Geoeffectiveness of Coronal Mass Ejections in the SOHO Era
- 21 October 2014
- journal article
- research article
- Published by Springer Science and Business Media LLC in Solar Physics
- Vol. 290 (2), 579-612
- https://doi.org/10.1007/s11207-014-0613-8
Abstract
No abstract availableKeywords
This publication has 41 references indexed in Scilit:
- A logistic regression model for predicting the occurrence of intense geomagnetic stormsAnnales Geophysicae, 2005
- Properties and geoeffectiveness of magnetic clouds in the rising, maximum and early declining phases of solar cycle 23Annales Geophysicae, 2005
- Evolutionary signatures in complex ejecta and their driven shocksAnnales Geophysicae, 2004
- Solar and interplanetary sources of major geomagnetic storms during 1996–2002Journal of Geophysical Research, 2004
- Kinematics of coronal mass ejections between 2 and 30 solar radiiAstronomy & Astrophysics, 2004
- A catalog of white light coronal mass ejections observed by the SOHO spacecraftJournal of Geophysical Research, 2004
- RELATIONSHIP BETWEEN CME KINEMATICS AND FLARE STRENGTHJournal of The Korean Astronomical Society, 2003
- Identification of Solar Sources of Major Geomagnetic Storms between 1996 and 2000The Astrophysical Journal, 2003
- A Statistical Study of Two Classes of Coronal Mass EjectionsThe Astrophysical Journal, 2002
- Coronal mass ejections and large geomagnetic stormsGeophysical Research Letters, 1990