Astron. Astrophys. 332, 1075-1081 (1998)

An approximate self-consistent theory of the magnetic field of fluted penumbrae

T. Neukirch ¹ and P.C.H. Martens <sup>2

1</sup> School of Mathematical and Computational Sciences, University of St. Andrews, St. Andrews, KY16 9SS, UK (e-mail: thomas@dcs.st-and.ac.uk)
² Space Science Department of ESA at Goddard Space Flight Center, Code 682.3, NASA/GSFC, Greenbelt, MD 20771, USA (e-mail: pmartens@esa.nascom.nasa.gov)

Received 21 November 1997 / Accepted 13 January 1998

Abstract

A self-consistent mathematical description of the magnetic field of fluted sunspot penumbrae is presented. This description is based on an expansion of the nonlinear force-free magnetohydrostatic equations written in cylindrical coordinates. The lowest order solutions are mathematically equivalent to laminated force-free equilibria in Cartesian geometry. The lowest order solutions have no toroidal component of the magnetic field and the magnetic pressure does not vary with azimuth but the solutions allow arbitrary variations of the magnetic field components with azimuth. Explicit solutions are presented which have a realistic radial profile of the magnetic field strength and reproduce the basic features of the observations.

Key words: sunspots Sun: magnetic fields MHD methods: analytical

Send offprint requests to: T. Neukirch

© European Southern Observatory (ESO) 1998

Online publication: March 30, 1998
helpdesk@link.springer.de