An MHD simulation of plasma flow past Io: Alfvén and slow mode perturbations

Geophysical Research Letters

Volumn 15, Issue 11, 1988, Pages 1311-1314

  Linker, Jon A ^a   Kivelson, Margaret G ^a   Walker, Raymond J ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0042586618     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/GL015i011p01311     Document Type: Article

References (17)

1. Standing Alfvén wave current system at Io: Voyager 1 observations
2. Revised ion temperatures for Voyager plasma measurements in the Io plasma torus
3. A time dependent three dimensional simulation of the earth's magnetosphere: Reconnection events
4. Drag and propulsion of large satellites in the ionosphere: An Alfven propulsion engine in space
5. The solar wind‐magnetosphere‐ionosphere current voltage relationship
6. Lo's interaction with the plasma torus
7. Global simulation of the three dimensional magnetosphere
8. Nonlinear standing Alfven wave current system at Io: Theory
9. A three‐dimensional MHD simulation of the interaction of the solar wind with the earth's magnetosphere: The generation of field‐aligned currents
10. A three dimensional MHD simulation of the interaction of the solar wind with comet Halley
11. Io and its plasma environment
12. Lo's interaction with the plasma torus: A self‐consistent model
13. Stationary Alfvénic structures
14. A three dimensional MHD model of the earth's magnet osphere