Class: EddingtonApproximation
http://www.astro.umd.edu/~eshaya/astro-ont/owl/astronomy.owl#EddingtonApproximation
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theory
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astronomyTheory
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stellarTheory
- EddingtonApproximation
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stellarTheory
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astronomyTheory
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astronomy
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astronomyTheory
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stellarTheory
- EddingtonApproximation
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stellarTheory
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astronomyTheory
Annotations
- definition: "The Eddington approximation can be used to obtain the intensity in a plane-parallel atmosphere with isotropic frequency-independent scattering. It assumes that the intensity is a linear function of μ = cosθ. i.e. Iν(μ,z) = a(z) + μb(z) where z is the normal direction to the slab atmosphere." (string)