A Malus-factor scan varies the angle between input polarization and polarizer axis across rows, showing how the cos^2(theta) factor and transmitted intensity move row by row. The arithmetic is exact only for the stated angles, factors, and rows in the ideal lossless-polarizer model. Real beams add finite bandwidth, imperfect polarizers, alignment error, detector calibration, surface assumptions, and measurement uncertainty.
Changing the projection factor while holding source intensity fixed shows why intensity squares the field factor. Exact arithmetic here means exact results for the stated model inputs; measured inputs still carry uncertainty and significant-figure limits.
highlighted = computed this step
Projection factor one keeps all intensity
Source intensity is 25 watts per square metre. Squaring factor 1 keeps transmitted intensity at 25 watts per square metre.
Iout=25W/m2(1)2=25W/m2
Factor four-fifths transmits sixteen
Changing only the projection factor to 4/5 sends the same source to 16 watts per square metre because intensity uses the squared factor.
Iout=25W/m2(54)2=16W/m2
Factor three-fifths transmits nine
The third factor is 3/5. It passes 9 watts per square metre and blocks 16 watts per square metre, so the squared relation is visible.