Effects of solar wind density on auroral electrojets

Geophysical Research Letters

Volumn 28, Issue 11, 2001, Pages 2181-2184

  Shue, J H ^a,b   Kamide, Y ^b  

^a JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY   (United States)

^b NAGOYA UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; SOLAR RADIATION; WIND; EARTH SCIENCES; GEOPHYSICS;

AURORAL ELECTROJETS; SOLAR WIND;

JETS; SOLAR WIND;

AURORA; ELECTROJET; SOLAR WIND;

AURORAL ELECTROJETS; DENSITY EFFECTS; DENSITY ENHANCEMENT; INTERPLANETARY MAGNETIC FIELDS; MAGNETIC CLOUDS; SOLAR WIND DENSITY; SOLAR WIND PARAMETERS;

EID: 0035365202     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL012858     Document Type: Article

References (16)

1. Interplanetary shock waves and magnetospheric substorms
2. Global structure of geomagnetic sudden commencement
3. The driving of the plasma sheet by the solar wind
4. Preconditions for the triggering of polar magnetic substorms by storm sudden commencements
5. Coordinated wind, interball/tail, and ground observations of Kelvin-Helmholtz waves at the near-tail, equatorial magnetopause at dusk: January 11, 1997
6. Solar windmagnetosphere coupling during intense storms
7. Analysis of the ionospheric cross polar cap potential drop and electrostatic potential distribution patterns during the January 1997 CME event using DMSP data
8. Interplanetary and ground magnetic conditions preceding SSC-triggered substorms
9. Internally and externally triggered substorms: A case study of the January 10, 1997 events
10. Triggering of substorms by solar wind discontinuities
11. The ionospheric response to the CME event of 6-11 January 1997
12. Effect of sudden impulses on currents in the auroral ionosphere under northward interplanetary magnetic field conditions: A case study
13. Effects of solar wind density on the westward electrojet
14. The effect of the January 10, 1997 pressure pulse on the magnetosphereionosphere current system
15. Rapid intensification and propagation of the dayside aurora: Large scale interplanetary pressure pulses (fast shocks)
16. Interplanetary shock triggering of nightside geomagnetic activity: Substorms, pseudobreakups and quiescent events