Observing coronal mass ejections without coronagraphs
Open Access
- 1 November 2001
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 106 (A11) , 25199-25213
- https://doi.org/10.1029/2000ja904026
Abstract
No abstract availableKeywords
This publication has 129 references indexed in Scilit:
- Bidirectional particle flows at cosmic ray and lower (∼1 MeV) energies and their association with interplanetary coronal mass ejections/ejectaJournal of Geophysical Research, 2000
- Small‐scale magnetic flux ropes in the solar windGeophysical Research Letters, 2000
- Continuous tracking of coronal outflows: Two kinds of coronal mass ejectionsJournal of Geophysical Research, 1999
- Coronagraph observations of inflows during high solar activityGeophysical Research Letters, 1999
- X‐ray coronal changes during Halo CMEsGeophysical Research Letters, 1998
- The solar origin of the January 1997 coronal mass ejection, magnetic cloud and geomagnetic stormGeophysical Research Letters, 1998
- SOHO/EIT observations of an Earth‐directed coronal mass ejection on May 12, 1997Geophysical Research Letters, 1998
- The solar energetic particle event of April 14, 1994, as a probe of shock formation and particle accelerationJournal of Geophysical Research, 1998
- Tracing the topology of the October 18–20, 1995, magnetic cloud with ∼0.1–10² keV electronsGeophysical Research Letters, 1997
- Evidence for magnetic disconnection of mass ejections in the coronaJournal of Geophysical Research, 1995