12.11.2014 Views

Introductory Physics Volume Two

Introductory Physics Volume Two

Introductory Physics Volume Two

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

7.8 Far Field Approximation 151<br />

§ 7.8 Far Field Approximation<br />

In most cases the detector is placed far from the two sources, far<br />

in the sense that the distance from the sources to the detector r is<br />

much bigger than the distance between the sources, d. There is a<br />

useful approximation for the path difference that can be used when the<br />

detector is far from the source.<br />

First consider the case when the detector<br />

is not far, as pictured in the figure to<br />

Detector<br />

the right. Notice that if we make of a section<br />

of arc, with the center at the detector,<br />

Source<br />

and going through the closest source, and<br />

then consider the section of the path from<br />

the furthest source that is cut off by this<br />

arc. This cut off section (marked as ∆r in<br />

the figure) is equal to the path difference.<br />

Δr<br />

Also notice that the arc is perpendicular to<br />

Source<br />

the path.<br />

Now imagine moving the detector further from the sources, as<br />

pictured in the diagram below. The section of arc that is between the<br />

two paths, subtends a smaller and smaller angle, and thus this section<br />

of arc becomes closer and closer to a straight line. At the same time<br />

the grey region becomes a right triangle.<br />

θ<br />

Let us examining this right triangle<br />

more closely. We see from the diagram<br />

to the right that<br />

sin θ = ∆r −→ ∆r = d sin θ<br />

d<br />

This is a very useful result, that allows<br />

us to find the path difference from the<br />

distance between the sources and the angle<br />

to the detector.<br />

Combining this with our previous result, ∆r = m λ 2<br />

, we find the<br />

d<br />

θ<br />

Δr<br />

θ

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!