Coronal mass ejections and large geomagnetic storms

Geophysical Research Letters

Volumn 17, Issue 7, 1990, Pages 901-904

  Gosling, J T ^a   Bame, S J ^a   McComas, D J ^a   Phillips, J L ^a  

^a LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 85005726044     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/GL017i007p00901     Document Type: Article

References (13)

1. Energy coupling between the solar wind and the magnetosphere
2. An analysis of shock wave disturbances observed at 1 au from 1971 through 1978
3. Field line draping about fast coronal mass ejecta: A source of strong out‐of‐the‐ecliptic interplanetary magnetic fields
4. Mass ejections from the Sun: A view from Skylab
5. Bidirectional solar wind election heat flux events
6. The magnetotail and substorms
7. Relationship of coronal transients to interplanetary shocks: 3D aspects
8. Coronal mass ejections and interplanetary shocks
9. Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978–1979)
10. Geomagnetic response to magnetic
11. Magnetic clouds geomagnetic disturbances, and cosmic ray decreases