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Application of digital image processing techniques to faint solar flare phenomenaDigital image processing of eight solar flare events was performed using the Video Information Communication and Retrieval language in order to study moving emission fronts, flare halos, and Moreton waves. The techniques used include contrast enhancement, isointensity contouring, the differencing of images, spatial filtering, and geometrical registration. The spatial extent and temporal behavior of the faint phenomena is examined along with the relation of the three types of phenomena to one another. The image processing techniques make possible the detailed study of the history of the phenomena and provide clues to their physical nature.
Document ID
19810041593
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Glackin, D. L.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Martin, S. F.
(San Fernando Observatory Sylmar, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1980
Subject Category
Solar Physics
Meeting Information
Meeting: Conference on Applications of Digital Image Processing to Astronomy
Location: Pasadena, CA
Start Date: August 20, 1980
End Date: August 22, 1980
Accession Number
81A25997
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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