Lu and Hamilton model for solar flares over a rewiring complex network
Alejandro Zamorano, Laura Morales, Denisse Past\'en, V\'ictor Mu\~noz

TL;DR
This paper introduces a modified solar flare model using a rewiring complex network, revealing a transition from power-law to exponential energy distributions influenced by network rewiring, which affects the scale-free behavior.
Contribution
The study presents a novel network rewiring approach in a Lu & Hamilton-type model, capturing dynamic topological changes and their impact on energy distribution in solar flare simulations.
Findings
Rewiring causes the energy distribution to shift from power-law to exponential.
Increased rewiring probability leads to microflare-dominated, non-scale-free dynamics.
Topological neighbors induce intrinsically nonlocal system behavior.
Abstract
We present a modified Lu \& Hamilton-type model where the neighborhood relations are replaced by topological connections, which can be dynamically altered. The model represents each grid node as a flux tube, as in the classic model, but with connections evolving to capture the complex effects of magnetic reconnection. Through this framework, we analyze how the dissipated energy distribution changes, particularly focusing on the power-law exponent , which decreases with respect to the original model due to rewiring effects. When the system is dominated by rewiring, it presents an exponential distribution exponent , showing a faster decay of dissipated energy than in the original model. This leads to microflare-dominated dynamics at short timescales, causing the system to lose the scale-free behavior observed in both the original model (Lu \& Hamilton 1991) and in…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Statistical Mechanics and Entropy
