Interaction between two flux ropes immersed in the solar atmosphere

Details Interaction between two flux ropes immersed in the solar atmosphere Interaction between two flux ropes immersed in the solar atmosphere

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...328..954y&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 328, May 15, 1988, p. 954-966.

Other

2

Magnetic Flux, Solar Atmosphere, Solar Corona, Solar Magnetic Field, Sunspots, Bipolarity, Perturbation Theory, Solar Activity, Solar Flares, Solar Gravitation

Scientific paper

The interaction between two flux ropes immersed in a magnetized medium is studied. The method of images is used to calculate the diamagnetic buoyancy force exerted by this interaction on an individual flux rope. The results show that the presence of an external magnetic field enables the ambient magnetic stress to give rise to an attractive force between the two legs of a bipolar arch in the lower solar corona. This provides a dynamical explanation for the photospheric observation that two magnetic features of opposite polarities can move toward each other.

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