Clearβsky global irradiance represents the amount of solar energy reaching a horizontal surface when clouds are absent, and it is a cornerstone for solarβenergy assessments and climate studies.
The irradiance depends on the solar constant, the EarthβSun distance correction, atmospheric transmissivity, and the solar zenith angle, which together modulate the direct solar beam reaching the ground.
Accurate estimation of this quantity enables designers to size photovoltaic systems, researchers to model surface temperature, and meteorologists to forecast solarβdriven processes.
I_{sc} = solar constant (~1361β―W/mΒ²)
E_{0} = EarthβSun distance factor
tau = atmospheric transmissivity
theta = solar zenith angle (degrees)
What is clear-sky global irradiance?
Why is clear-sky global irradiance important?
What factors affect clear-sky global irradiance?
How do I use this calculator to estimate clear-sky global irradiance?
Can this calculator be used for any location on Earth?
What is the difference between clear-sky and actual global irradiance?
How accurate are the estimates provided by this calculator?
Results are for informational purposes only and do not constitute professional advice.
