Abstract
Following the development of the companion paper [J. Opt. Soc. Am. 36, 1433 (2019) [CrossRef] ],
additional models for the coherence of quasi-monochromatic light are
constructed by placing incoherent monopole and dipole sources inside a
spherical ball and on a circular plane disk. The paraxial
approximation, which is valid for sunlight, reduces the number of
different models from eight to three. Based on the solar images
corresponding to these three models, the ball model is considered the
most appropriate. The ball model can be modified to match the
limb-darkening observations.
© 2019 Optical Society of
America
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