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Using the Earth's Magnetic Field for Measurements
You have spotted an unidentified flying object! Naturally, you wish to find its charge. You have a compass, a good sense of direction, and keen eyesight. You notice that it is flying due south on a course that will pass directly overhead, and it is 30 m above you, travelling at 200 m/s. You observe the dial on your properly aligned compass as the object passes overhead. As a function of time, this is what you see:
Facts
- We know |→Bearth|=32μT.
- If we align our coordinate axes, according to the represention below, →Bearth=32μT ˆy.
- h=30 m.
- →v=−200 m/s ˆy.
- You have the graph of θ versus t.
Lacking
- →BtextUFO
Approximations & Assumptions
- The UFO can be approximated as a moving point charge.
- q, →v, h, and →Bearth are all constants.
- Your sense of direction and eyesight can be trusted.
Representations
- We represent the Biot-Savart Law for the magnetic field from a moving point charge as
→B=μ04πq→v×→rr3
- We represent the situation with the following pictures. Coordinate axes and cardinal directions are specified.
Solution
Below, we show a diagram with a lot of pieces of the Biot-Savart Law unpacked. We show an example d→l, and a separation vector →r. Notice that d→l is directed along the segment, in the same direction as the current. The separation vector →r points as always from source to observation.
For now, we write d→l=⟨dx,dy,0⟩ and →r=→robs−→rsource=0−⟨x,y,0⟩=⟨−x,−y,0⟩ Notice that we can rewrite y as y=−L−x. This is a little tricky to arrive at, but is necessary to figure out unless you rotate your coordinate axes, which would be an alternative solution to this example. If finding y is troublesome, it may be helpful to rotate. We can take the derivative of both sides to find dy=−dx. We can now plug in to express d→l and →r in terms of x and dx: d→l=⟨dx,−dx,0⟩ →r=⟨−x,L+x,0⟩ Now, a couple other quantities that we see will be useful: d→l×→r=⟨0,0,dx(L+x)−(−dx)(−x)⟩=⟨0,0,Ldx⟩=Ldxˆz r3=(x2+(L+x)2)3/2 The last thing we need is the bounds on our integral. Our variable of integration is x, since we chose to express everything in terms of x and dx. Our segment begins at x=−L, and ends at x=0, so these will be the limits on our integral. Below, we write the integral all set up, and then we evaluate using some assistance some Wolfram Alpha. →B=∫μ04πI⋅d→l×→rr3=∫0−Lμ04πILdx(x2+(L+x)2)3/2ˆz=μ02πILˆz