Application of a magnetograph and X-ray telescope to the study of coronal structure variations

Details Application of a magnetograph and X-ray telescope to the study of coronal structure variations Application of a magnetograph and X-ray telescope to the study of coronal structure variations

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980sscs.nasa..259r&link_type=abstract

In NASA. Goddard Space Flight Center Study of the Solar Cycle from Space p 259-263 (SEE N80-17944 08-92)

Physics

Solar Corona, Solar Magnetic Field, X Ray Telescopes, Solar Physics, Solar X-Rays, X Ray Imagery

Scientific paper

The 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.

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