The externally-reflected component will normally represent only a very small
fraction of the total daylight factor value at a point in a room. Consequently a
simplified procedure is usually adopted for its calculation. This procedure
involves calculating an 'equivalent sky component' to the area of sky obscured
by the external obstruction, assigning a value of the luminance of the
obstruction as some fraction of the luminance of the obscured sky, and then
multiplying the equivalent sky component by the relative luminance. The outline
of the obstructions viewed from a point in the centre of the room is normally
reconfigured so that it becomes a horizontal line with an area of obstruction
below it similar in size to the actual obstruction outline.