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Electromagnetic Fields and Energy - Chapter 5 ... - MIT

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Sec. 5.6 Solutions to Poisson’s Equation 23<br />

Fig. 5.6.2 Equipotentials <strong>and</strong> field lines for configuration of Fig. 5.6.1<br />

showing graphically the superposition of particular <strong>and</strong> homogeneous<br />

parts that gives the required potential.<br />

The variable x in (5) has been replaced by x − vt. With this moving charge distribution,<br />

the field also moves. Thus, (10) becomes<br />

<br />

ρ o cosh βy<br />

Φ = 1 − cos β(x − vt) (12)<br />

o β 2 cosh βa<br />

Note that the homogeneous solution is now a linear combination of the first <strong>and</strong><br />

third solutions in the middle column of Table 5.4.1.<br />

As the space charge wave moves by, the charges induced on the perfectly<br />

conducting walls follow along in synchronism. The current that accompanies the<br />

redistribution of surface charges is detected if a section of the wall is insulated from<br />

the rest <strong>and</strong> connected to ground through a resistor, as shown in Fig. 5.6.1. Under<br />

the assumption that the resistance is small enough so that the segment remains at<br />

essentially zero potential, what is the output voltage v o ?<br />

The current through the resistor is found by invoking charge conservation for<br />

the segment to find the current that is the time rate of change of the net charge on<br />

the segment. The latter follows from Gauss’ integral law <strong>and</strong> (12) as<br />

l/2<br />

<br />

q = w o E y dx<br />

−l/2 y=−a<br />

wρ o<br />

= tanh βa sin β l<br />

− − vt (13)<br />

β<br />

2<br />

2<br />

+ sin β l<br />

+ vt <br />

2<br />

It follows that the dynamics of the traveling wave of space charge is reflected in a<br />

measured voltage of<br />

dq 2Rwρ ov βl<br />

v o = −R = − tanh βa sin sin βvt (14)<br />

dt β<br />

2

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