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Cited article:

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Doppler shifts of spectral lines formed in the solar transition region and corona

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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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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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ARE INTERNETWORK MAGNETIC FIELDS IN THE SOLAR PHOTOSPHERE HORIZONTAL OR VERTICAL?

B. W. Lites, M. Rempel, J. M. Borrero and S. Danilovic
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