1.

Solar constant may be defined as the amount of solar energy received per cm^(2) per minute. The dimensions of solar constant is

Answer»

`[ML^(2)T^(-3)]`
`[ML^(0)T^(-1)]`
`[ML^(0)T^(-2)]`
`[ML^(0)T^(-3)]`

Solution :SOLAR CONSTANT , `S = ("solar energy")/("Area" XX "TIME")= ([ML^(2)T^(-2)])/([L^(2)][T])= [ML^(0)T^(-3)]`


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