The Distribution of Quiet Sun Magnetic Field Strengths from 0 to 1800 G
The quiet-Sun photospheric plasma has a variety of magnetic field strengths going from zero to 1800 G. The empirical characterization of these field strengths requires a probability density function (PDF), i.e., a function P(B) describing the fraction of quiet Sun occupied by each field strength B. We show how to combine magnetic field strength
Domínguez Cerdeña, I. et al.
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2006