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28-4 Interference |
Next, we may test what happens when we have two sources side by side |
sevoral wavelengths apart (Fig. 28-3). The law is that the two sources should |
add theïr efects at point 1 when both of the sources are connected to the same |
generator and are both moving up and down the same way, so that the total |
electric ñeld is the sum of the two and is twice as strong as it was before. |
D S2 |
Fig. 28-3. lllustration of interference of sources. |
Now comes an interesting possibility. Suppose we make the charges In S1 |
and Š› both accelerate up and down, but delay the timing of Š5› so that they are |
1802 out of phase. 'Phen the field produced by ŠS¡ will be in one direction and |
the field produced by ŠS+ will be in the opposite direction at any instant, and |
therefore we should get øoø efect at point 1. The phase of oscillation is neatly |
adjustable by means of a pipe which is carrying the signal to S¿. By changing |
the length of this pipe we change the time it takes the signal to arrive at 5s and |
thus we change the phase of that oscillation. By adjusting this length, we can |
indeed fnd a place where there is no more signal left, in spite of the fact that |
both 5¡ and 52 are movingl The fact that they are both moving can be checked, |
because if we cut one out, we can see the motion of the other. So the bwo of |
them together can produce zero iŸ everything is adjusted correctly. |
Now, i1 is very interesting to show that the addition of the two fields is in |
fact a 0ector addition. We have Jjust checked it for up and down motion, bu§ |
let us check two nonparallel directions. First, we restore 5 and S2 to the same |
phase; that is, they are again moving together. But now we turn 5: through 902, |
as shown in Fig. 28-4. Now we should have at point 1 the sum of two efects, |
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2. /R |
S2 |
Fig. 28-4. lllustration of the vector character of the combination of |
SOUFCeS. |
one of which is vertical and the other horizontal. The electric fñeld is the vector |
sum oŸ these two in-phase signals—they are both strong at the same time and go |
through zero together; the total fñeld should be a signal at 45°. If we turn |
to get the maximum noise, it should be at about 45°, and not vertical. And if |
we turn i% at right angles to that direction, we should get zero, which is easy to |
mmeasure. Indeed, we observe just such behaviorl |
Now, how about the retardation? How can we demonstrate that the signal is |
retarded? We could, with a great deal of equipment, measure the time at which |
1t arrives, but there is another, very simple way. Referring again to Fig. 28-3, |
suppose that 5¡ and S52 are in phase. 'Phey are both shaking together, and |
they produce equal electric fields at point 1. But suppose we go to a certain |
place 2 which is closer to S2 and farther from Š¡. Then, in accordance with the |
principle that the acceleration should be retarded by an amount equal to r/e, |
1f the retardations are not equal, the signals are no longer in phase. Thus it |
should be possible to fnd a position at which the distances of 1 from 5% and S2 |
difer by some amount A, in such a manner that there is no net signal. 'Phat |
is, the distance A is to be the distance light goes in one-half an oscillation of |
the generator. We may go still further, and fñnd a poïint where the diferenece is |
greater by a whole cycle; that is to say, the signal from the first antenna reaches |
point 3 with a delay in time that is greater than that of the second antenna, |
by just the length of time it takes for the electric current to oscillate once, and |
therefore the two electric fñelds produced at 3 are in phase again. At point 3 the |
signal is strong again. |
This completes our discussion of the experimental verifcation of some of |
the important features of Eq. (28.6). Of course we have not really checked |
the 1/r variation of the electric feld strength, or the fact that there is also a |
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magnetic fñeld that goes along with the electric ñeld. To do so would require |
rather sophisticated techniques and would hardly add to our understanding at |
this point. In any case, we have checked those features that are of the greatest |
Importance for our later applications, and we shall come back to study some of |
the other properties of electromagnetic waves next year. |
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Xrfor'for-orte© |
29-1 Electromagnetic waves |
In this chapter we shall discuss the subject of the preceding chapter more |
mathematically. We have qualitatively demonstrated that there are maxima, |
and minima in the radiation fñeld from two sources, and our problem now is tO |
describe the field in mathematical detail, not just qualitatively. |
We have already physically analyzed the meaning of formula (28.6) quite |
satisfactorily, but there are a few points to be made about it mathematically. In |
the frst place, IŸ a charge is accelerating up and down along a line, in a motion |
of very small amplitude, the fñield at some angle Ø from the axis of the motion is |
in a direction at right angles to the line of sight and in the plane containing both |
the acceleration and the line of sight (Fig. 29-1). Iƒ the distance is called r, then |
at time £ the electric fñeld has the magnitude |
—qa{(‡ — r/e) sin 8 |
#(0 = _—_^.. (29.1) |
47cgc2r |
Fig. 29-1. The electric field E due to a positive charge whose retarded |
acceleration is a”. |
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Fig. 29-2. The acceleration of a certain charge as a function of time. |
Fig. 29-3. The electric field as a function of position at a later time. |
(The 1/r variation is ignored.) |
where a(# — r/e) is the acceleration at the time (£ — r/c), called the retarded |
acceleration. |
Now it would be interesting to draw a picture of the fñeld under different |
conditions. The thing that is interesting, of course, is the factor ø(£ — r/c), |
and to understand it we can take the simplest case, Ø = 90”, and plot the field |
graphically. What we had been thinking of before is that we stand in one position |
and ask how the fñeld there changes with time. But instead of that, we are now |
goïing to see what the field looks like at diferent positions in space at a given |
Instant. So what we want is a “snapshot” picture which tells us what the fñeld |
1s In diÑerent places. Of course it depends upon the acceleration of the charge. |
Suppose that the charge at first had some particular motion: it was Initially |
standing still, and ¡it suddenly accelerated in some mamner, as shown in Fig. 29-2, |
and then stopped. 'Then, a little bit later, we measure the field at a diferent |
place. Then we may assert that the feld will appear as shown in Eig. 29-3. At |
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