Charnotskii Mikhail
J Opt Soc Am A Opt Image Sci Vis. 2019 Aug 1;36(8):1440-1446. doi: 10.1364/JOSAA.36.001440.
Following the development of the companion paper [J. Opt. Soc. Am.36, 1433 (2019)JOAOD60740-323210.1364/JOSAA.36.00XXXX], 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.
继配套论文[《美国光学学会杂志》36, 1433 (2019)JOAOD60740 - 323210.1364/JOSAA.36.00XXXX]发表之后,通过将非相干单极子和偶极子源放置在一个球形球体内以及一个圆形平面盘上,构建了准单色光相干性的其他模型。对太阳光有效的傍轴近似将不同模型的数量从八个减少到三个。基于与这三个模型对应的太阳图像,球形模型被认为是最合适的。球形模型可以进行修改以匹配临边昏暗观测结果。