To use a razorblade to measure beam waist at four points along the optical axis, so as to later extrapolate the waist. This information will then be used to effectively couple AUX laser light to fibers for use in the frequency offset locking apparatus.
1) Step the micrometer-controlled razorblade across the beam at a given value of Z, along optical axis, in the plane orthogonal to it (arbitrarily called X).
2) At each value of X, record the corresponding output of a photodiode, (Thorlabs PD A55) here given in mV.
3) Repeat in Y plane at the same value of Z
4) Repeat process at multiple points along Z
Data from each iteration were fitted to the error function shown below.
y(x) = (.5*P)*(1-erf((sqrt(2)*(x-x0))/wz))
'P' corresponds to peak power, 'x0' to the corresponding value of x (or y, as the case may be), and 'wz' to the spot size at the Z value in question.
The spot sizes from the four Z values were then fit to:
y(x) = w0*sqrt(1+((x*x)/(zr*zr)))
Where 'w0' corresponds to beam waist, and 'zr' to Rayleigh Range.
This yielded a Y-Waist of 783.5 um, and an X-Waist of 915.2 um.
The respective Rayleigh ranges were 2.965e+05 um (Y) and 3.145e+05 um (X).
I will do the same analysis with light from the optical cables, which information I will then use to design a telescope to effectively couple the beams.