In this section
@inproceedings{Krüger:2005:10.1063/1.2134589,
author = {Krüger, H and Forsyth, RJ and Graps, AL and Grün, E},
doi = {10.1063/1.2134589},
pages = {157--160},
title = {Electromagnetically interacting dust streams during Ulysses' second jupiter encounter},
url = {http://dx.doi.org/10.1063/1.2134589},
year = {2005}
}
TY - CPAPER
AB - The Jupiter system is a source of collimated burst-like streams 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 strength 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 along the jovian equator. © American Institute of Physics 2005.
AU - Krüger,H
AU - Forsyth,RJ
AU - Graps,AL
AU - Grün,E
DO - 10.1063/1.2134589
EP - 160
PY - 2005///
SN - 0094-243X
SP - 157
TI - Electromagnetically interacting dust streams during Ulysses' second jupiter encounter
UR - http://dx.doi.org/10.1063/1.2134589
ER -