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In an area that isn't too extended, we may also regard , , as constant, and thus regard the motion as a system of plane waves. The direction constants , , of the wave normal are obviously to be determined from the condition

(43)

For , , , fall into , , , and the waves are perpendicular to . This is not the case if the light source is moving. From (43) follows, that the waves are perpendicular to the line that connects P with that point at which the light source was at the moment, when the light was sent that reaches P at time t.

The law of Doppler.

§ 37. In a point that moves together with the luminous molecule — and thus also for an observer who shares the translation — the values of are changing, as we have seen (§ 30), as often in unit time as it corresponds to the actual period of oscillation T of the ions.

We can also examine, with which frequency these values in a stationary point are changing their sign. This frequency causes the oscillation period for a stationary observer. The question can be solved immediately, if instead of x, y, z we introduce new coordinates , , , which refer to a stationary system of axes. If the two systems have the same directions of axes and the same origin at time t = 0, then

(44)

and by (42) for we obtain expressions of the form

where