Author name code: balke ADS astronomy entries on 2022-09-14 author:"Balke, A. Christiaan" ------------------------------------------------------------------------ Title: Percolation theory and the geometry of photospheric magnetic flux concentrations Authors: Balke, A. C.; Schrijver, C. J.; Zwaan, C.; Tarbell, T. D. Bibcode: 1993SoPh..143..215B Altcode: The magnetic field in solar active regions forms a highly structured pattern without an apparent length scale. We study this pattern in detail for a plage and its surroundings observed with the Swedish Solar Observatory on La Palma. The magnetogram has a resolution of about 1/3″, after image optimisation. We analysed the geometric properties of isolated patches of magnetic flux. Patches with a linear size up to 3″ appear to be statistically self-similar, with a fractal dimension ofDf = 1.54 ± 0.05 for the relation between area and linear size. This value agrees very well with the dimensionDf = 1.56 which is found in percolation theory for clusters of tracers placed randomly on a lattice with a tracer density below a critical threshold. The distribution of observed cluster areas also agrees with that of clusters on such a random lattice. The correspondence between properties of observations and of clusters on randomly filled lattices suggests that- well after emergence - the magnetic flux on the Sun is randomly distributed at least up to sizes of about 3″ and possibly larger. Title: Patterns in the photospheric magnetic field and percolation theory Authors: Schrijver, C. J.; Zwaan, C.; Balke, A. C.; Tarbell, T. D.; Lawrence, J. K. Bibcode: 1992A&A...253L...1S Altcode: The magnetic field in solar plages forms a highly structured pattern with no apparent characteristic length scale. This pattern appears to be a fractal with a dimension between 1.45 and 1.60. Small-scale displacements of concentrations of magnetic flux in the network are consistent with a random walk on a fractal with a similar dimension. Percolation theory offers an effective explanation for observed geometric properties of small-scale flux concentrations in the solar photosphere, by demonstrating the close correspondence with clusters formed by randomly placed tracers on a 2D (irregular) lattice. Percolation theory also offers a model for the subdiffusive behavior of tracers performing a random walk on clusters formed by bonded sites. The geometry of flux concentrations and of the displacement of magnetic flux as a function of time are equivalent to situations in percolation theory below a critical value, called 'the percolation threshold'. Title: Fractals in Magnetograms Authors: Schrijver, C. J.; Zwaan, C.; Balke, A. C.; Tarbell, T. D.; Lawrence, J. K. Bibcode: 1992ASPC...27...67S Altcode: 1992socy.work...67S No abstract at ADS Title: Short Term Evolution of Fine Scale Magnetic Structures Authors: Topka, K.; Frank, Z.; Shine, R.; Tarbell, T.; Title, A.; Scharmer, G.; Balke, A. Bibcode: 1989BAAS...21..842T Altcode: No abstract at ADS