Physics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.p51b1132j&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #P51B-1132
Physics
[5443] Planetary Sciences: Solid Surface Planets / Magnetospheres, [6265] Planetary Sciences: Solar System Objects / Planetary Rings
Scientific paper
We explore the dynamics of small charged dust particles in Jupiter's innermost magnetosphere. In this region the planet's ionosphere is the most important plasma source. Contrary to previous models, plasma and Poynting-Robertson drags appear to be unimportant, but the systematic charge variation of the grains results in surprisingly short lifetimes. Assuming a constant production of small dust particles via continual micrometeoroid bombardment of the larger parent bodies of the main ring, this model does reproduce most remote sensing observations of the ring/halo region of Jupiter made by Voyager, Galileo and Cassini spacecraft, and observations by the Keck telescope during ring plane crossings. The model is used to make predictions for the dust impact rates for the JUNO mission, which is expected to traverse this region multiple times starting in 2016. We report on the predicted fluxes of small grains for 3 different model calculations assuming: a) constant dust charge; b) two charge states representing the expected changes due to the lack of UV while grains are in eclipse; and c) full time-dependent dust charge. The three models predict vastly different life times, spatial and size distributions of small grains.
Horanyi Mihaly
Juhasz Andras
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