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Cited article:

Non-local thermodynamic equilibrium inversions of the Si I 10827 Å spectral line

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Accurate and experimentally validated transition data for Si I and Si II

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Measurements of Photospheric and Chromospheric Magnetic Field Structures Associated with Chromospheric Heating over a Solar Plage Region

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Velocity Field Diagnostics of the Quiet Sun Using the Lambda-Meter Method: Si I 1082.7 nm Line

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Kinematics and Physics of Celestial Bodies 36 (1) 1 (2020)
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Evolution of Stokes V area asymmetry related to a quiet Sun cancellation observed with GRIS/IFU

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Tracking Downflows from the Chromosphere to the Photosphere in a Solar Arch Filament System

Sergio Javier González Manrique, Christoph Kuckein, Adur Pastor Yabar, Andrea Diercke, Manuel Collados, Peter Gömöry, Sihui Zhong, Yijun Hou and Carsten Denker
The Astrophysical Journal 890 (1) 82 (2020)
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Capabilities of bisector analysis of the Si I 10 827 Å line for estimating line-of-sight velocities in the quiet Sun

S. J. González Manrique, C. Quintero Noda, C. Kuckein, B. Ruiz Cobo and M. Carlsson
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Diagnostics of the velocity field of the quiet Sun using the lambda-meter method: The Si I  1082.7 nm line

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Kinematika i fizika nebesnyh tel (Online) 36 (1) 3 (2020)
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Magnetic fields and thermodynamic conditions in the pre-peak phase of M6.4 / 3N solar flare

V. Lozitsky and M. Stodilka
Bulletin of Taras Shevchenko National University of Kyiv. Astronomy (59) 20 (2019)
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The diagnostic potential of the weak field approximation for investigating the quiet Sun magnetism: the Si I 10 827 Å line

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Astronomy & Astrophysics 628 A47 (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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Detection of emission in the Si I 1082.7 nm line core in sunspot umbrae

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Astronomy & Astrophysics 607 A102 (2017)
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