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Statistical properties and geoefficiency of interplanetary coronal mass ejections and their sheaths during intense geomagnetic storms
Jianpeng Guo, Xueshang Feng, Jie Zhang, Pingbing Zuo and Changqing Xiang Journal of Geophysical Research: Space Physics 115(A9) (2010) https://doi.org/10.1029/2009JA015140
Predictions of interplanetary shock arrivals at Earth: Dependence of forecast outcome on the input parameters
Lunar surface charging during solar energetic particle events: Measurement and prediction
J. S. Halekas, G. T. Delory, R. P. Lin, T. J. Stubbs and W. M. Farrell Journal of Geophysical Research: Space Physics 114(A5) n/a (2009) https://doi.org/10.1029/2009JA014113
Multifractal analysis of geomagnetic storm and solar flare indices and their class dependence
CME Propagation Characteristics from Radio Observations
S. Pohjolainen, L. van Driel-Gesztelyi, J. L. Culhane, P. K. Manoharan and H. A. Elliott Solar Physics 244(1-2) 167 (2007) https://doi.org/10.1007/s11207-007-9006-6
On the Evolution of Coronal Mass Ejections in the Interplanetary Medium
T. A. Howard, C. D. Fry, J. C. Johnston and D. F. Webb The Astrophysical Journal 667(1) 610 (2007) https://doi.org/10.1086/519758
Orientations of LASCO Halo CMEs and their connection to the flux rope structure of interplanetary CMEs
Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen Publications of the Astronomical Society of the Pacific 118(845) 947 (2006) https://doi.org/10.1086/506157
The Deceleration of an Interplanetary Transient from the Sun to 5 Au
Tracking halo coronal mass ejections from 0–1 AU and space weather forecasting using the Solar Mass Ejection Imager (SMEI)
T. A. Howard, D. F. Webb, S. J. Tappin, D. R. Mizuno and J. C. Johnston Journal of Geophysical Research: Space Physics 111(A4) (2006) https://doi.org/10.1029/2005JA011349
Recurrent Magnetic Storms: Corotating Solar Wind Streams
G. Lu Geophysical Monograph Series, Recurrent Magnetic Storms: Corotating Solar Wind Streams 167 97 (2006) https://doi.org/10.1029/167GM10
The Automatic Predictability of Super Geomagnetic Storms from halo CMEs associated with Large Solar Flares