Role of the plasma acceleration time in the dynamics of the Jovian magnetosphere

Geophysical Research Letters

Volumn 21, Issue 6, 1994, Pages 401-404

  Vasyliũnas, Vytenis M ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 85005569630     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/94GL00192     Document Type: Article

References (15)

1. A self‐consistent model of Jupiter's magnetodisc including the effects of centrifugal force and pressure
2. Drift waves, magnetospheric interchange instability, and plasma transport in the magnetosphere of Jupiter
3. Io's interaction with the plasma torus
4. Inertial limit on corotation
5. Corotation lag in Jupiter's magnetosphere: A comparison of observation and theory
6. The response of the day side magnetosphere‐ionosphere system to time‐varying field line reconnection at the magnetopause 1. Theoretical model
7. A transient response model of Pi2 pulsations
8. Plasma transport in the Io torus: the importance of microscopic diffusion
9. Nonlinear standing Alfvén wave current system at Io: Theory
10. Rotation‐driven plasma transport: the coupling of macroscopic motion and microdiffusion
11. Centrifugally driven diffusion of Iogenic plasma
12. Magnetospheric interchange motions
13. Io and its plasma environment
14. Maximum scales for preserving flux tube content in radial diffusion driven by interchange motions