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of „# can be considered as the horizontal projectlon of a rofating uector. Suppose |
there were a vector ¡ of length 4 rotating with time, so that its angle with the |
horizontal axis is œ‡ + ởị. (WS shall leave out the œ# in a minute, and see that it |
makes no diference.) Suppose that we take a snapshot at the tìme £ = 0, although, |
in fact, the picture is rotating with angular velocity œ (Fig. 29-9). The projection |
of Ai along the horizontal axis is precisely Ai cos (ð£ + ở). Now at £ =0 the |
second wave could be represented by another vector, 4a, of length 4a and at |
an angle ós, and also rotating. Phey are both rotating with the same angular |
velocity œ, and therefore the relafiue positions of the two are fxed. The system |
goes around like a rigid body. The horizontal projection oŸ Áa is 4a cos (0£ + da). |
But we know from the theory of vectors that if we add the bwo vectors in the |
ordinary way, by the parallelogram rule, and draw the resultant vector Án, the |
#-component of the resultant is the sum of the #z-components of the other two |
vectors. hat solves our problem. It is easy to check that this gives the correct |
--- Trang 509 --- |
result for the special case we treated above, where Ái = 4a = A. In this case, |
we see from Fig. 29-9 that Áp lies midway between 4+ and 4a and makes an |
angle 3(Óa — ới) with each. Therefore we see that Áp = 2Ácos 3(s — ới), a8 |
before. Also, as we see from the triangle, the phase of Ág, as it goes around, is |
the average angle of Áq and 4s when the two amplitudes are equal. Clearly, we |
can also solve for the case where the amplitudes are not equal, Just as easily. We |
can call that the geometrical way oŸ solving the problem. |
There is still another way of solving the problem, and that is the ønalfical |
way. hat is, instead of having actually to draw a picture like Fig. 29-9, we |
can write something down which says the same thing as the picture: instead of |
drawing the vectors, we write a complez mxwmber to represent each of the vectors. |
'The real parts of the complex numbers are the actual physical quantities. So in |
our particular case the waves could be written in this way: Aieff†1) [the real |
part of this is Ai cos (ø£ + ởi)| and Asef@f†22), Ñow we can add the two: |
h = Aiei@etrói) + Aasei6et92) = (Aie2t + Aac192)c«t (29.13) |
Ñ= Aic? + Aac!?2 = Ancl6n, (29.14) |
'This solves the problem that we wanted to solve, because it represents the result |
as a complex number of magnitude Áp and phase ón. |
To see how this method works, let us ñnd the amplitude An which is the |
“length” of f. To get the “length” of a complex quantity, we always multiply the |
quantity by its complex conjugate, which gives the length squared. he complex |
conjugate is the same expression, but with the sign of the 7's reversed. 'Phus we |
A? = (Aic'? + Aac??2)(Aie"??! + Aae”12), (29.15) |
In multiplying this out, we get 4ƒ + 443 (here the es caneel), and for the cross |
terms we have |
Ai4Aa(cft®i=4) + cit02~91)), |
e9 + e~?? = cosØ + isỉn Ø + cos Ø — ?sỉn 6. |
That is to say, e'? + e~? = 2cosØ. Qur fnal result is therefore |
4a = 4? + A2 + 2AI4a COS (Óa — Ị). (29.16) |
--- Trang 510 --- |
As we seo, this agrees with the length of Áp in Eig. 29-9, using the rules of |
trigonometry. |
Thus the sum of the two efects has the intensity 4? we would get with one |
of them alone, plus the intensity 43 we would get with the other one alone, |
plus a correction. 'Phis correction we call the mterƒference effect. It is really |
only the diference bebween what we get simply by adding the intensities, and |
what actually happens. We call it interference whether it is positive or negative. |
(Interference in ordinary language usually suggests opposition or hindranee, but |
in physics we often do not use language the way it was originally designedl) TỶ the |
Interference term is positive, we call that case construcfzue interference, horrible |
though it may sound to anybody other than a physicistl The opposite case is |
called des‡ructzue interference. |
Now let us see how to apply our general formula (29.16) for the case of Ewo |
oscillators to the special situations which we have discussed qualitatively. To |
apply this general formula, it is only necessary to fnd what phase diference, |
Ó1 — đa, ©exists between the signals arriving at a given point. (It depends only on |
the phase difference, of course, and not on the phase itself.) So let us consider |
the case where the two oscillators, of equal amplitude, are separated by some |
distance đ and have an intrinsic relative phase œ. (When one is at phase zero, the |
phase of the other is œ.) Then we ask what the intensity will be in some azimuth |
direction Ø from the E—W line. [Note that this is mof the same Ø as appears |
in (29.1). We are torn between using an unconventional symbol like lý, or the |
conventional symbol Ø (Fig. 29-10).| The phase relationship is found by noting |
that the diference in distance from ? to the two oscillators is đsin Ø, so that the |
phase diference contribution from this is the number of wavelengths in đsin 6, |
multiplied by 2z. (Those who are more sophisticated might want to multiply the |
wave number k, which is the rate of change of phase with distance, by đsin; |
Aell0tta) To Point P |
AeetZ đsin80 |
Fig. 29-10. 'Iwo oscillators of equal amplitude, with a phase differ- |
ence œ between them. |
--- Trang 511 --- |
1b is exactly the same.) The phase diference due to the distance difference is |
thus 2zdsin Ø/^À, but, due to the timing of the oscillators, there is an additional |
phase œ. So the phase diference at arrival would be |
Óa — Ôi = œ+ 2mdsin 0/À. (29.17) |
'This takes care of all the cases. 'Thus all we have to do is substitute this expression |
into (29.16) for the case 4 = 4a, and we can calculate all the various results for |
two antennas of equal intensity. |
Now let us see what happens in our various cases. The reason we know, for |
example, that the intensity is 2 at 30° in Eig. 29-5 is the following: the two |
oscillators are ¿À apart, so at 30°, dsin Ø = À/4. Thus ó¿ — ởị = 2mÀ/4ÀA = m/2, |
and so the interference term is zero. (We are adding two vectors at 909.) The |
result is the hypotenuse of a 45° right-angle triangle, which is v⁄2 times the unit |
amplitude; squaring it, we get ©wice the intensity of one oscillator alone. All the |
other cases can be worked out in this same way. |
--- Trang 512 --- |
})rffr-(rcff©ore |
30-1 The resultant amplitude due to ?øw equal oscillators |
'This chapter is a direct continuation of the previous one, although the name |
has been changed om /n#erference to Diffraction. No one has ever been able to |
defñne the diference between interference and difraction satisfactorily. It is just a |
question of usage, and there is no specife, important physical diference between |
them. The best we can do, roughly speaking, is to say that when there are only |
a Ífew sources, say ©wo, interfering, then the result is usually called interference, |
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