Kinematic Evolution of a Slow CME in Corona Viewed by STEREO-B on 8 October 2007
- 23 February 2011
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 269 (2) , 389-400
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This publication has 33 references indexed in Scilit:
- DETERMINING THE AZIMUTHAL PROPERTIES OF CORONAL MASS EJECTIONS FROM MULTI-SPACECRAFT REMOTE-SENSING OBSERVATIONS WITHSTEREOSECCHIThe Astrophysical Journal, 2010
- STEREO observations of interplanetary coronal mass ejections and prominence deflection during solar minimum periodAnnales Geophysicae, 2009
- Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)Space Science Reviews, 2008
- The STEREO Mission: An IntroductionSpace Science Reviews, 2007
- Properties of structured coronal mass ejections in solar cycle 23Advances In Space Research, 2006
- Introduction to the special section: Violent Sun‐Earth connection events of October–November 2003Geophysical Research Letters, 2005
- Intensity variation of large solar energetic particle events associated with coronal mass ejectionsJournal of Geophysical Research, 2004
- On the three-dimensional configuration of coronal mass ejectionsAstronomy & Astrophysics, 2004
- LASCO and EIT Observations of Helical Structure in Coronal Mass EjectionsThe Astrophysical Journal, 1999
- The propagation of coronal mass ejection transientsJournal of Geophysical Research, 1986