1. Field of the Invention
The present invention relates a dispersion compensation device used in optical communication.
2. Description of the Related Art
When an optical signal pulse transmission is performed using an optical fiber, a speed of transmission through the optical fiber differs depending on a light wavelength. Therefore, as a transmission distance increases, a signal pulse waveform flattens. This phenomenon is referred to as wavelength dispersion. When the wavelength dispersion is generated, a reception level is significantly degraded. For example, when a single mode fiber (SMF) is used, a wavelength dispersion of −15 to −16 ps/nm·km is generated near a wavelength of 1.55 micrometers (μm) that is often used in optical pulse communication. In wavelength dispersion compensation (referred to as dispersion compensation), wavelength dispersion of the same amount as the wavelength dispersion generated when the optical fiber is used is conversely added.
Currently, a dispersion compensating fiber (DCF) is the most common optical fiber used to perform dispersion compensation. The DCF is designed to generate dispersion (structure dispersion) that is an opposite of material dispersion of a fiber material. The opposing dispersion is generated by a specific refractive index distribution. In total, the DCF generates dispersion that is an opposite of dispersion generated in an ordinary SMF (dispersion compensation of about 5 to 10 times the amount generated in an SMF of a same length). The DCF is connected to the SMF at a relay station, and a total dispersion is zero (cancelled).
In recent years, in response to increasing communication demands, further increase in capacity is required for large, capacity transmission using wavelength division multiplexing (WDM). In addition to reduction in intervals between wavelength multiplexing, increase in communication speed is required (for example, 40 Gb/s). As a result, wavelength dispersion tolerance decreases when relay distances are the same. Temperature fluctuations generated when the wavelength dispersion is generated using SMF also requires compensation. The temperature fluctuations are conventionally not a problem. An actualization of a wavelength dispersion compensator that can change the compensation amount is required, in addition to the conventional fixed type DCF.
Specifically, a wavelength division type optical dispersion compensator using an etalon (for example, Japanese Patent Laid-open Publication Nos. 2002-267834 and 2003-195192). A tunable optical dispersion compensator using a reflective etalon is disclosed as a reflection type wavelength dispersion compensator (for example, Japanese Patent Laid-open Publication No. 2004-191521).
There is a wavelength dispersion compensator in which etalons that differ from each other in a group delay and a center wavelength are connected optically in series (for example, Japanese Patent Laid-Open Publication No. 2003-264505).
The optical circulator 2002 outputs light input from the input unit 2001 to the etalon 2003a, outputs light output from the etalon 2003a to the etalon 2003b, and outputs light output from the etalon 2003b to the output unit 2004.
The etalons 2003a and 2003b are the etalon 1010 explained in
When the center wavelengths of the group delay characteristic 2101 and the group delay characteristic 2102 are shifted by half the wavelength cycle interval FSR, as shown in
The center wavelength of a group delay characteristic varies corresponding to thickness of an etalon substrate. Therefore, by adjusting the thickness of the etalon substrate by changing the temperature of the etalon substrate of the etalon 2003a using the power source 2006 and the temperature control unit 2007, the center wavelength of the group delay characteristic can be changed. Thus, the dispersion compensation amount can be changed.
However, the reflective film 1011 included in the etalon 1010 has low manufacturability and low uniformity.
Furthermore, because the deposition mask 1050 is used, a vapor-deposition material tends to leak onto a back surface of the deposition mask 1050. Therefore, it is difficult to form the layer in a uniform thickness, and special measures are required to be taken to solve the leakage. As a result, the etalon, which is a main component of the tunable optical dispersion compensator, becomes costly. In addition, it becomes difficult to acquire desired characteristics regarding the dispersion compensation amount of the tunable optical dispersion compensator.
Moreover, in the tunable dispersion compensator 2000 shown in
It is an object of the present invention to at least solve the above problems in the conventional technologies.
A wavelength dispersion compensation device according to one aspect of the present invention includes an etalon in a slab shape having at least two surfaces opposite to each other. The etalon includes reflective films formed on the surfaces respectively. One of the reflective films has incident angle dependence in which reflectance differs depending on an incident angle of the light, and has a filter characteristic in which the reflectance abruptly changes in a range of wavelength of light to be used for the wavelength dispersion compensation.
The other objects, features, and advantages of the present invention are specifically set forth in or will become apparent from the following detailed description of the invention when read in conjunction with the accompanying drawings.
Exemplary embodiments of the present invention will be explained in detail below with reference to the accompanying drawings.
A light incident angle of light incident on the etalon 100 continuously changes. Light A1 has a perpendicular incident angle to the reflective film 103. Light An has a predetermined angle. By varying the light incident angle, the group delay amount is varied, thereby changing the dispersion compensation amount.
Therefore, when the light incident angle is changed by 10 degrees, the reflectance can be changed within a range of 20% to 65%. A characteristic of the reflective film 103, such as the above, can be actualized by setting the wavelength range to be used, to a portion (edge portion) at which filter characteristics of an optical band pass filter (BPF) and an optical band rejection filter (BRF) rapidly change. In addition, a state of changes in the reflectance with respect to the wavelength (a change rate and an angle of a characteristic line (slope)) can be arbitrarily set by adjusting the total number of layers in the reflective film 103 and thickness of each layer.
In the reflectance characteristic shown in
As shown in the diagram, the light emitted from the collimator 510 passes through the etalon 100a and the etalon 100b, and then, the light is reflected by a reflective body 520 to be returned. A returning path is sequentially returned through the etalon 100b and then the etalon 100a, and the light is incident on the collimator 510. The wavelength dispersion compensation module 500 has four stages structure in total in both ways.
The two etalons 100a and 100b are arranged on a stage 502. The stage 502 is rotatable about a rotation center of the stage 502 that is an approximately intermediate position between the two etalons 100a and 100b. The stage 502 is rotated by a rotation mechanism, and functions as an incident angle changing unit to change the incident angle of the light incident on the etalon 100a. The light is emitted from the collimator 510 that is an optical port. The rotation mechanism includes an extruding mechanism 530 and a biasing mechanism 540. The extruding mechanism 530 and the biasing mechanism 540 are provided beside the stage 502. The extruding mechanism 530 includes a combination of a stepping motor and a gear, or a piezo element and the like. In the extruding mechanism 530, a differential piece 531 extrudes a protrusion piece 502a of the stage 502 and rotates the stage 502. The biasing mechanism 540 includes a return spring and generates a bias force in a direction opposite of an extrusion direction of the extruding mechanism 530. The bias force is transmitted to a protrusion piece 502b of the stage 502, via a differential piece 541.
According to the wavelength dispersion compensating module 500, the stage 502 is rotated by the extruding mechanism 530 being operated. Due to the rotation, the incident angle of the light emitted from the collimator 510 to the two etalons 100a and 100b can be changed. For example, as shown in
According to the configuration shown in
According to the configuration shown in
According to the first embodiment explained above, the reflective film having a different reflectance depending on the light incident angle can be easily formed. Therefore, the manufacturability of the etalon can be improved, and the wavelength dispersion compensation device can be manufactured at a low cost. Furthermore, the reflectance can be made wavelength dependent. As a result, a wavelength dispersion compensation module that corresponds to required dispersion compensation characteristics can be manufactured.
The etalon substrate 101 can be formed with silicon or zinc selenide that are high-refraction materials. By a use of the high-refraction material, the changes in the wavelength interval caused by the changes in the light incident angle can be suppressed. Therefore, a variable range (number of wavelengths) can be increased.
The light output to the two etalons 100a and 100b is reflected at the etalons 100a and 100b to a planar mirror 703. The planar mirror 703 reflects the light from the two etalons 100a and 100b back to the etalons 100a and 100b. The light returned by the planar mirror 703 is reflected again at the two etalons 100a and 100b, passes through the collimator 702, and is output from the input/output fiber 701.
The two etalons 100a and 100b rotate about the same axis (see, for example, the rotation mechanism in
Moreover, the reflectance (%) of the reflective film 103 is indicated by R. A phase shift amount h (λ) can be expressed by Equation 1 below when the optical path length of the etalon 100 is L1, a refractive index of the etalon substrate 101 is n, and the wavelength of light to be input is λ.
h(λ)=exp[−j2π·L1·n/λ] (1)
Furthermore, the optical path length L1 can be expressed by Equation 2 below using the thickness t of the etalon substrate 101 and the incident angle θ of light to the reflective film 103.
L1=2·t/√{square root over ((1−(sin θ/n)2))} (2)
A transfer function H (λ) can be expressed by Equation 3 below using the reflectance R of the reflective film 103 and the attenuation ratio A of reflection at the reflective film 103.
A group delay D (λ) can be expressed by Equation 4 below in which a phase part argH (λ) in the transfer function and is differentiated by ω(=2πc/λ).
D(λ)=−(λ2/2πc)(d/dλ)(argH(λ)) (4)
Relation between the wavelength cycle interval FSR (Hz) of the group delay D (λ) and the optical path length L1 is determined by h (λ) having periodicity, and is a change of λ in which an element L1·n/λ of this h (λ) is integrally multiplied. The wavelength cycle interval FSR (Hz) can be expressed by Equation 5 below when a speed of light is C.
FSR(Hz)=C(L1·n),C(speed of light) (5)
Furthermore, the thickness t of the etalon substrate 101 when the wavelength cycle interval FSR (Hz) of the group delay D (λ) and the incident angle θ are specified can be expressed by Equation 6 below.
t=C/(2·n·FSR·√{square root over (1−(sin θ/n)2)}) (6)
Numerals 1001 to 1003 indicate settings 1 to 3, respectively. For the setting 1, the incident angle θ of light to the reflective film 103 of the etalon 100a from the input/output fiber 701 is set as 2.0 deg, the temperature of the etalon substrate 101 of the etalon 100a is set as 73° C., and the temperature of the etalon substrate 101 of the etalon 100b is set as 73° C. The center wavelength of the group delay characteristic in the etalon 100a is 1546.76 nm, and the center wavelength of the group delay characteristic in the etalon 100b is 1546.92 nm. In the setting 1, a group delay characteristic of −33.25 ps/nm can be obtained.
Next, the setting 2 to obtain a group delay characteristic of a dispersion compensation amount larger than that in the setting 1 is explained.
As described, in a region of a large compensation amount, the dispersion compensation amount can be adjusted by changing the incident angle θ of light to the reflective film 103 of the etalon 100a from the input/output fiber 701. The center wavelength of the group delay characteristic of the etalon 100 is determined by the optical path length L1 of the etalon 100. Therefore, when the incident angle θ of light is changed, the optical path length L1 changes, and the center wavelength of the group delay characteristic changes. It is necessary to suppress a change of the center wavelength by adjusting the optical path length L1 of the etalon 100.
For example, the optical path length L1 is controlled by adjusting temperature of the etalon substrate 101. Specifically, configuration may be such that a Peltier device and a control unit of the Peltier device are provided in at least one of the etalons 100a and 100b, and the temperature of the etalon substrate 101 is changed by the Peltier device (see
L1(θ+δ)=2·t/√{square root over ((1−(sin(θ+δ/n)2))} (7)
The refractive index n of the etalon substrate 101 and the thickness t of the etalon substrate 101 in Equations 1 to 6 above are dependent on temperature, and the refractive index n (T) of the etalon substrate 101 can be expressed by Equation 8 below when an initial temperature of the etalon substrate 101 is T0, a control temperature of the etalon substrate 101 is T, a change of the refractive index n of the etalon substrate 101 according to the temperature control is (dn/dT)NdT, and a linear expansion coefficient is α. Furthermore, the thickness t of the etalon substrate 101 can be expressed by Equation 9 below.
n(T)=n0·(1+NdT(T−T0)) (8)
t(T)=t0·(1+α(T−T0)) (9)
Therefore, a condition to make L1·n constant can be expressed by Equation 10 below.
For example, when the etalon substrate 101 is made of quartz and the wavelength of light to be input is 1550 nm, NdT is 9×10−6, and the linear expansion coefficient α is 5·5×10−7. Therefore, to increase the incident angle θ, it is necessary to control (decrease) the temperature of the etalon substrate 101 from the initial temperature T0. As a realistic temperature variable range, it is, for example, set to approximately 50° C. at the maximum.
Next, the setting 3 to obtain a group delay characteristic of a dispersion compensation amount smaller than that in the setting 1 is explained.
While in the region of a large compensation amount, the optical path length L1 (temperature) is controlled to be the same optical path length L1, in a region of a small compensation amount, for example, the optical path length L1 (center wavelength) of the etalon 100a is changed to shift the center wavelength by half the wavelength cycle interval (FSR), thereby obtaining the dispersion compensation amount of 0. By further shifting the center wavelength, inverse compensation is also possible.
In the region of a small compensation amount also, the dispersion compensation amount can be varied by changing the incident angle of light to the reflective film 103 of the etalon 100a. The reflective film 103 is designed such that the reflectance increases as the incident angle increases in the used wavelength band, and the temperature control range in the region of a large compensation amount and the temperature control range of the region of a small compensation amount are used in common, thereby enabling use in a realistic temperature range.
As described, with the wavelength dispersion compensation device according to the second embodiment, the effects of the wavelength dispersion compensation device according to the first embodiment can be achieved, and the dispersion compensation amount can also be set to 0 by connecting a plurality of etalons having different reflection characteristics optically in series.
Depending on the incident angle of light from the input/output fiber 701 to the etalon 100a (for example, in the case of the light beam 1211), interference between an edge 1220 of the etalon 100a and the light can occur when light is emitted from the two etalons 100a and 100b. The interference becomes more likely to occur as the number of stages in which light is reflected at the etalons 100a and 100b are increased.
With this configuration, even if the number of stages in which light is reflected at the etalons 100a and 100b is increased, the distance between the two etalons 100a and 100b does not increase, and therefore, it is possible to avoid a size increase of the device. Moreover, since the rotation angle of the two etalons 100a and 100b and the distance between the two etalons 100a and 100b have a one-to-one correspondence, one-dimensional control is also possible.
A distance P between reflection points of light at the etalon 100a or the etalon 100b can be expressed by Equations 11 to 13 below when the distance between the etalons 100a and 100b is W.
P(θ+δ)=2·W·tan(θ+δ) (11)
P(θ)=2·W·tan(θ) (12)
ΔP=2·W·(tan(θ+δ)−tan(θ)) (13)
When the distance W between the two etalons 100a and 100b is constant, and the number of stages in which light is reflected at the two etalons 100a and 100b is m, an amount of change mΔP, where ΔP is an amount of change in the distance P, must be canceled if present. By controlling the distance W between the etalons 100a and 100b as in Equation 14 below, P can be made constant. Therefore, it is possible to prevent the interference between the edge of the etalon 100a and light when the light is output from the two etalons 100a and 100b.
W(δ)=P(θ)/2 tan(θ) (14)
Configuration may be such that a point at which light enters the etalon 100a first is a rotation axis of the etalons 100a and 100b. With this arrangement, when configuration is such to return light output from the two etalons 100a and 100b by a mirror, an optical path of the returned light can be fixed to a position of an incident port even if the rotation angle of the etalons 100a and 100b changes. Therefore, it is not necessary to provide a mechanism to adjust the position of the port corresponding to the rotation angle of the two etalons 100a and 100b.
The recursive mirror 1513 reflects the light beam reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b as the height thereof changes (shifts). The recursive mirror 1513 is configured with two planar mirrors so that the optical path of the light beam before and after the reflection becomes parallel. The light beam returned by the recursive mirror 1513 is reflected again at the two etalons 100a and 100b.
At a position at which the light beam reflected again by the two etalons 100a and 100b is emitted, a returning planar mirror 1514 is provided. The returning planar mirror 1514 reflects the light beam reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b. The wavelength dispersion compensating module 1510 shown in
With the configuration shown in
As described, by multistaging in a vertical direction using the recursive mirror 1513, the dispersion compensation amount can be increased without increasing the number of stages in a horizontal direction. Therefore, it is possible to increase the dispersion compensation amount while suppressing the interference between the edge of the etalon 100a and light.
At a position at which the light beam reflected by the two etalons 100a and 100b is emitted, a recursive mirror 1523 is provided. The recursive mirror 1523 reflects the light beam reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b as the height thereof changes.
The light beam returned by the recursive mirror 1523 is reflected again at the two etalons 100a and 100b. The light reflected again by the two etalons 100a and 100b passes through a collimator 1524 to be output from an output fiber 1525. The wavelength dispersion compensating module 1520 is configured to reflect light in two to-and-fro stages, in total.
At a position at which the light beam reflected by the two etalons 100a and 100b is emitted, a recursive mirror 1533 is provided. The recursive mirror 1533 reflects the light beam reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b as the height thereof changes. The light beam returned by the recursive mirror 1533 is reflected again at the two etalons 100a and 100b.
At a position at which the light beam reflected again by the two etalons 100a and 100b is emitted, a recursive mirror 1543 is provided. The recursive mirror 1543 reflects the light beam reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b as the height thereof further changes. The light beam returned by the recursive mirror 1534 is reflected again at the two etalons 100a and 100b.
At a position at which the light beam reflected again by the two etalons 100a and 100b is emitted, a returning planar mirror 1535 is provided. The returning planar mirror 1535 reflects the light beam reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b. The wavelength dispersion compensating module 1530 shown in
As described, with the wavelength dispersion compensation device according to the third embodiment, the effects of the wavelength dispersion compensation device according to the first embodiment and the second embodiment can be achieved, and occurrence of the interference between the edge of an etalon and light can be prevented while increasing the dispersion compensation amount by increasing the number of stages at which light is reflected by etalons.
The light incident to the birefringent crystal 1713 is divided, in polarization directions, into two light beams to be emitted. At a position from which one of the two light beams is emitted, a ½-wavelength plate 1714 is provided in the birefringent crystal 1713. The two light beams emitted from the birefringent crystal 1713 are reflected at the etalons 100a and 100b.
At a position at which the light beam reflected by the two etalons 100a and 100b is emitted, a birefringent crystal 1715 is provided. The light beams incident to the birefringent crystal 1715 are combined into a single light beam to be emitted from the birefringent crystal 1715. At a position at which the one of the two light beams that has not passed through the ½-wavelength plate 1714 is input to the birefringent crystal 1715, a ½-wavelength plate 1716 is provided. The light beam emitted from the birefringent crystal 1715 passes through a collimator 1717, and is output from an output fiber 1718.
The light incident to the birefringent crystal 1723 is divided into two light beams according to a polarization state to be emitted from the birefringent crystal 1723. At a position from which one of the two light beams is emitted in the birefringent crystal 1723, a ½-wavelength plate 1724 is provided.
The two light beams emitted from the birefringent crystal 1723 are reflected at the etalons 100a and 100b. At a position at which the light beams reflected by the two etalons 100a and 100b are emitted, a recursive mirror 1725 is provided. The recursive mirror 1725 reflects the light beams reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b while switching optical paths thereof.
The light beams returned by the recursive mirror 1725 are reflected again at the two etalons 100a and 100b. The light beams reflected again by the etalons 100a and 100b enter the birefringent crystal 1723 again. The light beams that have entered the birefringent crystal 1723 are combined into a single light beam to be emitted from the birefringent crystal 1723. The light emitted from the birefringent crystal 1723 passes through the collimator 1722 and is output from the input/output fiber 1721.
The light incident to the birefringent crystal 1733 is divided into two light beams according to a polarization state to be emitted from the birefringent crystal 1733. At a position from which one of the two light beams is emitted in the birefringent crystal 1733, a ½-wavelength plate 1734 is provided.
The two light beams emitted from the birefringent crystal 1733 are reflected at the etalons 100a and 100b. At a position at which the light beams reflected by the two etalons 100a and 100b are emitted, a recursive mirror 1735 is provided. The recursive mirror 1735 reflects the light beams reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b as the height thereof changes.
The light beams returned by the recursive mirror 1735 are reflected again at the two etalons 100a and 100b. At a position at which the light beams reflected again by the two etalons 100a and 100b are emitted, a recursive mirror 1736 is provided. The recursive mirror 1736 reflects the light beams reflected from the two etalons 100a and 100b back toward the two etalons 100a and 100b while switching optical paths thereof.
As described, with the wavelength dispersion compensating module according to the fourth embodiment, the effects of the wavelength dispersion compensation device according to the first to the third embodiments can be achieved, and by making a polarization state of light either one of a P-polarization and an S-polarization, a stable dispersion compensation amount can be set independent of a polarization state of input light. Moreover, by using a recursive mirror as a reflecting member to return light by reflection, variation of optical path length dependent on a polarization state is not caused.
According to each of the embodiments described above, a reflective film whose reflectance varies corresponding to an incident angle of light can be easily formed. Therefore, productivity of an etalon can be improved, and a wavelength dispersion compensating module can be manufactured at a low cost. Furthermore, since the reflectance can be made dependent on wavelength, a wavelength dispersion compensating module that corresponds to a required dispersion compensation characteristic can be manufactured.
The etalon substrate of the etalon 100 can be formed with a high refractive index material such as silicon and zinc selenide. By using a high refractive index material, variation of a wavelength interval caused by a change of the incident angle of light can be suppressed, and a variable range (wavelength) can be expanded.
Moreover, by connecting a plurality of etalons that differ from each other in a reflection characteristic optically in series, a dispersion compensation amount can also be set to 0. Furthermore, the occurrence of interference between an edge of an etalon and light can be prevented while increasing a dispersion compensation amount by increasing the number of stages in which light is reflected by the etalons. Moreover, a stable dispersion compensation amount can be set independent of a polarization state of input light.
According to the embodiments described above, it is possible to obtain required dispersion compensation amount with ease. Moreover, it is possible to manufacture a wavelength dispersion compensation device easily at low cost.
Although the invention has been described with respect to a specific embodiment for a complete and clear disclosure, the appended claims are not to be thus limited but are to be construed as embodying all modifications and alternative constructions that may occur to one skilled in the art which fairly fall within the basic teaching herein set forth.
Number | Date | Country | Kind |
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2006-106497 | Apr 2006 | JP | national |
2007-092631 | Mar 2007 | JP | national |
This application is a continuation-in-part application of application Ser. No. 11/506,941 filed Aug. 21, 2006, and is based upon the prior Japanese Patent Application No. 2007-092631 filed on Mar. 30, 2007, the latter and the former being based upon the prior Japanese Patent Application No. 2006-106497, filed on Apr. 7, 2006.
Number | Date | Country | |
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Parent | 11506941 | Aug 2006 | US |
Child | 11976076 | US |