Context. While it is conjectured that a chromospheric canopy plays a role in penumbra formation, it has been difficult to find observational evidence of the connectivity between the …
We studied the variations of line of sight photospheric plasma flows during the formation phase of the penumbra around a pore in active region NOAA 11490. We used a high spatial …
We studied the formation of the first penumbral sector around a pore in the following polarity of the NOAA Active Region (AR) 11490. We used a high spatial, spectral, and temporal …
We investigate whether flux cancellation is responsible for the formation of a very massive filament resulting in the spectacular eruption on 2011 June 7. We analyze and quantify the …
J Jurčák, NB González, R Schlichenmaier… - Astronomy & …, 2017 - aanda.org
Context. We recently presented evidence that stable umbra-penumbra boundaries are characterised by a distinct canonical value of the vertical component of the magnetic field, B …
M García-Rivas, J Jurčák, NB González… - Astronomy & …, 2024 - aanda.org
Context. Fully fledged penumbrae have been widely studied both observationally and theoretically. Yet the relatively fast process of penumbra formation has not been studied …
P Lindner, R Schlichenmaier, NB González… - Astronomy & …, 2023 - aanda.org
Context. The intermediate stages between pores and the formation of sunspots are a rare phenomenon and can be manifested as transient photospheric penumbral-like filaments …
S Idrees, J Su, J Chen, Y Deng - Solar Physics, 2024 - Springer
In this study, we investigate the decay of sunspots in the active region NOAA 13229 using data from the ASO-S/FMG and SDO/HMI. We closely examine the decay patterns of …
B Löptien, A Lagg, M van Noort, SK Solanki - Astronomy & Astrophysics, 2020 - aanda.org
Context. It has been reported that the boundary between the umbra and the penumbra of sunspots occurs at a canonical value of the strength of the vertical magnetic field …