature. The simulation results are compared to the existing observation data. Future comparisons with the Galileo or other astronomical observations are expected to validate and improve our model.

Original languageEnglish (US)
DOIs
StatePublished - 2001
Externally publishedYes
Event35th AIAA Thermophysics Conference 2001 - Anaheim, CA, United States
Duration: Jun 11 2001Jun 14 2001

Other

Other35th AIAA Thermophysics Conference 2001
CountryUnited States
CityAnaheim, CA
Period6/11/016/14/01

ASJC Scopus subject areas

  • Aerospace Engineering
  • Mechanical Engineering
  • Condensed Matter Physics

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