Online-Ressource
American Geophysical Union (AGU)
;
1993
In:
Journal of Geophysical Research: Space Physics Vol. 98, No. A12 ( 1993-12), p. 21245-21251
In:
Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 98, No. A12 ( 1993-12), p. 21245-21251
Kurzfassung:
We suggest a model to explain the unexpected recurrent dust events that were observed during the Jupiter encounter by the dust detector on board the Ulysses spacecraft. This model is based on dust‐magnetosphere interactions. Dust particles inside the Jovian magnetosphere collect electrostatic charges and their interaction with the magnetic and electric fields can lead to energization and subsequent ejection. We discuss the dusty regions (ring/halo, “gossamer” ring) and also Io as potential sources for the Ulysses events. This model favors Io as a source. The mass and velocity range of the escaping particles are compatible with the observations, and we also suggest internal periodicities to explain the recurrent nature of the Ulysses dust events.
Materialart:
Online-Ressource
ISSN:
0148-0227
Sprache:
Englisch
Verlag:
American Geophysical Union (AGU)
Publikationsdatum:
1993
ZDB Id:
2033040-6
ZDB Id:
3094104-0
ZDB Id:
2130824-X
ZDB Id:
2016813-5
ZDB Id:
2016810-X
ZDB Id:
2403298-0
ZDB Id:
2016800-7
ZDB Id:
161666-3
ZDB Id:
161667-5
ZDB Id:
2969341-X
ZDB Id:
161665-1
ZDB Id:
3094268-8
ZDB Id:
710256-2
ZDB Id:
2016804-4
ZDB Id:
3094181-7
ZDB Id:
3094219-6
ZDB Id:
3094167-2
ZDB Id:
2220777-6
ZDB Id:
3094197-0
SSG:
16,13
Bookmarklink
Bibliothek |
Standort |
Signatur |
Band/Heft/Jahr |
Verfügbarkeit |