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Conference Paper

Electromagnetically Interacting Dust Streams During Ulysses' Second Jupiter Encounter

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Krüger,  H.
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Graps,  A. L.
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Grün,  E.
Ralf Srama - Heidelberg Dust Group, Research Groups, MPI for Nuclear Physics, Max Planck Society;

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Citation

Krüger, H., Forsyth, R. J., Graps, A. L., & Grün, E. (2005). Electromagnetically Interacting Dust Streams During Ulysses' Second Jupiter Encounter. In A. I. of Physics (Ed.), NEW VISTAS IN DUSTY PLASMAS: Fourth International Conference on the Physics of Dusty Plasmas (pp. 157-160).


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-87F2-8
Abstract
The Jupiter system is a source of collimated burst-like stream of electrically charged 10-nm dust particles. In 2004 the Ulysses spacecraft had its second flyby at Jupiter and from late 2002 to early 2005 it measured a total of 24 dust streams between 0.8 and 3.4 AU from the planet. The grains show strong coupling to the interplanetary magnetic field: their impact directions correlate with the orientation and strengh of the interplanetary magnetic field vector (namely its tangential and radial components) and they occur at 26 day intervals, closely matching the solar rotation period. Ulysses measured the dust streams over a large range in jovian latitude (+75° to -35°). Enhanced dust emission was measured alongthe jovian equator..