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  2. Optical depth (astrophysics) - Wikipedia

    en.wikipedia.org/wiki/Optical_depth_(astrophysics)

    Optical depth in astrophysics refers to a specific level of transparency. Optical depth and actual depth, τ {\displaystyle \tau } and z {\displaystyle z} respectively, can vary widely depending on the absorptivity of the astrophysical environment.

  3. Optical depth - Wikipedia

    en.wikipedia.org/wiki/Optical_depth

    In physics, optical depth or optical thickness is the natural logarithm of the ratio of incident to transmitted radiant power through a material. Thus, the larger the ...

  4. Category : Scattering, absorption and radiative transfer (optics)

    en.wikipedia.org/wiki/Category:Scattering...

    Optical depth (astrophysics) Optical properties of water and ice; Optical theorem; Oren–Nayar reflectance model; P. Penetration depth; Phase angle (astronomy)

  5. Category:Astrophysics - Wikipedia

    en.wikipedia.org/wiki/Category:Astrophysics

    Astrophysics is the branch of astronomy that deals with the physics of the universe, ... Optical depth (astrophysics) Osipkov–Merritt model; P. P-nuclei;

  6. Lambda-CDM model - Wikipedia

    en.wikipedia.org/wiki/Lambda-CDM_model

    The Planck collaboration version of the ΛCDM model is based on six parameters: baryon density parameter; dark matter density parameter; scalar spectral index; two parameters related to curvature fluctuation amplitude; and the probability that photons from the early universe will be scattered once on route (called reionization optical depth). [18]

  7. Gravitational microlensing - Wikipedia

    en.wikipedia.org/wiki/Gravitational_microlensing

    The density, mass, and location of the objects in these lens populations determines the frequency of microlensing along that line of sight, which is characterized by a value known as the optical depth due to microlensing. (This is not to be confused with the more common meaning of optical depth, although it shares some properties.) The optical ...

  8. Radiative transfer - Wikipedia

    en.wikipedia.org/wiki/Radiative_transfer

    Equations of radiative transfer have application in a wide variety of subjects including optics, astrophysics, atmospheric science, and remote sensing. Analytic solutions to the radiative transfer equation (RTE) exist for simple cases but for more realistic media, with complex multiple scattering effects, numerical methods are required.

  9. Solar radius - Wikipedia

    en.wikipedia.org/wiki/Solar_radius

    Solar radius is a unit of distance used to express the size of stars in astronomy relative to the Sun.The solar radius is usually defined as the radius to the layer in the Sun's photosphere where the optical depth equals 2/3: [1]