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On the fine structure of sunspot penumbrae

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Physical Properties of the Solar Magnetic Photosphere under the MISMA Hypothesis. III. Sunspot at Disk Center

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The Origin and Dynamics of Solar Magnetism

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Disintegration of Magnetic Flux in Decaying Sunspots as Observed with theHinodeSOT

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Formation of Moving Magnetic Features and Penumbral Magnetic Fields with Hinode/SOT

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Vector Magnetic Fields of Moving Magnetic Features and Flux Removal from a Sunspot

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A Study of the Hinode Observations of the Bipolar Moving Magnetic Features in Sunspot Penumbrae

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SST/CRISP observations of convective flows in a sunspot penumbra

G. B. Scharmer and V. M. J. Henriques
Astronomy & Astrophysics 540 A19 (2012)
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Azimuthal variations of magnetic field strength and inclination on penumbral boundaries

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RAPID TRANSITION OF UNCOMBED PENUMBRAE TO FACULAE DURING LARGE FLARES

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Recent Evidence for Convection in Sunspot Penumbrae

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

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The formation of a penumbra as observed with the German VTT and SoHO/MDI

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High-frequency oscillations in a solar active region observed with the RAPID DUAL IMAGER

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The flow field in the sunspot canopy

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Temporal evolution of the Evershed flow in sunspots

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Evershed flow observed in neutral and singly ionized iron lines

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Restoring Process of Sunspot Penumbra

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A distinct magnetic property of the inner penumbral boundary

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Robust method for determination of magnetic field strength in solar photosphere

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Magnetic fields of opposite polarity in sunspot penumbrae

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PROPERTIES OF SUPERSONIC EVERSHED DOWNFLOWS

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Fine Structure in Sunspots

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Polarimetry of sunspot penumbrae with high spatial resolution

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Spectropolarimetry of a sunspot at disk centre

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Asymmetrical appearance of dark-cored filaments in sunspot penumbrae

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Two magnetic components in sunspot penumbrae

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On the heat transport in a sunspot penumbra

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Three dimensional structure of a regular sunspot from the inversion of IR Stokes profiles

S. K. Mathew, A. Lagg, S. K. Solanki, et al.
Astronomy & Astrophysics 410 (2) 695 (2003)
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Observations of dark-cored filaments in sunspot penumbrae

K. Langhans, G. B. Scharmer, D. Kiselman and M. G. Löfdahl
Astronomy & Astrophysics 464 (2) 763 (2007)
DOI: 10.1051/0004-6361:20065215
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A 3D sunspot model derived from an inversion of spectropolarimetric observations and its implications for the penumbral heating

C. Beck
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Center-to-limb Variation of the Inverse Evershed Flow

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On the fine structure of sunspot penumbrae

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Robust Method for Determination of Magnetic Field Strength in the Solar Photosphere

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Astrophysics in 2003

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On the relation between penumbral intensity and flow filaments

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Astronomische Nachrichten 326 (3-4) 301 (2005)
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Sunspots: From Small-Scale Inhomogeneities Towards a Global Theory

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Magnetic Coupling between the Interior and Atmosphere of the Sun

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Magnetic Coupling between the Interior and Atmosphere of the Sun

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Magnetic Coupling between the Interior and Atmosphere of the Sun

J. Sánchez Almeida
Astrophysics and Space Science Proceedings, Magnetic Coupling between the Interior and Atmosphere of the Sun 210 (2010)
DOI: 10.1007/978-3-642-02859-5_16
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Magnetic Coupling between the Interior and Atmosphere of the Sun

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Astrophysics and Space Science Proceedings, Magnetic Coupling between the Interior and Atmosphere of the Sun 193 (2010)
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Magnetic Properties and Flow Angle of the Inverse Evershed Flow at Its Downflow Points

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The Astrophysical Journal 874 (1) 6 (2019)
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Vertical current densities and magnetic gradients in sunspots

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Modeling the Subsurface Structure of Sunspots

H. Moradi, C. Baldner, A. C. Birch, et al.
Solar Physics 267 (1) 1 (2010)
DOI: 10.1007/s11207-010-9630-4
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PRECURSOR OF SUNSPOT PENUMBRAL FORMATION DISCOVERED WITH HINODE SOLAR OPTICAL TELESCOPE OBSERVATIONS

Toshifumi Shimizu, Kiyoshi Ichimoto and Yoshinori Suematsu
The Astrophysical Journal 747 (2) L18 (2012)
DOI: 10.1088/2041-8205/747/2/L18
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EXPLANATION OF THE SEA-SERPENT MAGNETIC STRUCTURE OF SUNSPOT PENUMBRAE

I. N. Kitiashvili, L. R. Bellot Rubio, A. G. Kosovichev, et al.
The Astrophysical Journal 716 (2) L181 (2010)
DOI: 10.1088/2041-8205/716/2/L181
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