Total solar irradiance or solar constant Formula

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Total solar irradiance or solar constant is the solar energy reaching the earth’s/planet's atmosphere. Check FAQs
Gs=(r2)[Stefan-BoltZ](Ts4)L2
Gs - Total Solar Irradiance?r - Radius of the Sun?Ts - Effective Surface Temperature?L - Mean Distance between Sun and Planet?[Stefan-BoltZ] - Stefan-Boltzmann Constant?

Total solar irradiance or solar constant Example

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With units
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Here is how the Total solar irradiance or solar constant equation looks like with Values.

Here is how the Total solar irradiance or solar constant equation looks like with Units.

Here is how the Total solar irradiance or solar constant equation looks like.

1358.6563Edit=(7E+8Edit2)5.7E-8(5780Edit4)1.5E+11Edit2
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Total solar irradiance or solar constant Solution

Follow our step by step solution on how to calculate Total solar irradiance or solar constant?

FIRST Step Consider the formula
Gs=(r2)[Stefan-BoltZ](Ts4)L2
Next Step Substitute values of Variables
Gs=(7E+8m2)[Stefan-BoltZ](5780K4)1.5E+11m2
Next Step Substitute values of Constants
Gs=(7E+8m2)5.7E-8(5780K4)1.5E+11m2
Next Step Prepare to Evaluate
Gs=(7E+82)5.7E-8(57804)1.5E+112
Next Step Evaluate
Gs=1358.65631949202W/m²
LAST Step Rounding Answer
Gs=1358.6563W/m²

Total solar irradiance or solar constant Formula Elements

Variables
Constants
Total Solar Irradiance
Total solar irradiance or solar constant is the solar energy reaching the earth’s/planet's atmosphere.
Symbol: Gs
Measurement: Heat Flux DensityUnit: W/m²
Note: Value should be greater than 0.
Radius of the Sun
Radius of the sun is the radius of the sun/star.
Symbol: r
Measurement: LengthUnit: m
Note: Value should be greater than 0.
Effective Surface Temperature
Effective surface temperature is the surface temperature of the sun/star.
Symbol: Ts
Measurement: TemperatureUnit: K
Note: Value should be greater than 0.
Mean Distance between Sun and Planet
Mean distance between sun and planet is the mean distance between sun/star and earth/planet.
Symbol: L
Measurement: LengthUnit: m
Note: Value should be greater than 0.
Stefan-Boltzmann Constant
Stefan-Boltzmann Constant relates the total energy radiated by a perfect black body to its temperature and is fundamental in understanding blackbody radiation and astrophysics.
Symbol: [Stefan-BoltZ]
Value: 5.670367E-8

Other formulas in Atmospheric and Solar Radiation category

​Go Effective surface temperature of sun given solar constant
Ts=((L2)Gs(r2)[Stefan-BoltZ])0.25
​Go Mean distance between sun or star and earth or planet
L=((r2)[Stefan-BoltZ](Ts4)Gs)0.5
​Go Radius of sun given total solar irradiance
r=((L2)Gs[Stefan-BoltZ](Ts4))0.5
​Go Total solar energy incident on unit area of horizontal surface on ground
Gsolar=GDcos(i)+Gd

How to Evaluate Total solar irradiance or solar constant?

Total solar irradiance or solar constant evaluator uses Total Solar Irradiance = ((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/(Mean Distance between Sun and Planet^2) to evaluate the Total Solar Irradiance, Total solar irradiance or solar constant formula is defined as a measure of the amount of solar energy received per unit area at the top of the Earth's atmosphere, representing the rate at which the sun's energy is received on Earth, which is essential for understanding climate and weather patterns. Total Solar Irradiance is denoted by Gs symbol.

How to evaluate Total solar irradiance or solar constant using this online evaluator? To use this online evaluator for Total solar irradiance or solar constant, enter Radius of the Sun (r), Effective Surface Temperature (Ts) & Mean Distance between Sun and Planet (L) and hit the calculate button.

FAQs on Total solar irradiance or solar constant

What is the formula to find Total solar irradiance or solar constant?
The formula of Total solar irradiance or solar constant is expressed as Total Solar Irradiance = ((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/(Mean Distance between Sun and Planet^2). Here is an example- 1358.656 = ((695000000^2)*[Stefan-BoltZ]*(5780^4))/(150000000000^2).
How to calculate Total solar irradiance or solar constant?
With Radius of the Sun (r), Effective Surface Temperature (Ts) & Mean Distance between Sun and Planet (L) we can find Total solar irradiance or solar constant using the formula - Total Solar Irradiance = ((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/(Mean Distance between Sun and Planet^2). This formula also uses Stefan-Boltzmann Constant .
Can the Total solar irradiance or solar constant be negative?
No, the Total solar irradiance or solar constant, measured in Heat Flux Density cannot be negative.
Which unit is used to measure Total solar irradiance or solar constant?
Total solar irradiance or solar constant is usually measured using the Watt per Square Meter[W/m²] for Heat Flux Density. Kilowatt per Square Meter[W/m²], Watt per Square Centimeter[W/m²], Watt per Square Inch[W/m²] are the few other units in which Total solar irradiance or solar constant can be measured.
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