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Cited article:

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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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Structure of the Long-Living Elements of Solar Granulation

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The Small-scale Structure of Photospheric Convection Retrieved by a Deconvolution Technique Applied to Hinode/SP Data

T. Oba, T. L. Riethmüller, S. K. Solanki, Y. Iida, C. Quintero Noda and T. Shimizu
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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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Influence of magnetic field on propagation of five-minute oscillations in the sun’s atmosphere: Phase shifts

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The dynamics of the observed solar granulation: spatio-temporal variations of line of sight velocity and thermodynamic parameters

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Specifics of the solar photospheric convection at granulation, mesogranulation, and supergranulation scales

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