Field-aligned currents during IMF ○ 0

Geophysical Research Letters

Volumn 28, Issue 15, 2001, Pages 3055-3058

  Papitashvili, V O ^b   Christiansen, F ^a   Neubert, T ^a  

^a DANISH METEOROLOGICAL INSTITUTE   (Denmark)

^b UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETOSPHERE; MAGNETIC FIELDS; MAPPING; SATELLITES;

FIELD ALIGNED CURRENTS; FIELD LINES; INTERPLANETARY MAGNETIC FIELDS; NORTHWARD IMF; POLAR CAP; STATISTICAL DISTRIBUTION; VISCOUS INTERACTION;

MAGNETIC FIELDS; GEOPHYSICS;

FIELD-ALIGNED CURRENTS;

GEOMAGNETIC FIELD; SOLAR WIND;

EID: 0035418682     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001GL012944     Document Type: Article

References (14)

1. Field-aligned currents in the dayside cusp observed by Triad
2. Large-scale Birkeland currents in the dayside polar region during strongly Northward IMF: A new Birkeland current system
3. y derived from SuperDARN radar observations
4. Ionospheric convection produced by quasi-viscous interaction of the solar wind with the magnetosphere
5. A three-dimensional MHD simulation of the interaction of the solar wind with the Earth's magnetosphere: The generation of field-aligned currents
6. Four-sheet structures of dayside field-aligned currents: Statistical study
7. ØOrsted initial field model
8. Convection to the dayside at the center of the polar cap in the case of Southern IMF: A new current system
9. Equivalent ionospheric currents above Antarctica during the austral summer
10. Electric potential patterns in the Northern and Southern polar regions parameterized by the interplanetary magnetic field
11. y-dependent plasma flow and Birkeland currents in the dayside magnetosphere: 2. A global model for Northward and Southward IMF
12. y-controlled convection and field-aligned currents near midnight auroral oval for Northward interplanetary magnetic field
13. Field-aligned current systems in the magnetospheric ground state
14. Maps of ionospheric field-aligned currents as a function of the interplanetary magnetic field derived from dynamic explorer 2 data