Difference between revisions of "Kerr - June 30, 2016"

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[[file:LRappmin.jpeg|thumb|upright=2|In this graph the measured powers at the left and right of the minimum are in relation to a arbitrary rotation with 0 being perfect perpindicular interception of the polarizers.]]
 
[[file:LRappmin.jpeg|thumb|upright=2|In this graph the measured powers at the left and right of the minimum are in relation to a arbitrary rotation with 0 being perfect perpindicular interception of the polarizers.]]
[[file:Bvsdistance.jpeg|thumb|upright=2|This relationship will be important down the road for further Kerr effect calculations. The fit at this time is not completely accurate, I plan to touch it up when a presentation is closer or when I have some down time. ]]
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[[file:Bvsdistance.jpeg|thumb|upright=2|This relationship will be important down the road for further Kerr effect calculations. The fit at this time is not completely accurate, I plan to touch it up when a presentation is closer or when I have some down time.]]
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I also graphed a normalized version of minimum approaching data set. However, I am concerned that both of these shapes are not able to fit to our standard &Delta; p = A*sin<sup>2</sup> &theta;
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After a few attempts to fit with excel, I was unsuccessful. I may have to utilize Extrema or Canopy with Python.

Revision as of 21:39, 30 June 2016

In this graph the measured powers at the left and right of the minimum are in relation to a arbitrary rotation with 0 being perfect perpindicular interception of the polarizers.
This relationship will be important down the road for further Kerr effect calculations. The fit at this time is not completely accurate, I plan to touch it up when a presentation is closer or when I have some down time.

I also graphed a normalized version of minimum approaching data set. However, I am concerned that both of these shapes are not able to fit to our standard Δ p = A*sin2 θ

After a few attempts to fit with excel, I was unsuccessful. I may have to utilize Extrema or Canopy with Python.