An empirical model to predict the 1-AU arrival of interplanetary shocks
- 1 January 2005
- journal article
- Published by Elsevier in Advances In Space Research
- Vol. 36 (12) , 2289-2294
Abstract
No abstract availableThis publication has 10 references indexed in Scilit:
- Predicting the 1‐AU arrival times of coronal mass ejectionsJournal of Geophysical Research, 2001
- Interplanetary acceleration of coronal mass ejectionsGeophysical Research Letters, 2000
- Heliospheric 3D structure and CME propagation as seen from SOHO: Recent lessons for space weather predictionsAdvances In Space Research, 2000
- Particle acceleration at the Sun and in the heliosphereSpace Science Reviews, 1999
- Relationships between coronal mass ejection speeds from coronagraph images and interplanetary characteristics of associated interplanetary coronal mass ejectionsJournal of Geophysical Research, 1999
- A model of the Earth's distant bow shockJournal of Geophysical Research, 1997
- The solar flare mythJournal of Geophysical Research, 1993
- Magnetic field structure of interplanetary magnetic clouds at 1 AUJournal of Geophysical Research, 1990
- An analysis of shock wave disturbances observed at 1 AU from 1971 through 1978Journal of Geophysical Research, 1982
- Interplanetary acceleration of solar cosmic rays to relativistic energyJournal of Geophysical Research, 1974