When incident beam intensity from an ordinary source is `I_(0)`, beam intensity of polarised light from `P_(1)` is `I_(0)//2`. If `theta` is angle between `P_(1)` and `P_(2)`, then according to law of Malus, intensity of polarised light from `P_(2)` is
`I = (I_(0))/(2) cos^(2) theta`
When `theta = 0^(@)`, `I = (I_(0))/(2) cos^(2) theta = ((I_(0))/(2))`
When `theta = 30^(@)`, `I = (I_(0))/(2) cos^(2) 30^(@) = (3)/(4)((I_(0))/(2))`
When `theta = 45^(@)`, `I = (I_(0))/(2) cos^(2) 45^(@) = (1)/(2)((I_(0))/(2))`
When `theta = 60^(@)`, `I = (I_(0))/(2) cos^(2) 60^(@) = (1)/(4)((I_(0))/(2))`
When `theta = 90^(@)`, `I = (I_(0))/(2) cos^(2)90^(@) = Zero`
The variation of `I` with `theta` is plotted in Fig.
The blue colour of sky is due to scattering. Light from clear blue portion of sky polarised by scattering. The polaroid through which this light is observed atcs as analyser. The intensity of light viewed through rotating polaroid varies as per law of Malus.
