On the relationship between sunspot structure and magnetic field changes associated with solar flares
Yongliang Song, Mei Zhang

TL;DR
This study demonstrates a strong correlation between sunspot structural changes and magnetic field variations during solar flares, suggesting they are interconnected phenomena driven by the same underlying processes.
Contribution
It reveals a high correlation between sunspot structure and magnetic field changes during flares and extends this understanding to quiescent regions through observations and simulations.
Findings
Correlation coefficients between magnetic field and sunspot intensity exceed 0.90.
Sunspot structure and magnetic field changes are closely linked during flares.
Sunspot intensity correlates with horizontal magnetic field strength even in quiescent regions.
Abstract
Many previous studies have shown that magnetic fields as well as sunspot structures present rapid and irreversible changes associated with solar flares. In this paper we first use five X-class flares observed by SDO/HMI to show that not only the magnetic fields and sunspot structures do show rapid, irreversible changes but also these changes are closely related, both spatially and temporally. The magnitudes of the correlation coefficients between the temporal variations of horizontal magnetic field and sunspot intensity are all larger than 0.90, with a maximum value of 0.99 and an average value of 0.96. Then using four active regions in quiescent times, three observed and one simulated, we show that in sunspot penumbra regions there also exists a close correlation between sunspot intensity and horizontal magnetic field strength, in addition to the well-known one between sunspot…
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