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Hypatio
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(note I am designing this question myself, in order to understand this phenomenon by example)
Find the total radiative power emitted within a 0.1 m2 semi-transparent medium, having an absorption coefficient of 5 m-1 over all spectra, and a temperature of 1000 K. Note that total emitted power is needed, do not consider absorption of power, and do not find the power emitted from the surface of the medium.
We should be able to use the equation
[itex]4\pi \kappa_\lambda I_{\lambda b}(s)dVd\lambda=4\kappa_\lambda E_{\lambda b}(s)dVd\lambda[/itex]
where [itex]\kappa[/itex] is the absorption coefficient, [itex]\lambda[/itex] is the wavelength, V is volume, I is the radiative intensity, E is emissive power, and s is a distance. This equation should give the spectral emission by an isothermal volume element.
The Planck function is
[itex]I_{\lambda b}=\frac{2hc^2}{\lambda^5}\frac{1}{e^{\frac{hc}{\lambda k_bT}}-1}[/itex]
To get the total power emitted by a blackbody (change units from W/m3/sr to W/m3) I multiply by [itex]4\pi[/itex]:
[itex]I^{net}_{\lambda b}=\frac{8\pi hc^2}{\lambda^5}\frac{1}{e^{\frac{hc}{\lambda k_bT}}-1}[/itex]
Numerically integrating over all the spectra for T=1000K to get the total black body intensity, I get about 18 kW/m2. So if my medium had an infinite absorption coefficient (black body), my rounded answer for emission in a 0.1 m2 volume would be 1.8 kW. So far, so good, I think. Now I need to figure out how this value changes with a different absorption coefficient.
I get 5*1.8=9 kW. But this is impossible because 1.8 kW should be the maximum possible. I don't see how to calculate the correct value.
Thanks in advance for any help.
Homework Statement
Find the total radiative power emitted within a 0.1 m2 semi-transparent medium, having an absorption coefficient of 5 m-1 over all spectra, and a temperature of 1000 K. Note that total emitted power is needed, do not consider absorption of power, and do not find the power emitted from the surface of the medium.
Homework Equations
We should be able to use the equation
[itex]4\pi \kappa_\lambda I_{\lambda b}(s)dVd\lambda=4\kappa_\lambda E_{\lambda b}(s)dVd\lambda[/itex]
where [itex]\kappa[/itex] is the absorption coefficient, [itex]\lambda[/itex] is the wavelength, V is volume, I is the radiative intensity, E is emissive power, and s is a distance. This equation should give the spectral emission by an isothermal volume element.
The Planck function is
[itex]I_{\lambda b}=\frac{2hc^2}{\lambda^5}\frac{1}{e^{\frac{hc}{\lambda k_bT}}-1}[/itex]
The Attempt at a Solution
To get the total power emitted by a blackbody (change units from W/m3/sr to W/m3) I multiply by [itex]4\pi[/itex]:
[itex]I^{net}_{\lambda b}=\frac{8\pi hc^2}{\lambda^5}\frac{1}{e^{\frac{hc}{\lambda k_bT}}-1}[/itex]
Numerically integrating over all the spectra for T=1000K to get the total black body intensity, I get about 18 kW/m2. So if my medium had an infinite absorption coefficient (black body), my rounded answer for emission in a 0.1 m2 volume would be 1.8 kW. So far, so good, I think. Now I need to figure out how this value changes with a different absorption coefficient.
I get 5*1.8=9 kW. But this is impossible because 1.8 kW should be the maximum possible. I don't see how to calculate the correct value.
Thanks in advance for any help.
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