Sun Radiation to Earth: What Percent Reaches Us?

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Discussion Overview

The discussion revolves around the fraction of solar radiation that reaches the Earth, considering the sun as an absolute black body. Participants explore geometric calculations related to the Earth's cross-sectional area and the implications of the Earth's orientation towards the sun.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant asks about the portion of solar radiation that hits the Earth, seeking a true value rather than an approximation.
  • Another participant suggests that the question can be approached geometrically by comparing the area of the Earth's disc to the surface area of a sphere with the radius of Earth's orbit.
  • There is a discussion about whether to consider the full surface area of the Earth or just half, as only one side faces the sun at a time.
  • A hypothetical scenario is presented where the Earth is turned to face the sun in different orientations, affecting the amount of energy intercepted.
  • A participant expresses realization about the importance of using the area of a flat disc rather than a hemisphere in calculations.
  • Another participant provides the currently accepted value for the Solar Constant and discusses its variability based on solar emissivity and the Earth's position in its orbit.
  • Climatologists use a value of 342 watts per square meter for studies related to the Earth's heat budget, which is derived from the Earth's surface area compared to its cross-section.

Areas of Agreement / Disagreement

Participants generally agree on the geometric approach to calculating the fraction of solar radiation that reaches the Earth, but there are differing views on whether to consider the full surface area or just the cross-section. The discussion remains unresolved regarding the exact portion of radiation that can be considered as reaching the Earth.

Contextual Notes

The discussion includes assumptions about the sun's black body characteristics and the variability of solar radiation based on the Earth's elliptical orbit. There is also mention of the Solar Constant and its dependence on various factors, which may not be fully resolved in the discussion.

Bassalisk
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Assuming that the sun is absolute black body, what portion of radiation coming from the sun, hits the earth?

I know there are some approximations but what is true part arriving at the earth? At some point in time.
 
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Portion? So, you mean what fraction of the sun's total output?

That's a simple geometry question. What is the area of the disc of the Earth as a ratio of the area of a sphere with the radius of Earth's orbit?

But that has nothing to do with black body or anything, which suggest you're looking for a quantity rather than a ratio. Though you could then divide the Sun's total estimated output by the above ratio and work it out.

Alternately, the amount of energy impinging on the Earth per square metre is known. You could simply multiply that number by the area of the Earth's disc.
 
DaveC426913 said:
Portion? So, you mean what fraction of the sun's total output?

That's a simple geometry question. What is the area of the disc of the Earth as a ratio of the area of a sphere with the radius of Earth's orbit?

But that has nothing to do with black body or anything, which suggest you're looking for a quantity rather than a ratio. Though you could then divide the Sun's total estimated output by the above ratio and work it out.

Alternately, the amount of energy impinging on the Earth per square metre is known. You could simply multiply that number by the area of the Earth's disc.

But do I take in the full surface of the earth? OR just half of it? Because sun is not hitting the Earth entirely, just a fraction.
 
Bassalisk said:
But do I take in the full surface of the earth? OR just half of it? Because sun is not hitting the Earth entirely, just a fraction.

DaveC basically already answered that in his post. Read it carefully.
DaveC426913 said:
What is the area of the disc of the Earth

Of course you only use half of the earth, do you see the sun at night? Anyway, the approximation you use is to treat the Earth as a circle with a radius equal to that of the earth, where the normal of the surface of the circle points at the sun. Divide that area by the surface area of a sphere surrounding the sun, with the sun at the center and the Earth at the edge.
 
Last edited:
Suppose we could cut the Earth in half to make a hemisphere. Now suppose we face the flat side towards the sun, and then turn it so the curved side faces towards the sun. It intercepts the same amount of energy either way.

If we have it "half-turned," that is, facing "sideways" towards the sun, then it intercepts half as much energy.
 
I just got "ahaaaaaaaa" moment. Thank you guys. I understand now. It was bugging me because i see people use whole surface of the Earth when solving this problem.

Thanks
 
Just to beat the point to death... :wink: Note that you do not want to calculate the area of the surface of a hemisphere whose radius is that of Earth, you want to calculate the area of a flat disc, whose radius is that of the Earth.
 
Yea i figured that out ^^ thanks
 
Bassalisk said:
Assuming that the sun is absolute black body, what portion of radiation coming from the sun, hits the earth? I know there are some approximations but what is true part arriving at the earth? At some point in time.

The currently accepted value for the Solar Constant is 1366 joules per square meter per second measured normal to the Sun's rays at the outside of the Earth's atmosphere (Scaffeta and West, 2005). This was averaged over two sunspot cycles (22 years). The actual value at anyone instant is a function of the solar emissivity at that instant and the Earth's position on its elliptical orbit. This value has replaced earlier values, and will be replaced in its turn when evidence warrants.

Since the Earth's surface area is four times its cross-section, climatologists use a value of 342 watts per square meter for current studies of the Earth's heat budget.
 

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