Masses and velocity of Jovian dust streams detected by Galileo

Details Masses and velocity of Jovian dust streams detected by Galileo Masses and velocity of Jovian dust streams detected by Galileo

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..825l&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 825.

Physics

Jupiter (Planet), Galileo Spacecraft, Cosmic Dust, Solar Wind, Velocity Measurement, Line Of Sight

Scientific paper

The Galileo spacecraft detected streams of submicron dust particles near Jupiter. Two lines of evidence suggest the Jovian system to be the origin of the dust streams. Detailed modeling of the motion of small charged dust particles under the gravitational forces of the sun, Jupiter, and the solar wind magnetic field's Lorentz force shows that Jovian dust particles with radii smaller than 0.02 micron are strongly affected by the solar wind magnetic field.

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