Radio and soft X-ray evidence for dense non-potential magnetic flux tubes in the solar corona

Details Radio and soft X-ray evidence for dense non-potential magnetic flux tubes in the solar corona Radio and soft X-ray evidence for dense non-potential magnetic flux tubes in the solar corona

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...55..111s&link_type=abstract

Solar Physics, vol. 55, Nov. 1977, p. 111-120.

Physics

17

Magnetic Field Configurations, Magnetic Flux, Solar Corona, Solar Radio Bursts, Astronomical Maps, Potential Fields, Stellar Models

Scientific paper

The source positions of solar radio bursts of spectral types I, III(U) and III(J) and V observed by the Culgoora radioheliograph are found to lie almost radially above soft X-ray loops on pictures taken by the S-056 telescope aboard Skylab. The radio source positions and the X-ray loops occur near magnetic loops on computed potential field maps. However, the magnetic induction required to explain the radio observations is much greater than the computed potential field value at that height. Dense current-carrying magnetic flux tubes emanating from active regions on the Sun and extending to somewhat less than 1.5 solar radii above the photosphere provide a satisfactory model for the radio bursts.

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