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Cited article:

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Understanding the heating mechanism of the solar active region atmosphere in chromosphere

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https://doi.org/10.1088/1742-6596/2544/1/012006

Magnetic Properties and Flow Angle of the Inverse Evershed Flow at Its Downflow Points

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The Magnetic Response of the Solar Atmosphere to Umbral Flashes

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A Hot Downflowing Model Atmosphere for Umbral Flashes and the Physical Properties of Their Dark Fibrils

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A New MHD-assisted Stokes Inversion Technique

T. L. Riethmüller, S. K. Solanki, P. Barthol, A. Gandorfer, L. Gizon, J. Hirzberger, M. van Noort, J. Blanco Rodríguez, J. C. Del Toro Iniesta, D. Orozco Suárez, W. Schmidt, V. Martínez Pillet and M. Knölker
The Astrophysical Journal Supplement Series 229 (1) 16 (2017)
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THE APPEARANCE OF SPICULES IN HIGH RESOLUTION OBSERVATIONS OF Ca ii H AND Hα

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Evidence of quiet-Sun chromospheric activity related to an emerging small-scale magnetic loop

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Astronomy & Astrophysics 556 A7 (2013)
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Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations

C. Beck, D. Fabbian, F. Moreno-Insertis, K. G. Puschmann and R. Rezaei
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THE FORMATION OFIRISDIAGNOSTICS. III. NEAR-ULTRAVIOLET SPECTRA AND IMAGES

T. M. D. Pereira, J. Leenaarts, B. De Pontieu, M. Carlsson and H. Uitenbroek
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https://doi.org/10.1088/0004-637X/778/2/143