Heat Transfer - Radiation - Net heat transfer between two mirrors

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SUMMARY

The discussion focuses on the net heat transfer between two mirrors, specifically addressing the omission of self-reflected heat in calculations. The heat flux emitted by a mirror is defined by the equation q_{1} = \epsilon_{1} \sigma T_{1}^4, where ε represents emissivity and σ is the Stefan-Boltzmann constant. The derived net heat transfer equation is Q_{net} = Q_{12} - Q_{21} = \frac{A \epsilon_{1} \epsilon_{2} \sigma (T_{1}^4 - T_{2}^4)}{1 - \rho_{2} \rho_{1}}, assuming equal areas and T_1 > T_2. The discussion concludes that energy remaining within a mirror is irrelevant to the net heat transfer analysis.

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Master1022
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Homework Statement
There are two mirrors which act as grey bodies which are a short distance away from one another. There is no transmission at each of the mirrors. What is the net heat transfer between the mirrors?
Relevant Equations
[itex] q = \epsilon \sigma T^4 [/itex]
[itex] \alpha + \tau + \rho = 1 [/itex]
Hi,

So there is already a written solution which I have, but this is more a question about why we omit reflection that come back to the same mirror?

Method:

Let us consider one of the mirrors, we know it will emit a heat flux given by: q_{1} = \epsilon_{1} \sigma T_{1}^4. Given that we are dealing with grey bodies, then we know that \alpha = \epsilon and we are told that \tau = 0. If we want to consider the heat that reaches and is absorbed by the other mirror, then we get the following sum (as a result of successive reflections):
q_{12} = \epsilon_{2} q_{1} + \rho_{2} \rho_{1} \epsilon_{2} q_{1} + \left( \rho_{2} \rho_{1} \right)^2 \epsilon_{2} q_{1} + \left( \rho_{2} \rho_{1} \right)^3 \epsilon_{2} q_{1} + ... = \frac{\epsilon_{2} q_{1}}{1 - \rho_{2} \rho_{1}}

By symmetry, we can find that q_{21} = \frac{\epsilon_{1} q_{2}}{1 - \rho_{2} \rho_{1}}.
Then we can find Q_{net} = Q_{12} - Q_{21} = \frac{A \epsilon_{1} \epsilon_{2} \sigma (T_{1}^4 - T_{2}^4) } {1 - \rho_{2} \rho_{1}} (assuming areas are equal and that T_1 is greater than T_2). This is the answer that I am 'supposed' to get.

However, I was wondering why we don't also consider the rays that are emitted from a mirror and are reflected back towards itself (i.e. the \epsilon_{1} \rho_{2} q_{1}, etc...)? I think including these terms would change the q12 term to be: q_{12} = \frac{\epsilon_{2} ( q_{1} + \rho_{1} q_{2})}{1 - \rho_{2} \rho_{1}}

Thanks in advance.
 
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For the same reason that you don't include in ##q_{12}## the heat that never left 2 because ##\epsilon_2 < 1##.

You are looking at transfers from 1 to 2. Energy that stays in one object, for whatever reason, is irrelevant.
 
DrClaude said:
For the same reason that you don't include in ##q_{12}## the heat that never left 2 because ##\epsilon_2 < 1##.

You are looking at transfers from 1 to 2. Energy that stays in one object, for whatever reason, is irrelevant.
Ah okay that makes sense - we have defined q as the heat that has already left the mirror.

Thank you
 

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