A possible scenario for the associated occurrence of flares, prominence eruptions, coronal mass ejections, and coronal holes in relation to interplanetary shocks

Advances in Space Research

Volumn 17, Issue 4-5, 1996, Pages 285-288

  Bravo, S ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0041536611     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00586-4     Document Type: Article

References (19)

1. Coronal holes as sources of large-scale solar wind disturbances and geomagnetic perturbations
2. The solar causes of major geomagnetic storms
3. Why fast solar wind originates from slowly expanding coronal flux tubes
4. Solar sources of the interplanetary magnetic field and solar wind
5. The launch of solar coronal mass ejections: Results from the coronal mass ejection onset program
6. A major shock-associated energetic storm particle event wherein the shock plays a minor role