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.