Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1767366 | Advances in Space Research | 2010 | 9 Pages |
Abstract
The principal objective of this study is to analyze structures of Coronal Mass Ejections (CMEs) using a wavelet technique. We use data measured with the SOHO/LASCO coronographs C2–C3, EIT and STEREO COR1A–B, COR2A–B. We have found that different structures show up in a CME at different spatial scales of wavelets. We also study the orientation of the most intense flux and find the orientation of the structures in the CME.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
D.I. González-Gómez, X. Blanco-Cano, A.C. Raga,