Dust measurements in the Jovian magnetosphere

被引:29
作者
Grun, E
Kruger, H
Dermott, S
Fechtig, H
Graps, AL
Zook, HA
Gustafson, BA
Hamilton, DP
Hanner, MS
Heck, A
Horanyi, M
Kissel, J
Lindblad, BA
Linkert, D
Linkert, G
Mann, I
McDonnell, JAM
Morfill, GE
Polanskey, C
Schwehm, G
Srama, R
机构
[1] UNIV FLORIDA,GAINESVILLE,FL 32611
[2] STANFORD UNIV,CTR SPACE SCI & ASTROPHYS,STANFORD,CA 94305
[3] NASA,LYNDON B JOHNSON SPACE CTR,HOUSTON,TX 77058
[4] UNIV MARYLAND,COLLEGE PK,MD 20742
[5] CALTECH,JET PROP LAB,PASADENA,CA 91109
[6] UNIV COLORADO,ATMOSPHER & SPACE PHYS LAB,BOULDER,CO 80309
[7] LUND OBSERV,S-22100 LUND,SWEDEN
[8] MAX PLANCK INST AERON,D-37191 KATLENBURG DUHM,GERMANY
[9] UNIV KENT,CANTERBURY CT2 7NR,KENT,ENGLAND
[10] MAX PLANCK INST EXTRATERR PHYS,D-85740 GARCHING,GERMANY
[11] EUROPEAN SPACE AGCY,EUROPEAN SPACE RES & TECHNOL CTR,NL-2200 AG NOORDWIJK,NETHERLANDS
关键词
D O I
10.1029/97GL01593
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Dust measurements have been obtained with the dust detector onboard the Galileo spacecraft inside a distance of about 60R(J) from Jupiter (Jupiter radius, R-J = 71, 492 km) during two periods of about 8 days around Galileo's closest approaches to Ganymede on 27 June and on 6 Sept 1996. The impact rate of submicrometer-sized particles fluctuated by a factor of several hundred with a period of about 10 hours, implying that their trajectories are strongly affected by the interaction with the Jovian magnetic field. Concentrations of small dust impacts were detected at the times of Ganymede closest approaches that could be secondary ejecta particles generated upon impact of other particles onto Ganymede's surface. Micrometer-sized dust particles, which could be on bound orbits about Jupiter, are concentrated in the inner Jovian system inside about 20R(J) from Jupiter.
引用
收藏
页码:2171 / 2174
页数:4
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