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Amount of solar energy received on the earth's surface per unit area per unit time is defined a solar constant. Dimension of solar constant is :
Option: 1 ML^{2}T^{-2}
Option: 2 ML^{0}T^{-3}
Option: 3 M^{2}L^{0}T^{-1}
Option: 4 MLT^{-2}

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Let the solar constant= S


\mathrm{S}=\frac{E}{A*T}=\frac{\mathrm{P}}{\mathrm{A}}=\frac{\mathrm{ML}^{2} \mathrm{~T}^{-3}}{\mathrm{~L}^{2}}=\mathrm{ML^0T}^{-3}

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