Calculate the power measured by the detector at distance h from the source

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SUMMARY

The discussion focuses on calculating the power measured by a thin disc-like detector at a distance h from an isotropic point source emitting electromagnetic energy. Participants utilize key concepts such as Beer’s Law and the inverse square law to derive the intensity and power received by the detector. The final result presented is P = (-R² * i₀)/(4h²(h² + R²)), where R is the radius of the detector, h is the distance from the source, and i₀ is the intensity at the source. The conversation emphasizes the importance of integrating over the area of the detector and accounting for attenuation effects.

PREREQUISITES
  • Understanding of isotropic point sources and electromagnetic radiation
  • Familiarity with Beer’s Law for attenuation of light
  • Knowledge of the inverse square law in physics
  • Basic calculus for integration over circular areas
NEXT STEPS
  • Study the derivation of the inverse square law in electromagnetic contexts
  • Learn about Beer’s Law applications in different media
  • Explore integration techniques for circular areas in calculus
  • Investigate the physical implications of isotropic radiation in practical scenarios
USEFUL FOR

Students in physics or engineering, particularly those studying electromagnetism, as well as educators looking for practical examples of power calculations in radiation theory.

  • #31
gneill said:
Typing out is always better. It makes quoting and commenting much easier. Many helpers will just abandon ship if they have to do too much work to respond.

But, making an effort to clip, edit, and post a piece of your image, can you explain the exponent of 4 in your equation:
View attachment 233381

thanks, i will type from now on,it's from the inverse square law(S/(4*pi*d^4)=ir)
 
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  • #32
Hmm. I'd say that the power is spread over the surface area of a sphere of a given radius, so the flux would go as

##\Phi = \frac{P_o}{4 \pi r^2}##

Where r is the distance from the source.

The same should apply to intensity.
 
  • #33
gneill said:
Hmm. I'd say that the power is spread over the surface area of a sphere of a given radius, so the flux would go as

##\Phi = \frac{P_o}{4 \pi r^2}##

Where r is the distance from the source.

The same should apply to intensity.

oh okay, so if i replace the 4 with a 2, the final result is i0(ln(h^2+R^2)-2ln(h))/4, does that make more sense?
thanks
 
  • #34
Yes, it does to me :smile:

I think you could do some manipulation of the logs to get a more concise version, but otherwise I think you're doing fine.
 
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  • #35
gneill said:
Yes, it does to me :smile:

I think you could do some manipulation of the logs to get a more concise version, but otherwise I think you're doing fine.

that's great! i have been working on this for almost a week and couldn't figure it out hahahaha
thanks a lot!
nadi
 

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