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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:
(1) $ML^2T^{-2}$
(2) $ML^0T^{-3}$
(3) $M^2L^0T^{-1}$
(4) $MLT^{-2}$
Solar constant $= \frac{\text{Energy}}{\text{Time} \times \text{Area}} = \frac{M^1L^2T^{-2}}{TL^2} = M^1L^0T^{-3}$.
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