Behavior of aurora during 10-12 May, 1999 when the solar wind nearly dissapeared

Geophysical Research Letters

Volumn 27, Issue 24, 2000, Pages 4033-4036

  Parks, G ^a   Brittnacher, M ^a   Chua, D ^a   Fillingim, M ^a   Germany, G ^b   Spann, J ^c  

^a UNIVERSITY OF WASHINGTON   (United States)

^b UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^c NASA MARSHALL SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

AURORA; MAGNETOSPHERE; SOLAR WIND;

GEOMAGNETISM; MAGNETISM; MAGNETOSPHERE; SOLAR SYSTEM;

AURORAL ACTIVITIES; ELECTRON PRECIPITATION; GEOMAGNETIC ACTIVITIES; HIGH MAGNETIC LATITUDES; INTERPLANETARY MAGNETIC FIELDS; PRIMARY PARAMETERS; SOLAR WIND DENSITY; TIME-SCALES;

SOLAR WIND;

EID: 0034670979     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL000106     Document Type: Article

References (4)

1. Global auroral response to a solar wind pressure pulse
2. Energy characteristics of auroral electron precipitation: A comparison of substorms and pressure pulse related auroral activity
3. Coincident POLAR/UVI and WIND bservations of pseudobreakups
4. Electrodynamic patterns in the polar region during periods of extreme magnetic quiescence