Heat Transfer - Radiation - Net heat transfer between two mirrors

In summary, the author is asking why we omit reflection that come back to the same mirror. They explain that by considering the reflections from mirrors 1 and 2, it would change the q12 term to be q_{12} = \frac{\epsilon_{2} ( q_{1} + \rho_{1} q_{2})}{1 - \rho_{2} \rho_{1}}.
  • #1
Master1022
611
117
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: [itex] q_{1} = \epsilon_{1} \sigma T_{1}^4 [/itex]. Given that we are dealing with grey bodies, then we know that [itex] \alpha = \epsilon [/itex] and we are told that [itex] \tau = 0 [/itex]. 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):
[tex] 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}} [/tex]

By symmetry, we can find that [itex] q_{21} = \frac{\epsilon_{1} q_{2}}{1 - \rho_{2} \rho_{1}} [/itex].
Then we can find [itex] Q_{net} = Q_{12} - Q_{21} = \frac{A \epsilon_{1} \epsilon_{2} \sigma (T_{1}^4 - T_{2}^4) } {1 - \rho_{2} \rho_{1}} [/itex] (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 [itex] \epsilon_{1} \rho_{2} q_{1}, etc... [/itex])? I think including these terms would change the q12 term to be: [itex] q_{12} = \frac{\epsilon_{2} ( q_{1} + \rho_{1} q_{2})}{1 - \rho_{2} \rho_{1}} [/itex]

Thanks in advance.
 
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  • #2
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.
 
  • #3
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
 

What is heat transfer?

Heat transfer is the movement of thermal energy from one object or system to another. It can occur through three different mechanisms: conduction, convection, and radiation.

What is radiation?

Radiation is the transfer of heat through electromagnetic waves. Unlike conduction and convection, radiation does not require a medium to transfer heat and can occur in a vacuum.

How does heat transfer between two mirrors?

When two mirrors are facing each other, heat transfer occurs through radiation. The hotter mirror emits thermal radiation in the form of electromagnetic waves, which are absorbed by the cooler mirror. The cooler mirror then re-emits some of the energy back to the hotter mirror, resulting in a net transfer of heat between the two mirrors.

What factors affect the net heat transfer between two mirrors?

The net heat transfer between two mirrors is affected by several factors, including the temperature difference between the two mirrors, the surface area of the mirrors, and the reflective properties of the mirrors. The type of material used for the mirrors can also impact the amount of heat transferred.

How is net heat transfer calculated between two mirrors?

The net heat transfer between two mirrors can be calculated using the Stefan-Boltzmann law, which states that the rate of heat transfer is proportional to the fourth power of the temperature difference between the two objects and the emissivity of the objects' surfaces. The formula for net heat transfer is Q = σεA(T1^4 - T2^4), where Q is the net heat transfer, σ is the Stefan-Boltzmann constant, ε is the emissivity of the mirrors' surfaces, A is the surface area of the mirrors, and T1 and T2 are the temperatures of the two mirrors.

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