Solving a Puzzling Solar Radiation Problem

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SUMMARY

The discussion revolves around calculating the force exerted by solar radiation on the Earth's surface, given an average intensity of 1.4 kW/m² and a mean radius of 6400 km. The correct formula for force is derived as F = (IA/c), where A is the surface area of the Earth. The confusion arises from whether to use the full surface area (4πR²) or half of it (2πR²) due to sunlight only hitting half of the Earth at any time. Ultimately, the correct answer provided by the lecturer is 600 MN, highlighting the importance of understanding the geometry of solar radiation impact.

PREREQUISITES
  • Understanding of solar radiation intensity and energy density
  • Familiarity with the concept of radiation pressure
  • Knowledge of basic physics formulas related to force and area
  • Ability to perform calculations involving the speed of light (c)
NEXT STEPS
  • Study the derivation of radiation pressure formulas in classical physics
  • Learn about the geometry of solar radiation and its impact on planetary bodies
  • Explore the concept of energy density in electromagnetic waves
  • Investigate real-world applications of solar radiation calculations in environmental science
USEFUL FOR

Students preparing for physics exams, educators teaching concepts of solar radiation, and professionals in environmental science or renewable energy sectors.

Beer-monster
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Hi guys

I'm flicking thorugh some past papers for an upcoming exam and came across this seemingly easy problem.

"The average intensity of solar radiation at the Earth is 1.4kW/m^2. Assuming the Earth is a perfect absorber, calculate the force exerted by the radiation on the surface of the Earth. The mean radius of the Earth is 6400 km"

Now I know that the radiation pressure on a perfect absorber is equal to the energy density, which is equal to the intensity divided by the speed of light.

[tex]P = U = \frac{I}{c}[/tex]

Given that P=F/A I get that the force should be.

[tex]F = \frac {IA}{c} = \frac {I 4\pi R^2}{c}[/tex]

Although it could be [tex]\frac {I 2\pi R^2}{c}[/tex]

As the sunlight only directly hits approximately half of the Earth's surface. But either way, when I plug in the numbers I don't get the answer my Lecturer gave of 600 MN.

I must be missing something, but I can't see it. If any of you guys can I'd appreciate it.:biggrin:
 
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Since the sunlight is essentially parallel, the area of interest is that of a circle (not a hemisphere or sphere).
 
That makes sense, since I had noticed I was out by a factor of 4, I just couldn't come up with the physical meaning.

Thanks Doc Al
 

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