Jupiter's Dusty Plasma Manifested

Details Jupiter's Dusty Plasma Manifested Jupiter's Dusty Plasma Manifested

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....12540g&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #12540

Physics

Scientific paper

Upon applying criteria for "dust-in-plasma" and "dusty-plasma" using the dust grain size, Debye length, and dust intergrain distance of the Jovian dust stream particles, we find that, in the part of the Jovian magnetosphere starting from 10-15 Jovian radii, collective effects might be important. From roughly this distance, a dusty plasma, rather than a dust-in-plasma fits the Jupiter magnetopheric conditions. Collective interactions occur when self-generated fields of the particles take over a correlative role, therefore the particles could behave differently from what would be expected from single particle physics. More complex frequencies and waves should be seen. In this presentation, I will show how to distinquish between dust-in-plasma and dusty plasma regimes and why current Galileo dust stream data hints at dusty plasma collective behavior. Funding for this work was provided by the Deutsche Forschungsgemeinschaft (DFG).

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