Frozen-in Fractals All Around: Inferring the Large Scale Effects of Small-Scale Magnetic Structure
R. T. James McAteer

TL;DR
This paper introduces a multifractal spectrum approach to analyze solar magnetic fields, linking small-scale magnetic structures to large-scale solar eruptions, and proposes a method for predicting solar flare activity.
Contribution
It presents a novel application of multifractal spectrum analysis to connect photospheric magnetic gradients with large-scale solar eruptive phenomena.
Findings
Multifractal spectra are independent of data type and quality.
Quiet-Sun magnetic gradients do not persist over time.
Large-scale current density structures are linked to energy storage for eruptions.
Abstract
The large-scale structure of the magnetic field in the solar corona provides the energy to power large-scale solar eruptive events. Our physical understanding of this structure, and hence our ability to predict these events, is limited by the type of data currently available. It is shown that the multifractal spectrum is a powerful tool to study this structure, by providing a physical connection between the details of photospheric magnetic gradients and current density at all size scales. This uses concepts associated with geometric measure theory and the theory of weakly differentiable functions to compare Amp\`{e}re's law to the wavelet-transform modulus maximum method. The H\"{o}lder exponent provides a direct measure of the rate of change of current density across spatial size scales. As this measure is independent of many features of the data (pixel resolution, data size, data…
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