Photoelastic-modulator-based differential frequency polarization modulation measurement and error analysis

2013 ◽  
Vol 21 (4) ◽  
pp. 876-883 ◽  
Author(s):  
王志斌 WANG Zhi-bin ◽  
张瑞 ZHANG Rui ◽  
赵冬娥 ZHAO Dong-e ◽  
陈友华 CHEN You-hua ◽  
魏海潮 WEI Hai-chao
1986 ◽  
Vol 40 (4) ◽  
pp. 498-503 ◽  
Author(s):  
R. T. Graf ◽  
F. Eng ◽  
J. L. Koenig ◽  
H. Ishida

Polarization modulation infrared ellipsometric spectra were collected on an FT-IR spectrometer, with the use of two linear polarizers and a photoelastic modulator. Samples consisted of thin poly(vinyl acetate) and poly(methyl methacrylate) films on gold substrates. The relative phase retardation (delta) and relative amplitude (psi) were derived from these measurements. These spectra were superior to those from static infrared ellipsometry measurements on the same samples. The thickness and optical constants of the films were calculated from the ellipsometric measurements and compared with reference optical constant spectra.


1995 ◽  
Vol 26 (4) ◽  
pp. 151-159 ◽  
Author(s):  
D Yang ◽  
J C Canit ◽  
E Gaignebet

Optik ◽  
2018 ◽  
Vol 157 ◽  
pp. 798-803
Author(s):  
Jing Liu ◽  
Kai You ◽  
Qiuling Zhao ◽  
Xia Wang

2016 ◽  
Author(s):  
Shuyuan Gao ◽  
Rongyi Ji ◽  
Yao Li ◽  
Zhi Cheng ◽  
Weihu Zhou

1992 ◽  
Vol 46 (1) ◽  
pp. 156-158 ◽  
Author(s):  
Kenji Tochigi ◽  
Hideto Momose ◽  
Yutaka Misawa ◽  
Takaya Suzuki

A polarization-modulation technique has been combined with Fourier transform infrared (FT-IR) spectrometry to eliminate the large background radiation which interferes with the infrared emission from thin organic films on metal surfaces. A step scan and a continuous scan interferometer which were combined with a photoelastic modulator were also studied, and the step scan system was found to be stabler and have a better S/N. The spectrum of a 12-nm perfluoropolyether film was obtained at 120°C by this system.


1982 ◽  
Vol 36 (5) ◽  
pp. 496-498 ◽  
Author(s):  
Elmer D. Lipp ◽  
Carl G. Zimba ◽  
Laurence A. Nafie ◽  
D. Warren Vidrine

In vibrational circular dichroism (VCD) measurements and other polarization modulation techniques, artifact signals often arise due to polarization sensitivity of the optical components located subsequent to the sample. In this paper, we describe a method for demodulating the light beam after passage through the sample in such a manner that only one linearly polarized state is allowed to reach the detector, thus eliminating these artifacts. The method is a beam reversal technique in which the light subsequent to the sample is redirected through the photoelastic modulator in such a way that the retardation produced on the first traversal through the modulator is removed. The light is returned to its original state of linear polarization prior to detection. The method is applicable to Fourier transform as well as to dispersive spectrometers since demodulation is effected for all wavelengths simultaneously. The results of preliminary demodulation experiments are presented and found to be more than 90% efficient in removing circular dichroism intensity of a birefringent origin.


1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


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