An integral on the shape of isolated magnetic loops

Details An integral on the shape of isolated magnetic loops An integral on the shape of isolated magnetic loops

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...259..296c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 259, no. 1, p. 296-300.

Astronomy and Astrophysics

Astrophysics

5

Integral Calculus, Magnetic Field Configurations, Magnetic Flux, Solar Magnetic Field, Equations Of State, Solar Atmosphere

Scientific paper

Stationary flows in isolated magnetic flux tubes are studied using the thin flux tube approximation method. Assuming that the external atmosphere is a plane-stratified fluid in hydrostatic equilibrium, an important integral is found, which is independent of the energy transfer mechanism and parameters of the ambient gas. Applying the integral, we obtain some theoretical results about the shape of isolated magnetic flux tubes and examine some numerical results of previous studies in this field. The applications of the integral to the solar atmosphere magnetic field are discussed briefly.

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