Vector space and 3D flow field

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Leo Liu
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Homework Statement
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Relevant Equations
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Printed textbook page: Example 3 asks for the 3D flow field of a gas radiating outward from a source, with the solution's density relation highlighted in green, and F(x,y,z) = δv = c1/ρ² · (c2(xi + yj + zk)/ρ) = c(xi + yj + zk)/ρ³.

Could someone explain the green highlight to me, please?
 
The sum emits light of constant speed c with constant power. The emitted photons becomes more sparse at distant places as ##r^{-2}## so the sun is observed more dimmer.
 
anuttarasammyak said:
The sum emits light of constant speed c with constant power. The emitted photons becomes more sparse at distant places as ##r^{-2}## so the sun is observed more dimmer.
Thanks for providing some physical intuition. But is it because the surface density of a mass flow is
$$\frac{\dot m}{A}=\frac{\dot m}{4\pi r^2}$$
?
 
anuttarasammyak said:
Yes. What's wrong with it ?
Nothing. Just making sure I understand where this proportionality comes from.
 
Another perspective: imagine two concentric spherical surfaces of radii ##\rho_1## and ##\rho_2## (##\rho_2 > \rho_1##) which bound a region ##R##. In steady state the mass contained in ##R## is constant, so the mass fluxes into the inner surface and out of the outer surface are equal: ##4\pi {\rho_1}^2 \delta_1 v = 4\pi {\rho_2}^2 \delta_2 v \, \implies \, \delta \rho^2 = \mathrm{constant}##.