Generation of field-aligned currents in the near-Earth magnetotail

Geophysical Research Letters

Volumn 28, Issue 9, 2001, Pages 1883-1886

  Lee, Dong Hun ^a   Lysak, Robert L ^b   Song, Yan ^b  

^a Lamont Doherty Earth Observatory   (United States)

^b UNIVERSITY OF MINNESOTA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

SUBSTORMS;

COMPRESSIBILITY; PLASMAS; WAVE EQUATIONS;

GEOPHYSICS;

AURORA; MAGNETOSPHERE;

EID: 0035334971     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL012202     Document Type: Article

References (19)

1. Hydromagnetic wave coupling in the magnetosphere-plasmapause effects on impulse-excited resonances
2. A theory of long-period magnetic pulsations, 1, Steady state excitation of field line resonance
3. A theory of long-period magnetic pulsations, 2, Impulse excitation of surface eigenmode
4. Plasma heating by spatial resonance of Alfven wave
5. Latitudinal structures of nightside field-aligned currents and their relationships to the plasma sheet regions
6. Auroral luminosity and its relationship to magnetospheric plasma domains
7. The thermal catastrophe model of substorms
8. Particle acceleration by MHD surface wave and the formation of aurora
9. Kinetic processes in plasma heating by resonant mode conversion of Alfven waves
10. A theory of long-period magnetic pulsations, 3, Local field line oscillations
11. Substorm expansion onset
12. Dynamics of MHD wave propagation in the low-latitude region
13. Nonlinear MHD wave propagation in the magnetosphere: A time-dependent approach
14. MHD wave breaking in the outer plasmasphere
15. Observations of a detached discrete arc in association with field line resonances
16. Substorm intensifications and field line resonances in the nightside magnetosphere
17. Towards a new paradigm: From a quasisteady description to a dynamical description of the magnetosphere
18. Some features of field line resonances in the magnetosphere
19. Small-scale, dispersive field line resonances in the hot magnetospheric plasma