How Does the Nevada Solar One System Manage Radiative Heat Transfer?

In summary, the given problem involves the Nevada Solar One thermal solar power system, which uses 760 parabolic mirrors to reflect sunlight onto a cylindrical tube carrying a heat transfer fluid. Each mirror contributes 84kW, resulting in a total power output of 64MW. Assumptions include a mirror width of 1.4m, spectral emissivity of the central tube, and neglecting emitted energy from the tube and concentrator. To calculate the temperature of the tube, a balance is made between the incoming and outgoing heat, resulting in a temperature of 2150K. To determine the energy that must be removed by the coolant per meter of tube length, a balance is made between the energy coming in from the tube and the energy
  • #1
Vyrwnas
2
0

Homework Statement



The problem is about Nevada Solar One thermal solar power system.It uses 760 parabolic mirrors reflecting sunlight on a cylindrical tube carrying a heat transfer fluid.Each mirror contributes 84kW giving a total 64MW.
Assumptions:The mirror has a width(orthogonal to incoming sunlight) of 1.4m and reflects 95% of the solar light(1125W/m2) on to the central tube.Let the central tube have a diameter of 6cm and be of uniform temperature and coated with a material that has the direction independent spectral emissivity as follows:

ελ=0.85 for λ<2.6μm
ελ=0.35 for 2.6<λ<4.2μm
ελ=0.15 for λ>4.2μm

Emitted energy from the tube that is reflected by the concentrator(mirror) may be neglected as may emission from the concentrator.The surrounding environment is a relative low temperature.

Questions:
1.if the heat exchange is only by radiation compute the temperature of the tube.
2.if the tube is cooled to 650K by passing a coolant through its interior how much energy must be removed by the cooland per meter of tube length?
3.how much length is needed to reach a power of 84kW.Is this length comparable with the length of Nevada Solar One?If not which assumptions should be changed?


The Attempt at a Solution



Here are the solutions i gave:
1.if the heat exchange is only by radiation i can make a balance in what commes in and out of the tube so:
qin=qout
qin=1125*95/100=1068.75 so in total 760*1068.75*760=812250W/m2
qout=σT4[0.85[f(n=1,2.6,T)-f(0)]+0.35[f(n=1,4.2,T)-f(n=1,2.6,T)]+0.15[f([tex]\infty[/tex],T)-f(n=1,4.2,T)]]

So if i try some values for T i can see that for T=2150K qout=812250W/m2.
I think that this is correct but there must be a more appropriate way to solve this question.
Also i tried to take into account the spectral emission in wavelenghts below 2.6 as it is the most important in these temperatures and do a simple balance where qin=qout[tex]\Rightarrow[/tex]812250=0.85σΤ4 which results a T=2026.15K.So its reasonable.This offcourse is for the whole pipe and all the mirrors.

2.for the second question i also made a balance taking into account the q that's goes out with the cooland so 0=qin-qcoolant-qradiation,T=650[tex]\Leftrightarrow[/tex]qcoolant=1068.75-2072,5=-1003.75W/m2

So per meter of tube length 1003.75*2*π*r=189.2W/m

3.To reach a power of 84kW [tex]\frac{84000}{189.2}[/tex]=444 while if i use the width 1.4m 84000/1068.75=79m2 so 79/1.4=56m

In the second question i used the energy that comes in from one mirror since in the 3rd asks to reach a power of 84kW.i think that i could use the power from all mirrors qin=812250W/m2 if i had to compare it with the 64MW.Ive been also told that the qout by radiation is not important in this question but this doesn't seem the case to me.If i don't use energy emitted by radiation its basically like i don't define the temperature of the tube at 650K.Its also strange that i don't use the mirror width except when i calculate the tube length to compare it with what i find.I am looking for some inspiration and i would really appreciate any help and suggestions...

Thanks in advance :)
 
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  • #2

Thank you for sharing your solutions to the given problem. Your calculations seem to be correct and your approach is reasonable. However, there are a few points that could be improved upon.

Firstly, in your solution to the first question, you have correctly taken into account the spectral emissivity of the tube. However, you have not considered the spectral reflectivity of the mirrors. Since the mirrors reflect 95% of the solar light, only 95% of the incident radiation will be absorbed by the tube. This should be taken into account in your calculation of qin.

Secondly, in your solution to the second question, you have correctly calculated the energy that needs to be removed by the coolant per meter of tube length. However, the value you have used for qcoolant seems to be incorrect. You have used the value of qin at a temperature of 650K, which is not the same as the energy that needs to be removed by the coolant. The value of qcoolant should be equal to the energy that is transferred from the tube to the coolant, which can be calculated using the Stefan-Boltzmann law and the spectral emissivity of the tube at a temperature of 650K.

Lastly, in your solution to the third question, you have correctly calculated the length of the tube needed to reach a power of 84kW. However, you have not taken into account the fact that the mirrors are not all reflecting onto the same spot on the tube. The mirrors are spread out, and therefore, the length of the tube needed will be longer than the length of the array of mirrors. This is why the length you have calculated is not comparable to the length of Nevada Solar One. To accurately compare the lengths, you would need to consider the spacing between the mirrors and the distance between the mirrors and the tube.

I hope this helps to improve your solutions and provides some inspiration for further exploration. Keep up the good work!
 

FAQ: How Does the Nevada Solar One System Manage Radiative Heat Transfer?

What is radiative heat transfer?

Radiative heat transfer is the transfer of thermal energy through electromagnetic waves, such as infrared radiation. It does not require a medium, unlike conduction and convection, and can occur through a vacuum.

How does radiative heat transfer differ from other types of heat transfer?

Radiative heat transfer differs from conduction and convection in that it does not require a medium to transfer heat. It can occur through a vacuum and is not affected by the physical properties of the material it is passing through.

What are some common applications of radiative heat transfer?

Radiative heat transfer is commonly used in various heating and cooling systems, such as solar panels and thermal insulation. It is also important in industries such as aerospace and materials processing.

What factors affect the rate of radiative heat transfer?

The rate of radiative heat transfer is affected by the temperature difference between the objects, the emissivity of the surfaces, and the distance between the objects. It is also influenced by the type of material and its surface properties.

How is radiative heat transfer calculated?

Radiative heat transfer is calculated using the Stefan-Boltzmann law, which states that the rate of heat transfer is proportional to the temperature difference between the objects and their emissivity. It can also be calculated using the heat transfer coefficient, which takes into account other factors such as surface area and geometry.

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