isotropic

(adjective)

Having properties that are identical in all directions; exhibiting isotropy.

Related Terms

  • linear thermal expansion coefficient

Examples of isotropic in the following topics:

  • Emission

    • If the emitter is isotropic or the emitters are randomly oriented then the total power emitted per unit volume and unit frequency is
    • Often the emission is isotropic and it is convenient to define the emissivity of the material per unit mass
    • ϵν\epsilon_\nuϵ​ν​​ is simply related to jνj_\nuj​ν​​ for an isotropic emitter
  • Flux

    • For example, if you have an isotropic source, the flux is constant across a spherical surface centered on the source, so you find that
  • Eddington Approximation

    • In this region, the radiation field is nearly isotropic, but it need not be close to a blackbody distribution.
    • Because the intensity is close to isotropic we can approximate it by
    • which we found earlier to hold for strictly isotropic radiation fields.
    • The source function SνS_\nuS​ν​​ is isotropic, so let's average the radiative transfer equation over direction to yield
  • Volume Expansion

    • Such substances that expand in all directions are called isotropic.
    • For isotropic materials, the area and linear coefficients may be calculated from the volumetric coefficient (discussed below).
    • For isotropic material, and for small expansions, the linear thermal expansion coefficient is one third the volumetric coefficient.
  • A Physical Aside: Intensity and Flux

  • Energy Density

    • But let's assume that the radiation field is isotropic, so I=JI = JI=J for all directions, we get
  • Inverse Compton Scattering

    • If we assume that the photon distribution is isotropic, the angle ⟨cosθ⟩=0\langle \cos\theta \rangle = 0⟨cosθ⟩=0.
  • Dipole Approximation

    • The factor of threes arise because we assume that the radiation is isotropic so the value of Ex2E_x^2E​x​2​​ is typically one third of E2E^2E​2​​ .
  • Inverse Compton Spectra - Single Scattering

    • Let's suppose that we have an isotropic distribution of photons of a single energy E0E_0E​0​​ and a beam of electrons traveling along the xxx-axis with energy γmc2\gamma m c^2γmc​2​​ and density NNN.
    • Let's assume that there are many beams isotropically distributed, so we need to find the mean value of j(Ef,μf)j(E_f,\mu_f)j(E​f​​,μ​f​​) over angle,
    • To be more precise, we could have relaxed the assumption that the scattering is isotropic and we would have found
  • Relation to the flux

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