Steady magnetospheric convection: Statistical signatures in the solar wind and AE

Geophysical Research Letters

Volumn 29, Issue 7, 2002, Pages 34-1-34-4

  O'Brien, T P ^a   Thompson, S M ^a   McPherron, R L ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

HEAT CONVECTION; MAGNETIC FIELDS; MAGNETOSPHERE;

MAGNETOSPHERIC CONVECTION; SOLAR WIND;

GEOPHYSICS;

MAGNETOSPHERE; SOLAR WIND;

EID: 0036555044     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001GL014641     Document Type: Article

References (13)

1. Spontaneous substorm onset during a prolonged period of steady, southward interplanetary magnetic field
2. The occurrence rate of magnetospheric substorm onsets: Random and periodic substorms
3. Observations of magnetospheric substorms occurring with no apparent solar wind/IMF trigger
4. An evaluation of the statistical significance of the association between northward turnings of the IMF and substorm expansion onsets
5. Dependence of substorm occurrence probability on the interplanetary magnetic field and on the size of the auroral oval
6. Substorms: Fundamental observation features, distinction from other disturbances and external triggering
7. Auroral disturbances during the January 10, 1997 magnetic storm
8. Multiplesatellite studies of magnetospheric substorms: Distinction between polar magnetic substorms and convection-driven negative bays
9. Steady magnetospheric convection: A review of recent results
10. Short-duration convection bays and localized interplanetary magnetic field structures on November 28, 1995
11. z
12. The paradox of the expected time until the next earthquake