Modelling of a solar coronal loop.

Details Modelling of a solar coronal loop. Modelling of a solar coronal loop.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jplph..56..427k&link_type=abstract

Journal of Plasma Physics, Vol. 56, p. 427 - 440

Physics

Plasma Physics

4

Solar Coronal Loops: Models, Solar Coronal Loops: Magnetohydrodynamics

Scientific paper

Montgomery and co-workers have developed a framework to describe the steady state of a turbulent magnetofluid, without the usual recourse to linearization. Thus the magnetic and velocity fields emerge in their fully nonlinear form as a consequence of the selective decays of the invariants of the system. Using this statistical theory of magnetohydrodynamic turbulence, the pressure, magnetic and flow fields of a solar coronal loop have been determined. The spatial and time profiles of the loop pressure are derived. A comparison with the observed properties of the loops is made, whenever possible.

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