Topological structure of coronal-interplanetary magnetic field

Details Topological structure of coronal-interplanetary magnetic field Topological structure of coronal-interplanetary magnetic field

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...56..439y&link_type=abstract

Solar Physics, vol. 56, Feb. 1978, p. 439-447.

Physics

3

Interplanetary Magnetic Fields, Lines Of Force, Magnetic Field Configurations, Solar Corona, Current Sheets, Electric Current, Topology

Scientific paper

The topological structure of the coronal-interplanetary magnetic field is determined by the arrangement of the neutral lines at the coronal base. It is characterized by nested separatrices, which are interfaces between closed and open field lines or between oppositely directed open field lines, in the coronal-interplanetary space. In the neighborhoods of these separatrices there are important electric currents. These currents form the basis for the sheet-current model.

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