00:02
In this problem, we have a rectangular region.
00:05
I'm drawing that with orange, and that is rotating at a uniform angular velocity omega.
00:11
It's rotating in a uniform magnetic b field that's pointing along the x -axis, and at time t equals zero, this region is entirely contained in the yz plane.
00:25
Our goal is to find the plots of the flux, the rate of change of the flux, the emf, and the emf, if we were to double the angular velocity.
00:35
And i'm going to draw all of those on the same plot.
00:38
So let's start out with a flux.
00:40
Let's recall that the net flux in a uniform b field is given by ea cosine, where fee is the angle between the perpendicular of the area and the b field.
00:55
So the perpendicular of our area, i'll draw that in red on our diagram, and that's given by that guy.
01:02
So we see at time t equals zero, these are pointing in the same direction.
01:08
So we don't have to worry about any phase shift.
01:10
This is just b a cosine omega -t.
01:15
On our plot, we see that this has an amplitude of b -a.
01:20
So i will draw this in green.
01:25
And on the axes, i'll delineate that by, let's go pi over two omega, pi over omega, 3 pi over 2 omega, and we'll go 2 pi.
01:42
So we just have a normal cosine here.
01:45
Let's see how we can do this.
01:49
Zero, maximum negative, zero.
01:55
Okay, for the second part, we have the rate of change of our flux.
02:05
Now, this is going to be given by the slope of the plot that we just drew.
02:09
So let's get a qualitative feel for what this should be.
02:14
We see that it starts out with zero slope.
02:16
So it's going to have a node here.
02:19
It has a zero slope at pi over omega...