Advances in OptoElectronics
Volume 2015 (2015), Article ID 472852, 4 pages
http://dx.doi.org/10.1155/2015/472852

Research Article

Analysis of the Interference Modulation Depth in the Fourier Transform Spectrometer

Rilong Liu

School of Engineering, Jiangxi Agricultural University, Nanchang 330045, China

Received 21 August 2015; Revised 14 September 2015; Accepted 20 September 2015

Academic Editor: Michele Norgia

Copyright © 2015 Rilong Liu. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract.

Based on the principle of the Michelson interferometer, the paper briefly describes the theoretical significance and calculates and deduces three expressions of the interference modulation depth. The influence of the surface shape error of plane mirror on modulation depth is analyzed, and the tolerance of error is also pointed out. Moreover, the dependence of modulation depth on the reflectance change of beam splitter interface is also analyzed, and the curve is given. It is concluded that this paper is of general significance for the Fourier transform spectrometer based on the principle of the Michelson two-beam interference.

1. Introduction

The Fourier transform spectrometer is an instrument which is used to analyze the spectral distribution of the light source by means of the interference effect based on the Fourier transform technology. It has incomparably more advantages than conventional spectral instruments in acquiring higher spectral resolution. There are many kinds of Fourier transform spectrometers, including Michelson interferometer, Fabry-Perot interferometer, Sagnac interferometer, and double refraction interferometer [1, 2].

The classical Michelson interferometer consists of a moving mirror and a fixed mirror. The two beams of lights, reflected by these two mirrors, make up the phase difference. When the moving mirror moves, the intensity of interference signals is modulated to form the interferogram. The modulation depth is also known as the interference modulation efficiency. It is one of the most important factors influencing the signal-to-noise ratio of the interferogram, and a change in it will significantly affect the sensitivity of the spectrometer [3, 4]. Based on the Michelson type Fourier transform spectrometer, this paper explores the optical principle of interference system through a quantitative analysis of influencing factors of surface shape of mirror and performance change of beam splitter. It is hoped that suggestions can be made for the obtaining of ideal interferogram.

2. The Modulation Depth of Fourier Transform Spectrometer

The most classical Fourier transform spectrometer is the Michelson interferometer, which is composed of a fixed mirror, a moving mirror, a beam splitter, and a detector. Its basic structure is shown in Figure 1.

Figure 1: Basic structure of Michelson interferometer.

In the Michelson interferometer, the fixed mirror and the moving mirror are perpendicular to each other, with an angle of 45° between the beam splitter and two mirrors. The collimated beam shines the interference system, and the beam splitter separates the incident light into two beams with roughly the same reflectance and transmittance. One reflected beam by the fixed mirror then goes through the beam splitter again, whereas the other transmitted beam is reflected by the moving mirror and divided by the beam splitter. Because these two beams of light are produced by the same beam, they have a constant phase difference. When these two beams of light travel through a convergent lens, the interference is formed on the detector.

Upon arrival at the detector, the two coherent beams have an optical path difference for the shift of the moving mirror. The optical path difference then shows periodic changes with round-trip translation of the moving mirror. According to the principle of interference spectroscopy, the interference signals can be obtained on the detector.

According to the interference theory, the intensity of interference signals generated by the two-beam interference is [5]

where and are, respectively, the intensity of two coherent beams and is the phase difference of two coherent beams.

The definition of the modulation depth of interference signals, namely, the visibility of interference signals , is

This equation indicates the degree of bright dark contrast of fringes in the interference field, where and stand for the maximum intensity and the minimum intensity of interference signals. We then get the following equation:

Then (1) can be rewritten as

From (3), we can have the coefficient of the cosine, namely, the modulation depth, after we obtain the distribution of the cosine light intensity, and normalize the constant term. If and only if , that is to say, when the intensity of two coherent beams of light is equal, the modulation depth reaches a maximum and also an ideal . However, with practical applications taken into consideration, the modulation depth will usually be less than 1.

3. The Surface Shape Error of Plane Mirror

The fixed mirror and the moving mirror of Fourier transform spectrometer are composed of plane mirrors with a rectangular aperture. In the process of making plane mirrors, there are a number of factors modulating the surface error, such as polishing, coating, and mirror bending. It follows that these mirrors are not ideal surface shape, and there is always a certain surface error. Therefore, in a spectrometer composed of these mirrors, the modulation depth is often not ideal. In what follows, we will analyze the influence of curve error and polishing error of plane mirror on interference modulation depth. Suppose polishing error of mirror obeys normal distribution with zero mean, and its maximum fluctuation is . In addition, curve error of mirror is subject to uniform distribution, and its maximum curvature is . Assume also that other optical components in Fourier transform spectrometer are ideal.

When there is a surface shape error of plane mirror, the reflection of two beams of coherent light will generate wavefront distortion, which results in a change in optical path difference of interferometer. The phase difference of the two beams of coherent light changes accordingly. For a small change of the surface shape error, the change of the phase difference is

where is the wave number of the incident light. Suppose is the probability density function of surface shape error. If , then we obtain surface . Because of the effect of surface shape error, the intensity of interference signals is [6]

where represents the distribution of interference intensity in any one point. The probability density function is

where is the standard deviation of .

When is substituted to (6), we can get the intensity of interference signals:

Hence, the interference modulation depth is

It can be seen that the interference modulation depth is inversely proportional to the variance of polishing error of mirror, which means that a good polishing surface can improve the modulation depth. If the interference modulation depth is set at , the error tolerance of standard deviation is

In the same way, when the mirror surface is curved, the existence of the curve error causes the intensity distribution of the interference signals to be

It follows that, when the surface of mirror is deformed, the interference modulation depth is

Equation (12) shows that is a function of sinc, and the modulation depth decreases when the curvature increases. If the interference modulation depth is set at , the error tolerance of the curvature is

Through the above analysis, we know that the surface error of mirror has an effect on the modulation depth. In order to achieve better interference effect, the surface error of mirror should meet error tolerance requirements.

4. The Reflectance Change of Beam Splitter Interface

In the Michelson interferometer shown in Figure 1, the separating surface of the beam splitter is coated with transflective film. Suppose and represent the amplitude reflection coefficient and the amplitude transmission coefficient of beam from the surrounding medium into surface of the beam splitter, respectively. Meanwhile, and are the amplitude reflection coefficient and the amplitude transmission coefficient of beam from surface of the beam splitter into the surrounding medium, respectively. At the same time, is the amplitude reflection coefficient of fixed mirror, and is the amplitude reflection coefficient of moving mirror, and stands for the amplitude of incident light [7, 8]. The complex amplitude of the two beams of light reflected by Michelson interferometer, respectively, is

where is the wave number of the incident light, while and represent optical path of two beams of light, respectively. Generally speaking, if the amplitude reflection coefficient of the fixed mirror equals that of the moving mirror, that is, , then we get

From (15), the modulation depth can be expressed as

According to the Fresnel formula, the amplitude reflection coefficient and the amplitude transmission coefficient satisfy the following conditions:

And the interface reflectance of the beam splitter is

Then substituting (18) into (17), we can get

Thus, the interference modulation depth is

From (20), it can be seen that the interference modulation depth will change with the interface reflectance of the beam splitter. Their relationship is captured in Figure 2.

Figure 2: Influence of reflectance change of beam splitter on modulation depth.

From Figure 2, the smaller the interface reflectance of the beam splitter is, the greater the interference modulation depth becomes. To put it another way, if value is 0, then . When the interference modulation depth is set at , is

5. Experimental Results

The analysis of interference modulation depth indicates that, in order to realize the interference modulation depth , the maximum value of the curve error of mirror should be . Figure 3 presents measured results of the surface of the plane mirror with the aid of Zygo interferometer. As can be seen from Figure 3, the plane mirror has a good surface, with the PV value .

Figure 3: The surface shape of plane mirror.

The interferometer is placed on the testbed, and the interference is formed by using the He-Ne laser. The electrical signal of the laser interference can then be acquired. Figure 4 provides the interference signal generated by the laser light source.

Figure 4: The electrical signal of the laser interference.

As can be seen from Figure 4, the laser interference signal is a sinusoidal signal, and the amplitude of the interference signal is stable and the fringe is clearly visible, which meets the requirement of the interference modulation depth.

6. Conclusions

In the Fourier transform spectrometer, the Michelson interferometer is the core optical system. By focusing on the classic Michelson interferometer, we have conducted a theoretical analysis of the influence of surface shape of mirror and performance change of the beam splitter on the modulation depth. Theoretical deductions are obtained regarding tolerance requirements for the error of surface shape mirror and the reflection ratio of the beam splitter. The results obtained are applicable to the Fourier transform spectrometer within the framework of the Michelson dual beam interference.

Conflict of Interests

The author declares that there is no conflict of interests regarding the publication of this paper.

Acknowledgment

The research was supported by the Program for Science and Technology funded by the Education Department of Jiangxi Province (GJJ14316).

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