北京锦坤科技有限公司 www.jon-kon.com
The ARCspectro-NIR (MIR) and ARCspectro-HT manufactured by ARCoptix are Fourier transform
spectrometers (FTS). Although this type of device is used for the same scope as more conventional grating
spectrometers - i.e. analyzing the spectrum of light - FTS operates in a different manner. This document
describes their basic working principle in a concise and didactical manner.
HOW DOES IT WORK?
A FT spectrometer is an interferometer. Its historical and most widely known configuration is the Michelson
interferometer, shown on Fig. 1. A beam-splitter is used for dividing the light to be spectrally analyzed into
two beams. After they have been reflected on two distinct mirrors, the two beams are recombined by the
same beam-splitter and sent to a detector. One of the mirrors is fixed, while the other is a movable mirror.
When the fixed and the movable mirrors are equidistant from the beam splitter (d=0) both beams travel
the same distance before reaching the detector. However, if the movable mirror moved away, one of the
light beams has to travel an additional distance δ = 2d (back and forth) called retardation, or optical path
difference.
MONOCHROMATIC LIGHT - INTERFERENCE
Let us first consider a perfectly monochromatic light source. At the detector, the recombined beams will
produce interference, which can be constructive&nbs*******bsp; destructive. If δ=0 (i.e. if the two mirrors are
equidistant from the beamsplitter)&nbs*******bsp; if δ is an integer multiple of the wavelengthλ (δ=nλ, with n
integer) then the two beams are said to be in phase are and constructive interference is produced: the
intensity at the detector is equal to the intensity of the source.
On the opposite, if δ=λ /2 or if 𝛿 is equal to δ=λ /2 plus an integer multiple of the wavelength λ (i.e. if
δ=(n+1)λ /2)
then the two beams are said to be in out of phase are and destructive interference is
produced: the intensity at the detector is zero.
For intermediate retardations δ, a smooth behaviour takes place. By scanning the movable mirror over
some distance, the intensity I(δ) recorded on the detector is a sinusoidal function:
Where I0 is the intensity of the source. Graphically, it looks like this:
The intensity I(δ) measured as a function of the retardation δ is called the interferogram. It is important to
understand that the period in the recorded interferogram depends on the light wavelength: the longer is
the wavelength, the larger is the period in the interferogram.
BI-CHROMATIC LIGHT
Let us consider a slightly more complicated situation where the light source emits at two discrete
wavelengths, which is illustrated on Fig. 3. The left graph schematically illustrates the spectra of such a bi-chromatic light. We have assumed that the shorter wavelength (blue) is less intense than the longer
wavelength (red).
Fig. 3 – Schematic representation of an interferogram produced by bi-chromatic light
The right-hand graph in Fig. 3 shows three interferograms. The upper interferogram is the one produced by
the spectral line with shorter wavelength and weaker intensity (upper blue). It has a short period and small
amplitude. The interferogram produced by the spectral line with longer wavelength and higher intensity
(middle red) has a longer period and larger amplitude. Due to the linearity of the process, the
interferogram that is effectively recorded by the photo-detector is simply the sum of the two other
interferograms (lower black curve).
In the example above, the two original wavelengths can still be distinguished quite clearly in the composed
interferogram. However, in more complex circumstances, it is usually not so evident. A mathematical
operation is needed for identifying the spectral intensity of the source starting from the measured
interferogram - called Fourier transform - which will be discussed further.
POLYCHROMATIC LIGHT
When the light source is characterized by a wide-band spectrum things are not so much different. For
example, consider the spectrum shown in Fig.4. Each spectral component of the light source can be
thought of producing an interferogram with its characteristic period, and whose amplitude is weighted by
the relative spectral intensity.
Again, the interferogram recorded by the detector is simply the sum of all these weighted monochromatic
interferograms (red line). Note that all wavelengths are simultaneously interfering constructively at the
zero retardation point (δ=0). This causes a strong intensity peak in the compound interferogram,
commonly called centerburst, which is typical of interferograms recorded with wide-band spectra. At larger
retardations, the modulation in the interferogram progressively dies-out. Indeed, the maxima of the
monochromatic interferograms are progressively going out of phase, thus they are cancelling each other.
FOURIER TRANSFORM
Mathematically speaking, the sum of the monochromatic interferograms simply turns into an integral (i.e.
not a discrete but a continuous summation). The recorded interferogram can by calculated by:
where S(υ) is the spectrum of the light source expressed in wave-numbers υ=λ/𝜆 (the inverse of the
wavelength, the so-called wave-number or spatial frequency). Do not bother too much on the fact that the
spectrum is expressed in terms of wave-numbers instead of wavelengths. The only reason is that the
integral, called (cosine) Fourier transform, has a slightly simpler mathematical form when expressed in
wave-numbers.
Getting the spectra from the interferogram
Usually, one is interested in the spectrum of the light source producing the interferogram. The Fourier
transform has the useful property of having an inverse, that allows calculating back the spectrum S(u) from
the interferogram I(δ). The inverse cosine Fourier transform is very simply expressed by:
In conclusion, the essential idea to remember is that there is a 1-to-1 correspondence between spectra and
interferogram. Each particular light spectrum is related to a unique interferogram, and each interferogram
corresponds to a unique spectrum. The mathematical relationship between the two is the Fourier
transform.
北京锦坤科技有限公司
www.jon-kon.com
电话：010-62530053，52494037
邮箱：jon_kon@163.com
地址：北京市海淀区农大南路1号硅谷亮城B座210室
The ARCspectro-NIR (MIR) and ARCspectro-HT manufactured by ARCoptix are Fourier transform
spectrometers (FTS). Although this type of device is used for the same scope as more conventional grating
spectrometers - i.e. analyzing the spectrum of light - FTS operates in a different manner. This document
describes their basic working principle in a concise and didactical manner.
HOW DOES IT WORK?
A FT spectrometer is an interferometer. Its historical and most widely known configuration is the Michelson
interferometer, shown on Fig. 1. A beam-splitter is used for dividing the light to be spectrally analyzed into
two beams. After they have been reflected on two distinct mirrors, the two beams are recombined by the
same beam-splitter and sent to a detector. One of the mirrors is fixed, while the other is a movable mirror.
When the fixed and the movable mirrors are equidistant from the beam splitter (d=0) both beams travel
the same distance before reaching the detector. However, if the movable mirror moved away, one of the
light beams has to travel an additional distance δ = 2d (back and forth) called retardation, or optical path
difference.
MONOCHROMATIC LIGHT - INTERFERENCE
Let us first consider a perfectly monochromatic light source. At the detector, the recombined beams will
produce interference, which can be constructive&nbs*******bsp; destructive. If δ=0 (i.e. if the two mirrors are
equidistant from the beamsplitter)&nbs*******bsp; if δ is an integer multiple of the wavelengthλ (δ=nλ, with n
integer) then the two beams are said to be in phase are and constructive interference is produced: the
intensity at the detector is equal to the intensity of the source.
On the opposite, if δ=λ /2 or if 𝛿 is equal to δ=λ /2 plus an integer multiple of the wavelength λ (i.e. if
δ=(n+1)λ /2)
then the two beams are said to be in out of phase are and destructive interference is
produced: the intensity at the detector is zero.
For intermediate retardations δ, a smooth behaviour takes place. By scanning the movable mirror over
some distance, the intensity I(δ) recorded on the detector is a sinusoidal function:
Where I0 is the intensity of the source. Graphically, it looks like this:
The intensity I(δ) measured as a function of the retardation δ is called the interferogram. It is important to
understand that the period in the recorded interferogram depends on the light wavelength: the longer is
the wavelength, the larger is the period in the interferogram.
BI-CHROMATIC LIGHT
Let us consider a slightly more complicated situation where the light source emits at two discrete
wavelengths, which is illustrated on Fig. 3. The left graph schematically illustrates the spectra of such a bi-chromatic light. We have assumed that the shorter wavelength (blue) is less intense than the longer
wavelength (red).
Fig. 3 – Schematic representation of an interferogram produced by bi-chromatic light
The right-hand graph in Fig. 3 shows three interferograms. The upper interferogram is the one produced by
the spectral line with shorter wavelength and weaker intensity (upper blue). It has a short period and small
amplitude. The interferogram produced by the spectral line with longer wavelength and higher intensity
(middle red) has a longer period and larger amplitude. Due to the linearity of the process, the
interferogram that is effectively recorded by the photo-detector is simply the sum of the two other
interferograms (lower black curve).
In the example above, the two original wavelengths can still be distinguished quite clearly in the composed
interferogram. However, in more complex circumstances, it is usually not so evident. A mathematical
operation is needed for identifying the spectral intensity of the source starting from the measured
interferogram - called Fourier transform - which will be discussed further.
POLYCHROMATIC LIGHT
When the light source is characterized by a wide-band spectrum things are not so much different. For
example, consider the spectrum shown in Fig.4. Each spectral component of the light source can be
thought of producing an interferogram with its characteristic period, and whose amplitude is weighted by
the relative spectral intensity.
Again, the interferogram recorded by the detector is simply the sum of all these weighted monochromatic
interferograms (red line). Note that all wavelengths are simultaneously interfering constructively at the
zero retardation point (δ=0). This causes a strong intensity peak in the compound interferogram,
commonly called centerburst, which is typical of interferograms recorded with wide-band spectra. At larger
retardations, the modulation in the interferogram progressively dies-out. Indeed, the maxima of the
monochromatic interferograms are progressively going out of phase, thus they are cancelling each other.
FOURIER TRANSFORM
Mathematically speaking, the sum of the monochromatic interferograms simply turns into an integral (i.e.
not a discrete but a continuous summation). The recorded interferogram can by calculated by:
where S(υ) is the spectrum of the light source expressed in wave-numbers υ=λ/𝜆 (the inverse of the
wavelength, the so-called wave-number or spatial frequency). Do not bother too much on the fact that the
spectrum is expressed in terms of wave-numbers instead of wavelengths. The only reason is that the
integral, called (cosine) Fourier transform, has a slightly simpler mathematical form when expressed in
wave-numbers.
Getting the spectra from the interferogram
Usually, one is interested in the spectrum of the light source producing the interferogram. The Fourier
transform has the useful property of having an inverse, that allows calculating back the spectrum S(u) from
the interferogram I(δ). The inverse cosine Fourier transform is very simply expressed by:
In conclusion, the essential idea to remember is that there is a 1-to-1 correspondence between spectra and
interferogram. Each particular light spectrum is related to a unique interferogram, and each interferogram
corresponds to a unique spectrum. The mathematical relationship between the two is the Fourier
transform.
北京锦坤科技有限公司
www.jon-kon.com
电话：010-62530053，52494037
邮箱：jon_kon@163.com
地址：北京市海淀区农大南路1号硅谷亮城B座210室
公安机关备案号：
