On the nature of photospheric magnetic fields beneath large coronal holes

Details On the nature of photospheric magnetic fields beneath large coronal holes On the nature of photospheric magnetic fields beneath large coronal holes

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...55...83f&link_type=abstract

Solar Physics, vol. 55, Nov. 1977, p. 83-97.

Physics

1

Magnetic Field Configurations, Solar Corona, Solar Magnetic Field, Astronomical Models, Field Theory (Physics), Photosphere, Solar Physics, Solar Wind, Stellar Envelopes

Scientific paper

Proposed mechanisms for the formation of coronal holes are considered; the crucial issue appears to be whether the holes are permeated by rigidly rotating fields. It is suggested that the interaction between such a field and the differentially rotating, diffusive solar envelope will produce a fore aft asymmetry in the distribution of fields which emerge to the photosphere. An initial study is carried out in the context of an illustrative example, and the results indicate that the asymmetry may be observed for a certain range of parameters involving the properties of the solar envelope and the characteristic size of the emerging field pattern.

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