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X-ray imaging of a filament eruption with the Solar Maximum Mission satelliteSoft X-ray observations of a filament located near NOAA AR 4640 were obtained with the Flat Crystal Spectrometer (FCS) on board the Solar Maximum Mission satellite on April 3-12, 1985. On April 7 the filament partially lifted off. At the same time and location an enhancement was imaged in soft X-rays. A total of 16 h of FCS observations, including 25 raster images, were made of the filament prior to the eruption, and over 40 h of observations, including 57 raster images, were made following the eruption. Careful alignment of H-alpha images taken during the same period has made possible the calculation of the integrated soft X-ray emission around the filament channel before, during, and after the eruption. Kitt Peak magnetograms have also been examined for this period to determine the corresponding magnetic field structure. A time history of the eruption in X-ray and optical wavelengths, and the development of the magnetic-field structure are presented. Evidence is seen for X-ray brightening in preexisting magnetic-field loops over the filament.
Document ID
19870052714
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Slater, G. L.
(Applied Research Corp. Landover, MD, United States)
Saba, J. L. R.
(Applied Research Corp. Landover, MD, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Publication Information
Publication: Advances in Space Research
Volume: 6
Issue: 6 19
ISSN: 0273-1177
Subject Category
Solar Physics
Accession Number
87A39988
Funding Number(s)
CONTRACT_GRANT: NAS5-23758
Distribution Limits
Public
Copyright
Other

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