Tracking of magnetic flux concentrations over a five-day observation and an insight into surface magnetic flux transport

TL;DR

This study analyzes magnetic flux transport on the solar surface over five days, revealing scale-dependent super-diffusive and sub-diffusive behaviors that differ from classical diffusion, providing insights into magnetic flux dynamics.

Contribution

It presents the longest satellite observation of magnetic flux transport, identifying a power-law dependence and a transition in diffusion regimes at a specific spatial scale.

Findings

Super-diffusion with an index of 1.4 on small scales

Sub-diffusion with an index of 0.6 on larger scales

Transport behavior differs significantly from classical diffusion

Abstract

The solar dynamo problem is the question of how the cyclic variation in the solar magnetic field is maintained. One of the important processes is the transport of magnetic flux by surface convection. To reveal this process, the dependence of the squared displacement of magnetic flux concentrations upon the elapsed time is investigated in this paper via a feature-recognition technique and a continual five-day magnetogram. This represents the longest time scale over which a satellite observation has ever been performed for this problem. The dependence is found to follow a power-law and differ significantly from that of diffusion transport. Furthermore there is a change in the behavior at a spatial scale of 10^{3.8} km. A super-diffusion behavior with an index of 1.4 is found on smaller scales, while changing to a sub-diffusion behavior with an index of 0.6 on larger ones. I interpret this difference in the transport regime as coming from the network-flow pattern.