A Magneto-optic Polarization Readout Model

D. Campbell, D. Towner
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引用次数: 2

Abstract

Information stored on magneto-optic disks is typically read using a linearly polarized laser beam whose state of polarization is altered by the Faraday and/or polar Kerr effects upon reflection from the recording medium. Polarization sensitive optics are used to convert these media induced polarization changes into irradiance variations at photodetectors. Because the magneto-optic polarization effects are small (typically less than one degree of polarization rotation in the reflected beam) it is essential that the optical system introduce little additional polarization change if the recorded signal is to be recovered faithfully. This paper describes a polarization model that is used to predict the effects that real optical elements will have on the readout signals, noise, and ultimately, the signal to noise ratio of a magneto-optic recording system.
磁光偏振读出模型
存储在磁光盘上的信息通常使用线偏振激光束读取,其偏振状态由法拉第和/或极性克尔效应在记录介质反射后改变。偏振敏感光学用于将这些介质引起的偏振变化转化为光电探测器的辐照度变化。由于磁光偏振效应很小(通常在反射光束中小于1度的偏振旋转),因此如果要忠实地恢复记录的信号,光学系统必须引入很少的额外偏振变化。本文描述了一个偏振模型,用于预测实际光学元件对磁光记录系统的读出信号、噪声以及最终的信噪比的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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