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9.6: Problems

  • Page ID
    141660
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    1. Show that the specific intensity along a ray in empty space is constant.
    2. Compute the specific intensity and the radiative flux at a distance r on the axis of an emitting disk having radius ρ and temperature Te. Assume the disk to be located at r = 0.
    3. Derive the equation of radiative transfer that is appropriate for spherical geometry. List carefully all the assumptions that you make.
    4. Derive the plane-parallel equation of radiative transfer appropriate for a dispersive medium with an index of refraction n which is different from unity and which may vary with position.
    5. Show that for any diagonal tensor A, in spherical coordinates, \[(\nabla \cdot \mathrm{A})_r=\frac{\partial A_{r r}}{\partial r}+\frac{2 A_{r r}-A_{\theta \theta}-A_{\phi \phi}}{r}\nonumber\]
    6. Use the above equation to show that if K is a diagonal tensor with all elements equal to K, then \[(\boldsymbol{\nabla} \cdot \mathbf{K})_\boldsymbol{r}=\frac{\partial K}{\partial r}+\frac{3 K-J}{r}\nonumber\]

    Here K, J, and K have their usual meanings for radiative transfer [see equations (9.3.1), (9.3.8), and (9.3.14)].

    1. Derive equation (9.2.11) from equations (9.2.8) through (9.2.10). Show all your work.
    2. Derive equation (9.2.18) from equations (9.2.2), (9.2.8), (9.2.14), (9.2.15), (9.2.17). Show all your work.
    3. Derive equation (9.4.10) from first principles and axioms. Clearly list all assumptions that you make.

    This page titled 9.6: Problems is shared under a Public Domain license and was authored, remixed, and/or curated by George W. Collins II (Pachart Foundation) via source content that was edited to the style and standards of the LibreTexts platform.