Determination of geometrical and kinematical properties of halo coronal mass ejections using the cone model
- 31 August 2002
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 107 (A8), SSH 13-1-SSH 13-9
- https://doi.org/10.1029/2001ja009143
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998Journal of Geophysical Research, 2000
- Relationship of halo coronal mass ejections, magnetic clouds, and magnetic stormsJournal of Geophysical Research, 2000
- Interplanetary acceleration of coronal mass ejectionsGeophysical Research Letters, 2000
- Continuous tracking of coronal outflows: Two kinds of coronal mass ejectionsJournal of Geophysical Research, 1999
- X‐ray coronal changes during Halo CMEsGeophysical Research Letters, 1998
- The interplanetary events of January–May, 1997 as inferred from energetic particle data, and their relationship with solar eventsGeophysical Research Letters, 1998
- SOHO/EIT observations of an Earth‐directed coronal mass ejection on May 12, 1997Geophysical Research Letters, 1998
- LASCO observations of an Earth‐directed coronal mass ejection on May 12, 1997Geophysical Research Letters, 1998
- Coronal transient geometry. I - The flare-associated event of 1981 March 25The Astrophysical Journal, 1984
- The observation of a coronal transient directed at earthThe Astrophysical Journal, 1982