The acceleration of slow coronal mass ejections in the high‐speed solar wind
- 15 October 1996
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 23 (21) , 2867-2870
- https://doi.org/10.1029/96gl02843
Abstract
No abstract availableKeywords
This publication has 7 references indexed in Scilit:
- Some Macroscopic Properties of Shock Waves in the HeliosphereGeophysical Monograph Series, 2013
- Magnetohydrodynamic simulations of the motion of magnetic flux tubes through a magnetized plasmaJournal of Geophysical Research, 1996
- A CME‐driven solar wind disturbance observed at both low and high heliographic latitudesGeophysical Research Letters, 1995
- A new class of forward‐reverse shock pairs in the solar windGeophysical Research Letters, 1994
- The speeds of coronal mass ejections in the solar wind at mid heliographic latitudes: UlyssesGeophysical Research Letters, 1994
- Ulysses at 50° south: constant immersion in the high‐speed solar windGeophysical Research Letters, 1994
- Speeds of coronal mass ejections: SMM observations from 1980 and 1984‐1989Journal of Geophysical Research, 1994