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Solar Wind Modulation of Jupiter Dust Stream Detection
Bibcode: 2007ESASP.643...87F

Flandes, A.; Krueger, H.

During late 2002 and mid 2005, the Ulysses spacecraft approached Jupiter ( 0.8 AU at its closest distance) and detected 28 new Jovian dust particle streams. The tiny positively charged dust grains ( 10 nm) in the streams are accelerated away from Jupiter by its corotational electric field to very high speeds (greater than 200 km s^{-1}). Data indi…

2007 Dust in Planetary Systems
Ulysses 5
Dust Measurements During Ulysses' 2nd Jupiter Encounter
Bibcode: 2007ESASP.643...69K

Gruen, E.; Krueger, H.

In 2004 the Ulysses spacecraft had its second flyby at Jupiter at 0.8 AU from the planet. 28 dust streams emanating from the jovian system were identified over a 26- month period while the spacecraft was within 4 AU of the planet, and the dust instrument was operating, scanning jovigraphic latitudes from +75 degrees to -25 degrees . From late 2002…

2007 Dust in Planetary Systems
Ulysses 0
Dust in Planetary Systems
Bibcode: 2007ESASP.643.....K

Krueger, H.; Graps, A.

The workshop 'Dust in Planetary Systems' was held in Kauai'i/Hawaii from September 26 to 30, 2005, following the tradition of holding meetings in the field of Interplanetary Dust Research at regular intervals of a few years. The series of meetings started in Honolulu, Hawaii (USA) in 1967, followed by Heidelberg (Germany) in 1975, Ottawa (Canada) …

2007 Dust in Planetary Systems
Rosetta Ulysses 0