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Cited article:

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The Sun’s Magnetic Power Spectra over Two Solar Cycles. I. Calibration between SDO/HMI and SOHO/MDI Magnetograms

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Can Small-scale Magnetic Fields Be the Major Cause for the Near-surface Effect of the Solar p-mode Frequencies?

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Analysis of quiet-sun turbulence on the basis of SDO/HMI and goode solar telescope data

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Monthly Notices of the Royal Astronomical Society 497 (4) 5405 (2020)

The Dimmest State of the Sun

K. L. Yeo, S. K. Solanki, N. A. Krivova, M. Rempel, L. S. Anusha, A. I. Shapiro, R. V. Tagirov and V. Witzke
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On the Contribution of Quiet-Sun Magnetism to Solar Irradiance Variations: Constraints on Quiet-Sun Variability and Grand-minimum Scenarios

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Achievements of Hinode in the first eleven years

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The Solar Photospheric Continuum Brightness as a Function of Mean Magnetic Flux Density. I. The Role of the Magnetic Structure Size Distribution

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Small-scale Dynamo Simulations: Magnetic Field Amplification in Exploding Granules and the Role of Deep and Shallow Recirculation

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B. W. Lites, M. Rempel, J. M. Borrero and S. Danilovic
The Astrophysical Journal 835 (1) 14 (2017)