Multiscale Feature Identification in Solar Flares and CMEs

Details Multiscale Feature Identification in Solar Flares and CMEs Multiscale Feature Identification in Solar Flares and CMEs

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spd....34.0307m&link_type=abstract

American Astronomical Society, SPD meeting #34, #03.07; Bulletin of the American Astronomical Society, Vol. 35, p.809

Mathematics

Logic

Scientific paper

Multiscale methods offer a powerful approach to solar image processing and analysis. In this paper, wavelet-based methods are applied to a sequence of TRACE 195 Å passband images to unambiguously identify faint features associated with the 2002 April 21 X-class flare and CME. Morphological properties, such as feature width, height, velocity and acceleration are then extracted, and compared to recent results from traditional image processing techniques.

Affiliated with

Also associated with

No associations

Rating

Multiscale Feature Identification in Solar Flares and CMEs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multiscale Feature Identification in Solar Flares and CMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiscale Feature Identification in Solar Flares and CMEs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-985553