Coronal holes with a saddle structure as deduced from Yohkoh observations

Details Coronal holes with a saddle structure as deduced from Yohkoh observations Coronal holes with a saddle structure as deduced from Yohkoh observations

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..854f&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 10, pp.854-856

Physics

Scientific paper

Saddle structures are seen in some images of the Sun in the soft X-rays obtained by Yohkoh mission. At the center of any such structure, there is a small coronal hole having the outlines of an astroid or a cross. The coronal saddles occur in magnetic configurations with a high degree of symmetry (quadrupoles). Comparison with the models shows that open field lines cannot be modeled using only the source surface.

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