Identification of Low Coronal Sources of “Stealth” Coronal Mass Ejections Using New Image Processing Techniques
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/840/i=2/a=103/pdf
Reference29 articles.
1. JETS, CORONAL “PUFFS,” AND A SLOW CORONAL MASS EJECTION CAUSED BY AN OPPOSITE-POLARITY REGION WITHIN AN ACTIVE REGION FOOTPOINT
2. SoFAST: Automated Flare Detection with the PROBA2/SWAP EUV Imager
3. The Large Angle Spectroscopic Coronagraph (LASCO)
4. Improved methods for determining the kinematics of coronal mass ejections and coronal waves
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