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Application of a magnetograph and X-ray telescope to the study of coronal structure variationsThe application of magnetographs and X-ray imaging techniques to determine the magnitude, structure, origin, and evolution of the solar coronal magnetic field is examined. The spatial and temporal resolution of the X-ray telescope is discussed and a comparison of ground based magnetogram sequences versus a magnetograph in space is presented. Skylab photographs of the evolution of transient coronal holes are provided.
Document ID
19800009701
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Rust, D. M.
(American Science and Engineering, Inc. Cambridge, MA, United States)
Date Acquired
August 10, 2013
Publication Date
February 1, 1980
Publication Information
Publication: NASA. Goddard Space Flight Center Study of the Solar Cycle from Space
Subject Category
Solar Physics
Accession Number
80N17963
Funding Number(s)
CONTRACT_GRANT: NAS8-27758
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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