3D Modeling of the solar corona in different stages of the solar magnetic cycle over the period 1870 to 1991

Details 3D Modeling of the solar corona in different stages of the solar magnetic cycle over the period 1870 to 1991 3D Modeling of the solar corona in different stages of the solar magnetic cycle over the period 1870 to 1991

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..849m&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 10, pp.849-853

Physics

Scientific paper

Three-dimensional (3D) modeling of the solar corona has been carried out on the basis of the magnetic field distribution on H-alpha charts for the epochs of solar eclipses that occur near the epoch of the polar magnetic field reversal. Analysis of the 3D modeling shows that:
1.
Besides the global neutral sheet, two high-latitude coronal neutral sheets are also observed during the epoch of the polar magnetic field reversal.
2.
The observed structure of the coronal streamers is due to a projection of the folds of corrugated neutral sheets on the picture plane rather than due to the peculiar configuration of the magnetic field lines.

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