Correct option is C
Introduction:
- The Solar Constant refers to the amount of solar electromagnetic energy per unit area received at the outer edge of Earth's atmosphere, on a surface perpendicular to the Sun's rays, when the Earth is at mean distance from the Sun.
- The Solar Constant (S) is a fundamental parameter in climatology and environmental physics. It represents the total solar irradiance (TSI) reaching the Earth before any atmospheric interference (absorption or scattering).
- It is calculated at the mean distance between the Earth and the Sun, which is one Astronomical Unit (AU) ( 150 million km).
- For environmental scientists, this value is the "starting point" for Earth's energy budget; it determines the equilibrium temperature of our planet and drives all atmospheric and oceanic circulation.
Information Booster:
- The Solar Constant is defined as the total solar electromagnetic radiation (Total Solar Irradiance) per unit area that would be incident on a plane perpendicular to the rays, at a distance of one Astronomical Unit (AU) from the Sun (roughly the mean distance from the Sun to the Earth).
- It is measured at the Top of the Atmosphere (TOA) to eliminate the effects of atmospheric scattering, absorption by greenhouse gases, and reflection by clouds.
- This value serves as the "Solar Input" for all climatological and meteorological models.
- This is the formal scientific definition. It represents the mean solar electromagnetic radiation (total solar irradiance) per unit area incident on a plane perpendicular to the rays at the Top of the Atmosphere (TOA).
Though termed a "constant," it is variable.It fluctuates by about 0.1% during the 11-year solar cycle and varies by approximately ±3.3% annually due to the Earth's elliptical orbit (varying distance between the Sun and Earth).
Additional knowledge:
- The solar constant is a measure of energy flux (power per unit area), not the temperature of the Sun’s surface.
- The average surface temperature (photosphere) is approximately 5,778 K.
- The accepted value of the solar constant is approximately 1361–1367 W/m².
- The value of 1000 W/m² is generally the standard used for solar panel testing at the Earth's surface (Standard Test Conditions) after atmospheric attenuation.