Skin temperature increase due to radiation absorption

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SUMMARY

The discussion focuses on calculating the increase in human skin temperature due to radiation absorption, specifically using the Stefan-Boltzmann law. The key equations mentioned are Pnet = Pemit - Pabsorb and Pnet = Aσε(T4 - T04), where A is body surface area, ε is emissivity, T is skin temperature, and T0 is ambient temperature. The initial skin temperature and radiation intensity (e.g., 1000 W/m2) are critical for these calculations. The discussion highlights the complexity of the problem due to physiological factors like blood flow affecting heat transfer.

PREREQUISITES
  • Understanding of the Stefan-Boltzmann law
  • Familiarity with black-body radiation concepts
  • Knowledge of thermal dynamics and heat transfer principles
  • Basic mathematics for manipulating equations
NEXT STEPS
  • Research the Stefan-Boltzmann constant and its applications in thermal calculations
  • Explore the concept of emissivity and its impact on heat absorption
  • Learn about blood flow's role in thermoregulation and heat transfer in human skin
  • Investigate the effects of different radiation intensities on skin temperature
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This discussion is beneficial for physicists, biomedical engineers, and anyone interested in thermoregulation and heat transfer in biological systems.

fog37
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Hello,

I am trying to figure out how much the human skin temperature would increase when the skin is illuminated by radiation of a certain intensity (W/m^2). We can assume that the skin has an emissivity and absorptivity both equal to 1. For instance, imagine the skin illuminated by the sun (I= 1000W/m^2) or by another radiation source..
We know the initial temperature of the skin and the intensity of the incident radiation.

What equation would I use?

Thanks!
 
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fog37 said:
What equation would I use?
You have poked on the Intermediate Level.
Are you familiar with the Stefan-Boltzmann law?
The Stefan–Boltzmann law states that the power emitted per unit area of the surface of a black body is directly proportional to the fourth power of its absolute temperature
Prad = σ T4
 
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fog37 said:
Hello,

I am trying to figure out how much the human skin temperature would increase when the skin is illuminated by radiation of a certain intensity (W/m^2). We can assume that the skin has an emissivity and absorptivity both equal to 1. For instance, imagine the skin illuminated by the sun (I= 1000W/m^2) or by another radiation source..
We know the initial temperature of the skin and the intensity of the incident radiation.

What equation would I use?

Thanks!
Interesting question.
I worked out a similar problem for a black rock about 6 months ago. Unfortunately, I can't remember how I did it, nor do I know whether or not my answer was correct.

I would recommend looking at the wiki entry on "Black-body radiation", subsection "Human body emission".
It may not give you the answer, but it has a couple of equations that will get you started:
Pnet = Pemit - Pabsorb
and
Pnet = Aσε(T4 - T04)

A is body surface area
T is body surface temperature
ε is body emissivity
T0 is the ambient temperature
σ is the Stefan–Boltzmann constant​

Of course, your problem is a bit more complicated, as rocks don't sweat.
 
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The heat that the skin absorbs is continuously being transferred away with the blood flow through the capillary veins in the skin, so this can't be calculated as a simple radiative transfer problem.
 

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