The horizontal advection speed of solar magnetic flux decreases smoothly with increasing vertical field strength, from roughly 110 m/s at 150 G to 10 m/s at 2500 G, and is fit by a fourth-degree polynomial.
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Quantifying Suppression of Solar Surface Magnetic Flux Advection with Increasing Field Strength
The horizontal advection speed of solar magnetic flux decreases smoothly with increasing vertical field strength, from roughly 110 m/s at 150 G to 10 m/s at 2500 G, and is fit by a fourth-degree polynomial.