Observations and non-linear simulations of Jupiter's 2010 SEBD

Details Observations and non-linear simulations of Jupiter's 2010 SEBD Observations and non-linear simulations of Jupiter's 2010 SEBD

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..389l&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.389

Physics

Scientific paper

We present the evolution, motions and nonlinear simulations of the planetary-scale disturbance that initiated in the South Equatorial Belt of Jupiter (SEBD) on November 9, 2010. Data on motions were obtained from high-resolution images submitted to the PVOL-International Outer Planet Watch database [1]. Non-linear simulations of the disturbance potential vorticity evolution at cloud level were done using the EPIC code [2].

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