Morphological Study of Coronal Mass Ejections using Wavelet

Details Morphological Study of Coronal Mass Ejections using Wavelet Morphological Study of Coronal Mass Ejections using Wavelet

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsh41b..04g&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SH41B-04

Physics

2101 Coronal Mass Ejections (7513), 7509 Corona, 7513 Coronal Mass Ejections (2101), 7536 Solar Activity Cycle (2162)

Scientific paper

The principal objective of this study is to analyze structures inside Coronal Mass Ejections (CMEs) using wavelet technique. We have used the archived public data taken with the SOHO/LASCO coronographs C2 and C3. We have found that different structures that can exist in a CME can be observed at different spatial scales of wavelets. We also look for the direction and orientation of the most intense flux that is present in a CME in the entire image. We intend to use the same wavelet technique to reconstruct the original image and obtain higher contrasts of the image.

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