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    The Solar constant is: (A) average temperature at sun’s surface (B) a measure of solar energy impinging upon sun-facing unit area of Earth’s top of
    Question

    The Solar constant is:

    (A) average temperature at sun’s surface

    (B) a measure of solar energy impinging upon sun-facing unit area of Earth’s top of atmosphere

    (C) 1000 W/m²

    (D) variable

    Choose the correct answer from the options given below:

    A.

    (A), (C) and (D) Only

    B.

    (B), (C) and (D) Only

    C.

    (B) and (D) Only

    D.

    (A) and (C) Only

    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) (\approx​ 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.

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