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Cited article:

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Solar faculae: microturbulence as an indicator of inclined magnetic fields

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Kinematika i fizika nebesnyh tel (Online) 36 (4) 3 (2020)
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Solar Faculae: Microturbulence as an Indicator of Inclined Magnetic Fields

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Intensity contrast of solar plage as a function of magnetic flux at high spatial resolution

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Astronomy & Astrophysics 621 A78 (2019)
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Features of Convection in the Atmospheric Layers of the Solar Facula

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Kinematics and Physics of Celestial Bodies 35 (6) 261 (2019)
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Robust method for determination of magnetic field strength in solar photosphere

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Kinematika i fizika nebesnyh tel (Online) 34 (6) 3 (2018)
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Robust Method for Determination of Magnetic Field Strength in the Solar Photosphere

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Diagnostics of the solar atmosphere by the Non-LTE inversion method: Line of Ba II λ 455.403 nm

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What mechanisms allow 5-minute oscillations in active regions of the solar surface to penetrate from the photosphere into the chromosphere?

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Influence of magnetic field on propagation of five-minute oscillations in the sun’s atmosphere: Phase shifts

R. I. Kostik, N. G. Shchukina, N. I. Kobanov and V. A. Pulyaev
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Multiple accretion events as a trigger for Sagittarius A* activity

D. Kunneriath, B. Czerny, V. Karas and T. K. Das
Proceedings of the International Astronomical Union 9 (S303) 320 (2013)
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COMPARISON OF PHYSICAL PROPERTIES OF QUIET AND ACTIVE REGIONS THROUGH THE ANALYSIS OF MAGNETOHYDRODYNAMIC SIMULATIONS OF THE SOLAR PHOTOSPHERE

S. Criscuoli
The Astrophysical Journal 778 (1) 27 (2013)
https://doi.org/10.1088/0004-637X/778/1/27