Can Calculus Prove Average Solar Irradiance is a Quarter of Total?

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SUMMARY

The discussion focuses on demonstrating that the average solar irradiance over Earth's surface is one-quarter of the total solar irradiance (So) using calculus. The user initially approaches the problem geometrically, showing that the average solar irradiance can be expressed as So/4 by calculating the ratio of the incident area to the total surface area of a sphere. The user seeks guidance on how to apply calculus, specifically through integration of Socos(θ), to achieve the same result, while also acknowledging the need to consider the Earth's rotation in the analysis.

PREREQUISITES
  • Understanding of solar irradiance and its definition (So)
  • Familiarity with calculus concepts, particularly integration
  • Knowledge of spherical geometry and surface area calculations
  • Basic understanding of the Earth's rotation and its impact on solar irradiance
NEXT STEPS
  • Study the process of integrating functions over spherical coordinates
  • Learn about the implications of Earth's rotation on solar irradiance calculations
  • Explore advanced calculus techniques for surface integrals
  • Review geometric interpretations of solar energy distribution on spherical surfaces
USEFUL FOR

Students and educators in physics and mathematics, particularly those focusing on solar energy calculations, calculus applications, and geometric interpretations of physical phenomena.

Dr.Doom
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Homework Statement


I am trying to show that the average solar irradiance over Earth's surface is 1/4 of the total solar irradiance using only calculus.


Homework Equations


Solar Irradiance = [itex]S_{o}[/itex]
Irradiance = F = [itex]S_{o}[/itex]cos(θ)


The Attempt at a Solution


Using geometry, I can easily show that the average solar irradiance is [itex]S_{o}[/itex]/4 by multiplying [itex]S_{o}[/itex] by the ratio of the incident area and total surface area of a sphere:
[itex]\frac{S_{o}*∏r^2}{4∏r^2}[/itex]=[itex]\frac{S_{o}}{4}[/itex]

My question is how can I use calculus to show this? I was thinking that I could integrate [itex]S_{o}[/itex]cos(θ), but I'm not sure what my integration bounds should be. I'm having trouble visualizing how I can integrate over the entire surface area of a sphere.

Any suggestions would be greatly appreciated!

[Edit] I realize this is probably not the right forum to post this question in but I don't know how to change it.
 
Last edited:
Physics news on Phys.org
Googling the definition of solar irradiance your problem came up in one of the links, looks like you need to consider the rotating Earth in your problem.
 

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