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How to get the polarization state of the reflected light?
Posted 2016年3月21日 GMT-4 08:55 Wave Optics 7 Replies
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I have been working on the magneto-optical effect. A linearly polarized light is reflected by a magnetized film, Cobalt film for example. The reflected light is supposed to be ellipcitally polarized. Then is it possible to get the polarization state of this ellipcitally polarized, i.e., the polarization rotation and ellipticity?
All ideas will be appreciated. Thanks in advance!
Best regards,
Xiaokun
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Since "An elliptical polarized state just means there is a phase shift between the field in different directions", so what I need to do is to measure the amplitudes and phases of the in-plane and out-of-plane components of the reflected field.
Under the default coordinate system, for p-polarized incidence, after Kerr reflection, the in-plane component would be Ex+Ez, and the out-of-plane component would be Ey. For s-polarized incidence, however, it is hard to tell the two components giving rise to the the Kerr rotation and ellipticity. Am I right?
best regards,
Xiaokun
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I do not really understand your concerns. Since I'm not working on this subject, please correct me if I am wrong.
As far as I know, after a wave is reflected by a magnetic-optic film, there will be two components. One is the "normal component". By normal it means it has the same polarization as the incident wave as s-polarized or p-polarized. The other component is the so-called "Kerr component", the direction of this component will depend on the magnetization direction. There will be a phase different between the normal component and the Kerr component. And this makes the total reflected field elliptical. So I guess the phase and amplitude difference of these two components are the qualities you need to measure, to calculate the ellipticity, right?
If so, you can always measure all components of the total reflected field (total field minus incident field, or use port) in a Cartesian coordinate, then do the math yourself to decomposite them into the normal component and the other component with respect to the direction of k. Do I understand correctly?
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As far as I am concerned, it is totally correct for your description of the reflected light by a magnetized surface, being the known Magneto-optical Kerr Effect (MOKE).
What I was wondering all these days is that whether the COMSOL is able or not to give the information about the amplitude and phase difference of both normal component and Kerr component. And from your response, it seem to be positive to obtain them by measuring the total reflected field and then decomposing it into those two components. This is quite inspiring!
It's just, I am a rookie in comsol. I am still working on how to measuring the reflected field.. I could understand the "total field minus incident field" approach using the expression like "Ex-Ein" (total-incidence), right? However, what do you mean by "use ports"? Could you explain a little bit more?
Thank you so much!
Xiaokun
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To measure the amplitude and phase of both components, I actually have two ideas in my mind.
1) Using "scattered field" instead of "full field" solver. In this way, you can easily get the scattered field ( say, emw.relEx) conveniently, which is exactly "totalfield (emw.Ex) minus incident field (emw.Ebx)".
2) Using port. You can set two orthogonal ports ( e.g. with two different polarizations ) to absorb the reflected waves separately, and use S-parameter to calculate their amplitudes and phases.
Best regards.
Peng
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The explanation couldn't be more explicit. I will try those two methods and if there is more question coming up, I'll turn to you for help in this thread. Thanks again!
Best,
Xiaokun
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In the figure found attached, Q is the magneto-optical constant, and m is the normalized magnetization, that is, it assumes values between 0 and 1.
Thanks.
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