# Solar Wind Magnetic Field Bending of Jovian Dust Trajectories

@article{Zook1996SolarWM,
title={Solar Wind Magnetic Field Bending of Jovian Dust Trajectories},
author={Herbert A. Zook and Eberhard Gr{\"u}n and Michael Baguhl and David P. Hamilton and G. Linkert and Jim C. P. Liou and Robert J. Forsyth and John L. Phillips},
journal={Science},
year={1996},
volume={274},
pages={1501 - 1503}
}
• Published 29 November 1996
• Physics, Geology
• Science
From September 1991 to October 1992, the cosmic dust detector on the Ulysses spacecraft recorded 11 short bursts, or streams, of dust. These dust grains emanated from the jovian system, and their trajectories were strongly affected by solar wind magnetic field forces. Analyses of the on-board measurements of these fields, and of stream approach directions, show that stream-associated dust grain masses are of the order of 10−18 gram and dust grain velocities exceed 200 kilometers per second…
• Physics, Geology
• 2000
The Ulysses spacecraft, launched in October 1990, orbits the Sun on a polar trajectory. The spacecraft is equipped with a highly sensitive impact- ionization dust detector which can in situ measure
• Physics, Geology
Nature
• 2005
All bursts of dust impacts detected within 150 Saturn radii are characterized by impact directions markedly different from those measured between the bursts, and they clearly coincide with the spacecraft's traversals through streams of compressed solar wind.
• Physics, Geology
• 1997
Dust measurements have been obtained with the dust detector onboard the Galileo spacecraft inside a distance of about 60RJ from Jupiter (Jupiter radius, RJ = 71,492 km) during two periods of about 8
• Physics, Geology
• 2002
Jupiter was discovered to be a source of high speed dust particles by the Ulysses spacecraft in 1992. These dust particles originate from the volcanic plumes on Io. They collect electrostatic charges
• Geology, Physics
Nature
• 1999
Dust pervades the Solar System, and is concentrated in the ring systems surrounding the giant planets and along the plane of the planetary orbits (the Zodiacal cloud). Individual dust grains are
This is a review of recent in situ and remote sensing observations, and theoretical advances of our understanding dust plasma interactions in Jupiter's magnetosphere. Dust grains exposed to plasmas
• Physics, Geology
• 1998
We report on dust measurements obtained during the seventh orbit of the Galileo spacecraft about Jupiter. The most prominent features observed are highly time variable dust streams recorded
• Physics, Geology
• 2005
In 1992 the impact ionisation dust detector on board the Ulysses spacecraft discovered periodic burst-like streams of dust particles within 2AU from Jupiter. The streams occurred at approximately
• Physics, Geology
Nature
• 2000
Io's volcanoes, rather than impact ejecta, are the dust sources of the jovian dust streams, on the basis of periodicities in the dust impact signal.
• Physics, Geology
• 2012
Stream particles are nanometer-sized dust particles ejected from the Jovian and Saturnian systems with speeds higher than 100$$\mathrm{{km\,s}}^{-1}$$. Due to the large charge-to-mass ratio, their

## References

SHOWING 1-10 OF 20 REFERENCES

• Physics, Geology
Science
• 1996
About a hundred dust impacts per day were detected during the first week in December 1995 by Galileo during its approach to Jupiter. These impacts were caused by submicrometer-sized particles that
• Physics, Geology
Nature
• 1993
PERHAPS the most unexpected finding of the Ulysses mission so far has been the detection of quasi-periodic streams of high-velocity, submicrometre-sized dust particles during the spacecraft's
• Physics, Geology
Science
• 1992
Dust flux measurements give evidence of the recent rates of production from sources such as comets, asteroids, and moons, as well as the possible presence of interstellar grains.
• Physics, Geology
Nature
• 1996
THE Ulysses spacecraft detected streams of sub-micrometre-sized dust particles as it approached Jupiter in 19921,2. Although interplanetary space was known to contain dust, the presence of discrete
• Physics, Geology
• 1993
Near-ecliptic solar wind observations by Ulysses on its way to the polar regions of the Sun, compared with those from IMP 8 at 1 AU, showed that high-speed streams decay and broaden with heliocentric

### R found 5 additional streams in the Ulysses' CDD dataset

• Space Sci. 41,
• 1994