00:01
In this question, we're given e, which is the solar energy passing through a hemisphere object or surface, per unit time per unit area.
00:14
I is the solar intensity, and teter is the angle at which is directed from the perpendicular.
00:21
So we want to find e by integrating this expression here.
00:26
There are a couple ways to integrate this.
00:28
For this topic, we are using substitution method and the integration.
00:32
Power rule.
00:35
Let you be sine teter.
00:37
It can be cosine teter as well, but it's easier to differentiate sign.
00:41
So the u over d teter will be cosine teter.
00:47
So the u will be cosine teter d teter.
00:52
So let me rearrange we are two pi i.
00:59
I will have sign teter in front and cosine teter d titter at the back here.
01:05
So you can see this is u and this will be the u.
01:08
Now do not forget to sub up the lower upper limit...