Solar Constant: Earth's Receiving Intensity

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SUMMARY

The solar constant is defined as 1380 W/m², representing the solar power received per unit area at the top of Earth's atmosphere when considering the Earth as a sphere. However, when accounting for the Earth's surface area and the angle of sunlight, the effective solar energy received at any given point is approximately 340 W/m². This discrepancy arises because not all areas of the Earth are directly facing the Sun at all times, and the intensity varies based on the angle of incidence. Understanding these values is crucial for accurate calculations in solar energy applications.

PREREQUISITES
  • Understanding of solar radiation concepts
  • Familiarity with the geometry of spheres and discs
  • Basic knowledge of power and intensity calculations
  • Awareness of Earth's position relative to the Sun
NEXT STEPS
  • Research the calculation of solar irradiance using the inverse square law
  • Explore the impact of Earth's axial tilt on solar energy distribution
  • Learn about solar energy applications and efficiency metrics
  • Investigate the differences between direct and diffuse solar radiation
USEFUL FOR

Students and professionals in environmental science, solar energy engineers, and anyone interested in understanding solar radiation and its implications for energy systems.

Peter G.
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Hi,

So, I understand the concept that the power radiated by the sun spreads out as a sphere with a radius equal to 1 AU. Therefore, in order to find the intensity, we have to divide the power radiated by the surface area of the sphere. I thought the result of this calculation would yield the intensity per meter squared, that is, in an area of 1 m by 1 m on the surface of the Earth.

However, I was reading some websites and I got really confused. They claim 1380 Wm-2 is the solar constant provided we treat the Earth as a sphere but 340 Wm-2 if we consider only a "disc" is receiving the energy at any given point.

So, is 1380 Wm-2 received at every point on Earth or the Earth itself receives 1380 Wm-2?

Thanks!
 
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Peter G. said:
Hi,

So, I understand the concept that the power radiated by the sun spreads out as a sphere with a radius equal to 1 AU.
The energy spreads our spherically - but the radius depends on where you do the measurement.
Therefore, in order to find the intensity, we have to divide the power radiated by the surface area of the sphere.
That is to say, the intensity at the Earth's orbit.
I thought the result of this calculation would yield the intensity per meter squared, that is, in an area of 1 m by 1 m on the surface of the Earth.
Yes it will ... and the solar flux will be radial through each square meter.
However, I was reading some websites and I got really confused. They claim 1380 Wm-2 is the solar constant provided we treat the Earth as a sphere but 340 Wm-2 if we consider only a "disc" is receiving the energy at any given point.
These sites are taking into account the fact that not everywhere on the Earth is directly facing the Sun. (Not all the same distance from the Sun either.)
 

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