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B
[M1L1T−2]
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C
[M1L−1T−2]
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D
[M1T−3]
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Solution
The correct option is C[M1T−3] Solar constant(S) is defined as energy due to sun falling on an unit area per unit time . ⇒S=(EA)×1T=(ML2T2)×1L2×1T=MT−3