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Cited article:

The magnetic fine structure of the Sun’s polar region as revealed by Sunrise

A. Prabhu, A. Lagg, J. Hirzberger and S. K. Solanki
Astronomy & Astrophysics 644 A86 (2020)
https://doi.org/10.1051/0004-6361/202038704

Solar Faculae: Microturbulence as an Indicator of Inclined Magnetic Fields

M. I. Stodilka and R. I. Kostyk
Kinematics and Physics of Celestial Bodies 36 (4) 153 (2020)
https://doi.org/10.3103/S0884591320040054

Solar faculae: microturbulence as an indicator of inclined magnetic fields

M.I. Stodilka and R.I. Kostyk
Kinematika i fizika nebesnyh tel (Online) 36 (4) 3 (2020)
https://doi.org/10.15407/kfnt2020.04.003

The Formation of a Sunspot Penumbra Sector in Active Region NOAA 12574

Qiaoling Li, Xiaoli Yan, Jincheng Wang, DeFang Kong, Zhike Xue, Liheng Yang and Wenda Cao
The Astrophysical Journal 857 (1) 21 (2018)
https://doi.org/10.3847/1538-4357/aab6b0

Solar polarimetry through the K i lines at 770 nm

C. Quintero Noda, H. Uitenbroek, Y. Katsukawa, et al.
Monthly Notices of the Royal Astronomical Society 470 (2) 1453 (2017)
https://doi.org/10.1093/mnras/stx1344

FORMATION OF THE PENUMBRA AND START OF THE EVERSHED FLOW

M. Murabito, P. Romano, S. L. Guglielmino, F. Zuccarello and S. K. Solanki
The Astrophysical Journal 825 (1) 75 (2016)
https://doi.org/10.3847/0004-637X/825/1/75

Properties of solar plage from a spatially coupled inversion of Hinode SP data

D. Buehler, A. Lagg, S. K. Solanki and M. van Noort
Astronomy & Astrophysics 576 A27 (2015)
https://doi.org/10.1051/0004-6361/201424970

Opposite polarity field with convective downflow and its relation to magnetic spines in a sunspot penumbra

G. B. Scharmer, J. de la Cruz Rodriguez, P. Sütterlin and V. M. J. Henriques
Astronomy & Astrophysics 553 A63 (2013)
https://doi.org/10.1051/0004-6361/201220899

ANALYSIS OF QUIET-SUN INTERNETWORK MAGNETIC FIELDS BASED ON LINEAR POLARIZATION SIGNALS

D. Orozco Suárez and L. R. Bellot Rubio
The Astrophysical Journal 751 (1) 2 (2012)
https://doi.org/10.1088/0004-637X/751/1/2

Evolution of Active and Polar Photospheric Magnetic Fields During the Rise of Cycle 24 Compared to Previous Cycles

G. J. D. Petrie
Solar Physics 281 (2) 577 (2012)
https://doi.org/10.1007/s11207-012-0117-3