Consider an opaque plate that is well insulated on the edges and it is heated at the bottom with an electric heater. The plate has an emissivity of \(0.67\), and is situated in an ambient surrounding temperature of \(7^{\circ} \mathrm{C}\) where the natural convection heat transfer coefficient is \(7 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\). To maintain a surface temperature of \(80^{\circ} \mathrm{C}\), the electric heater supplies \(1000 \mathrm{~W} / \mathrm{m}^{2}\) of uniform heat flux to the plate. Determine the radiosity of the plate under these conditions.

Short Answer

Expert verified
Answer: To find the radiosity of the plate, follow these steps: 1. Calculate the heat transfer by convection (q_conv) using the formula: q_conv = h * (T_s - T_inf) 2. Apply the energy balance equation: q_heater = q_conv + q_rad 3. Find the emissive power (E_b): q_rad = ε * σ * (T_s^4 - T_inf^4) 4. Calculate the radiosity (J): J = E_b + (q_conv / emissivity) By plugging in the given values and performing calculations according to the solution steps above, the radiosity of the plate can be determined.

Step by step solution

01

Calculate the heat transfer by convection

Calculate the heat transfer by convection between the plate and ambient surroundings using the natural convection heat transfer coefficient: \(q_{conv} = h \cdot (T_s - T_\infty)\) where \(h = 7 \: \mathrm{W/m^2 \cdot K}\) (given natural convection heat transfer coefficient) \(T_s = 80^{\circ} \mathrm{C}\) (desired surface temperature) \(T_\infty = 7^{\circ} \mathrm{C}\) (ambient surrounding temperature) Plugging in the values, we will find the heat transfer by convection.
02

Apply the energy balance equation

Use the energy balance equation to find the relationship between heat losses from the surface by convection and radiation. Let \(q_{rad}\) be the heat transfer by radiation. \(q_{heater} = q_{conv} + q_{rad}\) where \(q_{heater} = 1000 \: \mathrm{W/m^2}\) (heat supplied by the heater) Use the calculated value of \(q_{conv}\) from the previous step and plug it into the equation to find the heat transfer by radiation, \(q_{rad}\).
03

Find the emissive power

To find the emissive power for the given plate, we need to use the relationship: \(q_{rad} = \epsilon \cdot \sigma \cdot (T^4_s - T^4_\infty)\) where \(\epsilon = 0.67\) (emissivity of the plate) \(\sigma = 5.67 \times 10^{-8} \: \mathrm{W/m^2 \cdot K^4}\) (Stefan-Boltzmann constant) We know \(q_{rad}\) from the energy balance equation. We can rearrange the equation to directly calculate the emissive power \(E_b = \sigma \cdot T^4_s\).
04

Calculate the radiosity

Finally, we will calculate the radiosity using the following equation: \(J = E_b + \cfrac{q_{conv}}{emissivity} = \sigma \cdot T_s^4 + \cfrac{q_{conv}}{0.67}\) Plug in the values of emissive power \(E_b\) and the calculated heat transfer by convection, \(q_{conv}\), for the given system, to find the radiosity of the plate.

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