A study of geomagnetic storms

Geophysical Journal of the Royal Astronomical Society

Volumn 54, Issue 3, 1978, Pages 547-573

  Perreault, Paul ^a   Akasofu, S I ^a  

^a UNIVERSITY OF ALASKA FAIRBANKS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84984496688     PISSN: 00168009     EISSN: 1365246X     Source Type: Journal    
DOI: 10.1111/j.1365-246X.1978.tb05494.x     Document Type: Article

References (23)

1. Recent progress in studies of DMSP auroral photographs
2. Interplanetary magnetic field and magnetospheric substorms
3. The development of the main phase of magnetic storms
4. Magnetic storms: The simultaneous development of the main phase (DR) and of polar magnetic substorms (DP)
5. Signature in the interplanetary medium for substorms
6. An empirical relationship between interplanetary conditions and Dst
7. Plasma clouds in the magnetosphere
8. A quantitative model for the potential resulting from reconnection with an arbitrary interplanetary magnetic field
9. Absence of a large‐scale reconnection flow in the frontside magnetopause
10. Is there an electrostatic field tangential to the dayside magnetopause and neutral line
11. Magnetic merging in a collisionless plasma
12. Observation of a solar flare induced interplanetary shock and helium enriched driven gas
13. Dependence of substorm occurrence probability on the interplanetary magnetic field and on the size of the auroral oval
14. Latitudinal cross section of the auroral electrojet and its relation to the interplanetary magnetic field polarity
15. Auroral electrojet current density deduced from the Chatanika radar and from the Alaska meridian chain of magnetic observatories
16. Storm sudden commencements and polar magnetospheric substotms
17. Dynamics of the geomagnetic storm
18. Global problems in magnetospheric plasma physics and prospects for their solution
19. A correlation of the occurrence of simultaneous sudden magneto‐spheric compressions and geomagnetic bay onsets with selected geophysical indices
20. Magnetopause reconnection rate
21. Auroral energy input from energetic electrons and Joule heating at Chatanika