In this section
@article{Zook:1996:10.1126/science.274.5292.1501,
author = {Zook, HA and Grün, E and Baguhl, M and Hamilton, DP and Linkert, G and Liou, J and Forsyth, R and Phillips, JL},
doi = {10.1126/science.274.5292.1501},
journal = {Science},
pages = {1501--1503},
title = {Solar wind magnetic field bending of Jovian dust trajectories.},
url = {http://dx.doi.org/10.1126/science.274.5292.1501},
volume = {274},
year = {1996}
}
TY - JOUR
AB - 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. These masses and velocities are, respectively, about 10(3) times less massive and 5 to 10 times faster than earlier reported.
AU - Zook,HA
AU - Grün,E
AU - Baguhl,M
AU - Hamilton,DP
AU - Linkert,G
AU - Liou,J
AU - Forsyth,R
AU - Phillips,JL
DO - 10.1126/science.274.5292.1501
EP - 1503
PY - 1996///
SN - 0036-8075
SP - 1501
TI - Solar wind magnetic field bending of Jovian dust trajectories.
T2 - Science
UR - http://dx.doi.org/10.1126/science.274.5292.1501
UR - https://www.ncbi.nlm.nih.gov/pubmed/8929405
VL - 274
ER -