The solar photospheric continuum brightness as a function of mean magnetic flux density. I. The role of the magnetic structure size distribution

Peck, C. L., M. P. Rast, S. Criscuoli, and M. Rempel, 2019: The solar photospheric continuum brightness as a function of mean magnetic flux density. I. The role of the magnetic structure size distribution. The Astrophysical Journal, 870, 89, doi:10.3847/1538-4357/aaf289.

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Published Version: http://dx.doi.org/10.3847/1538-4357/aaf289

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