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Paper: Magnetic Flux Emergence on Different Scales
Volume: 415, The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding
Page: 167
Authors: Hagenaar, M.; Cheung, M.
Abstract: Magnetic flux emerges on the Sun on many different scales, from weak intranetwork to network concentrations and (ephemeral) active regions. Methods previously developed to recognize regions of magnetic emergence on MDI Full Disk magnetograms fail when applied to Hinode/SOT Stokes maps: the resolution is so much higher that simple bipoles on MDI are observed as collections of fragments. We present a new method for the automatic detection and characterization of flux emergence on a range of scales.
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