23.05.2014 Views

William Angerer - Department of Physics and Astronomy - University ...

William Angerer - Department of Physics and Astronomy - University ...

William Angerer - Department of Physics and Astronomy - University ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

53<br />

S-polarized<br />

P-polarized<br />

Figure 3.2: Prism pair to rotate p-polarized light to s-polarized light.<br />

the fundamental <strong>and</strong> second-harmonic beams constrains the second-order susceptibility<br />

elements probed. The fundamental output from a Ti:Ah03 laser is p-polarized<br />

(horizontally polarized). vVe used a simple combination <strong>of</strong> prisms [38] to rotate the<br />

p-polarized beam by 90° for the fundamental s-polarized measurements. As indicated<br />

by Fig. 3.2. the prism pair lowered the height <strong>of</strong> the fundamental beam. The original<br />

beam height was restored using a combination <strong>of</strong> gold coated mirrors. Although this<br />

optical setup is not the most elegant solution for converting a p-polarized beam into<br />

an s-polarized beam, it avoided the problem associated with using a half wave plate<br />

over a broad spectral range. In the latter case, for wavelengths far from the central<br />

operating wavelength <strong>of</strong> the half wave plate, the waveplate is unable to introduce a<br />

relative phase shift <strong>of</strong> IT between polarization components <strong>of</strong> the wave, <strong>and</strong> is therefore<br />

unable to rotate one linear polarization into another.<br />

Reproduced with permission <strong>of</strong> the copyright owner. Further reproduction prohibited without permission.

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

Saved successfully!

Ooh no, something went wrong!