Coronal holes and icosahedral symmetry. I - Icosahedral coordinates

Details Coronal holes and icosahedral symmetry. I - Icosahedral coordinates Coronal holes and icosahedral symmetry. I - Icosahedral coordinates

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115..161n&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 115, no. 1, 1988, p. 161-169. DFG-supported research.

Physics

2

Coronal Holes, Icosahedrons, Mass Flow, Solar Magnetic Field, Magnetohydrodynamics, Symmetry

Scientific paper

A new type of coordinate to describe the mass outflow out of coronal holes is proposed which assumes symmetry under the icosahedral group I3. The present method takes into account the interaction between neighboring holes or flux tubes. It is demonstrated that the symmetry properties of Coxeter (1948) groups can effectively model symmetrical outflows. The transformation equations between the different coordinate systems are derived.

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