Development of a complex of activity in the solar corona

Details Development of a complex of activity in the solar corona Development of a complex of activity in the solar corona

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...54...65h&link_type=abstract

Solar Physics, vol. 54, Sept. 1977, p. 65-105.

Physics

47

Solar Activity, Solar Corona, Lines Of Force, Photosphere, Skylab Program, Solar Magnetic Field, Solar X-Rays

Scientific paper

Using Skylab observations of soft solar X-rays, the development of a complex of activity in the solar corona during its whole lifetime of seven solar rotations is studied. The basic components of the activity complex were determined to be permanently interconnected through sets of magnetic field lines, which suggests similar connections also below the photosphere. The visibility of individual loops in these connections, however, was greatly variable and typically shorter than one day. Each brightening of a coronal loop in X-rays seems to be related to a variation in the photospheric magnetic field near its footprint.

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