Page:Zur Theorie der Strahlung in bewegten Körpern.djvu/12

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Then it is

(22)

When we neglect magnitudes beginning with order , it becomes

(23)

Thus, is evidently the density of true radiation. In order to calculate , i.e., the density of the apparent radiation, we have to know the values of and , with which we want to concern ourselves in the following section.


§ 4.

According to Abraham, the radiation pressure upon a moving plane is equal to the radiation incident or emanating in unit time (in our terminology, this is the total relative radiation) divided by the speed of light; namely, this pressure is acting in the direction of the absolute propagation in the sense of the negative normal. Since we understood and as perpendicular pressure components, it is thus:

If we divide away the same factors at both sides, and if we insert for its value from (6), then under consideration of the corresponding sign:

(24a)
(24b)

If we insert this into equations (17), then we obtain

(25a)
(26a)