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  • Solar Constant: Understanding Solar Energy Reaching Earth
    The solar constant is a measure of the amount of solar energy that reaches Earth's upper atmosphere per unit area per unit time.

    In other words, it tells us how much solar radiation is received by a surface perpendicular to the sun's rays, located outside Earth's atmosphere.

    Here are some key details:

    * Units: The solar constant is typically measured in watts per square meter (W/m²).

    * Value: The average value of the solar constant is approximately 1361 W/m².

    * Variability: The solar constant isn't perfectly constant and can fluctuate slightly due to variations in the Sun's output.

    * Importance: The solar constant is crucial for understanding Earth's climate system, as it drives the energy balance that regulates our planet's temperature.

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