Scale Model Location

a. b. c.

Figure 6: Comparison of illuminancse monitored in the test module and in scale model 2

a. 2.2 m., b. 4.2 m., c. 6.2 m. from window side, л к,*™* . . ..

14:C0 14:15 14:30 141:45 150 1515 1530 1545 1600 14:00 141:15 141:30 14:45 150 1515 1530 1545 1600 14:00 14:15 14:30 14:45 150 1515 1520 1545 Ш)

Tine Tine line

Workplane illuminances monitored within a scale model placed in two different considered locations (cf. Figure 1.b) overestimate daylighting performances of the test module. Figures 7 and 9 illustrate the observed discrepancies, which remain constant and close to 35 — 40% in relative terms for all profile positions. It shows that moving the model from one location to the other has no impact on the remaining divergence (0 — 1% percent-point reduction) : this indicates that the different sky view factors and external reflected component are apparently not responsible for the remaining discrepancy (cf. Table 3).

a. b. c.

Figure 7: Comparison of relative divergence between illuminances monitored in the test

module and in scale model 2 a. 2.2 m., b. 4.2 m., c. 6.2 m from window side.

14:00 14:15 141:20 14:45 1500 1515 1530 1545 15C0

141:00 14:15 14130 14:45 1500 1515 1530 1545 1500

14:C0 141:15 141:30 1445 1500 1515 1520 1545 1600

a.

b.

c.

Figure 9 : Comparison of relative divergence between illuminances monitored in the test module and in scale model 2. a. 2.2 m., b. 4.2 m., . 6.2 m. from window side

Sky

condition

Maximal Discrepancies (%) First location

Maximal Discrepancies (%) Second location

Percent-point Reduction (%) between both locations

2.2m. from

window

4.2m. from

window

6.2m. from

window

2.2m. from

window

4.2m. from

window

6.2m. from window

2.2m. from

window

4.2m. from

window

6.2m. from window

Clear sky

35

36

37

34

36

37

1

0

0

Table 3 : Comparison of relative divergence for the two different scale model locations

(impact of sky view factor and external reflected component)