Rosseland mean opacity

E46432

Rosseland mean opacity is an average measure of a material’s opacity weighted toward frequencies where radiation is most effectively transported, widely used in stellar and astrophysical radiative transfer calculations.

AI illustration

How this image was made

AI-generated illustration of Rosseland mean opacity

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of Rosseland mean opacity (Rosseland mean opacity is an average measure of a material’s opacity weighted toward frequencies where radiation is most effectively transported, widely used in stellar and astrophysical radiative transfer calculations.)

All labels observed (2)

Label Occurrences
Rosseland mean opacity canonical 5
Rosseland mean opacities 1

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf astrophysical opacity measure ⓘ
mean opacity ⓘ
radiative transfer quantity ⓘ
appliesTo continuum opacity ⓘ
line opacity ensembles ⓘ
assumes diffusion approximation for radiative transfer ⓘ
local thermodynamic equilibrium ⓘ
optically thick medium ⓘ
characteristic emphasizes frequency ranges where radiation diffuses most efficiently ⓘ
contrastsWith Planck mean opacity weighting by Planck function itself ⓘ
dependsOn chemical composition ⓘ
density ⓘ
frequency-dependent opacity ⓘ
ionization state ⓘ
temperature ⓘ
domain astrophysics ⓘ
plasma physics ⓘ
radiative transfer theory ⓘ
stellar astrophysics ⓘ
introducedBy Svein Rosseland ⓘ
introducedIn 20th century ⓘ
mathematicalDefinition harmonic mean of monochromatic opacity weighted by derivative of Planck function with respect to temperature ⓘ
namedAfter Svein Rosseland ⓘ
relatedTo OP opacity project ⓘ
OPAL opacity project ⓘ
Planck mean opacity ⓘ
equation of radiative transfer ⓘ
flux-mean opacity ⓘ
monochromatic opacity ⓘ
radiation pressure ⓘ
radiative diffusion approximation ⓘ
radiative energy transport ⓘ
stellar opacity tables ⓘ
roleInModels controls radiative energy flux for given temperature gradient ⓘ
symbol kappa_R ⓘ
unit square meter per kilogram ⓘ
usedFor computing radiative temperature gradient in stars ⓘ
determining convective stability criteria ⓘ
estimating radiative conductivity ⓘ
modeling energy transport in stellar interiors ⓘ
usedIn accretion disk models ⓘ
astrophysical radiative transfer ⓘ
interior models of stars ⓘ
radiation hydrodynamics ⓘ
stellar atmosphere modeling ⓘ
stellar evolution models ⓘ
stellar structure calculations ⓘ
weightingFunction dB_nu_dT ⓘ

How these facts were elicited

Referenced by (6)

Full triples — surface form annotated when it differs from this entity's canonical label.

Radiative Transfer → relatedConcept → Rosseland mean opacity ⓘ
Svein Rosseland → knownFor → Rosseland mean opacity ⓘ
Svein Rosseland → hasEponym → Rosseland mean opacity ⓘ
Svein Rosseland → notableConcept → Rosseland mean opacity ⓘ
OP opacity project → computes → Rosseland mean opacities ⓘ
linked to: Rosseland mean opacity
Kramers opacity law → relatedTo → Rosseland mean opacity ⓘ