How northward turnings of the IMF can lead to substorm expansion onsets

Geophysical Research Letters

Volumn 27, Issue 20, 2000, Pages 3257-3259

  Russell, C T ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

IONOSPHERE;

EARTH ATMOSPHERE; MAGNETIC FIELD EFFECTS; MAGNETIC FLUX; MAGNETIZATION; MAGNETOPLASMA; WIND EFFECTS; MAGNETIC FIELDS; PLASMA SHEATHS;

PLASMA SHEETS;

STORMS; EXPANSION;

EXPANSION PHASE; INTERPLANETARY MAGNETIC FIELDS; MAGNETIC FIELD LINE; MAGNETIZED PLASMAS; NEUTRAL POINTS; PLASMA SHEET; RECONNECTION RATE; SUBSTORM EXPANSION;

EID: 0034353011     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL011910     Document Type: Article

References (16)

1. Predictions of substorms following northward turnings of the interplanetary magnetic field
2. Characteristics of the association between the interplanetary magnetic field and substorm
3. Evidence of two active reconnection sites in the distant magnetotail
4. A quasi-stagnant plasmoid observed with geotail on October 15, 1993
5. Triggering of substorms by solar wind discontinuities
6. Coordinated observations demonstrating external substorm triggering
7. Satellite studies of magnetospheric substorms on August 15, 1968. IX. Phenomenological model for substorms
8. Study of weak substorms observed during December 8, 1990, Geospace Environment Modeling campaign: Timing of different types of substorm onsets
9. Two distinct types of substorm onsets
10. Plasmoids as magnetic flux ropes
11. Quasi-stagnant plasmoid in the middle tail. A new pre-expansion phase phenomenon
12. Plasma acceleration at the Earth's magnetopause: Evidence for reconnection
13. The configuration of the magnetosphere
14. Reconnexion
15. The magnetotail and substorms
16. Localized reconnection in the near Jovian magnetotail