Interplanetary magnetic clouds of toroidal shapes

Details Interplanetary magnetic clouds of toroidal shapes Interplanetary magnetic clouds of toroidal shapes

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..535r&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Physics

3

Magnetic Clouds, Force-Free Fields, Models

Scientific paper

Analytical solutions of force-free equation inside a toroid are derived for constant and non-constant alpha. They can be used for interpretation of solar flux ropes and interplanetary magnetic clouds. The solution with non-constant alpha is valid for arbitrary aspect ratio torus. Magnetic fiels inside toroids with low aspect ratios give very high ratios Bmax/Bmin > 10, while for high aspect ratios this value is about 2.

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