Automatic recognition of solar features

Details Automatic recognition of solar features Automatic recognition of solar features

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..371b&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 371-3

Computer Science

H Alpha Line, Image Analysis, Pattern Recognition, Solar Magnetic Field, Solar Prominences, Algorithms, Images, Imaging Techniques, Sun

Scientific paper

Initial algorithms were developed to recognize two very different types
of features in solar images: H alpha filaments and large scale magnetic
field patterns. These algorithms provide an effective way to evaluate
possibilities for future routine, automated image analysis of large
numbers of solar images.

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