Precursor of Sunspot Penumbral Formation discovered with Hinode SOT Observations
Toshifumi Shimizu, Kiyoshi Ichimoto, Yoshinori Suematsu

TL;DR
This study used Hinode SOT observations to identify an annular chromospheric zone around a pore that precedes sunspot penumbra formation, highlighting the role of magnetic canopy structures in this process.
Contribution
It reveals a previously unrecognized chromospheric precursor, the annular zone, indicating magnetic canopy formation before penumbra develops.
Findings
Annular zone appears before penumbra formation.
Magnetic canopy overlying the umbra is observed in the chromosphere.
No strong systematic flows detected in the annular zone.
Abstract
We present observations of a precursory signature that would be helpful for understanding the formation process of sunspot penumbrae. The Hinode Solar Optical Telescope successfully captured the entire evolution of a sunspot from the pore to a large well-developed sunspot with penumbra in an emerging flux region appeared in NOAA Active Region 11039. We found an annular zone (width 3"-5") surrounding the umbra (pore) in Ca II H images before the penumbra is formed around the umbra. The penumbra was developed as if to fill the annular zone. The annular zone shows weak magnetogram signals, meaning less magnetic flux or highly inclined fields there. Pre-existing ambient magnetic field islands were moved to be distributed at the outer edge of the annular zone and did not come into the zone. There is no strong systematic flow patterns in the zone, but we occasionally observed small magnetic…
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