The field of the invention is optical filtering. More specifically, it is directed to tunable optical filters using cascaded etalons.
Tunable optical filters are devices for optical frequency selection. They are used in a wide range of applications, such as selecting laser cavity modes in tunable lasers, creating narrow-band tunable light sources, adding or dropping optical signals of different frequencies from a spectrally multiplexed beam, or making sweeping spectrometers. A common architecture of a tunable optical filter, attractive because of its low cost, is a tunable Fabry-Perot (FP) etalon. In the tunable FP etalon architecture, the resonance frequency of the device is tuned by changing the cavity optical path length, either by changing the refractive index of the medium in the etalon cavity, or by changing the length of the etalon cavity. Common low-cost implementations of an optical-fiber-based tunable Fabry-Perot etalon are i) a free-space dielectric slab in which the resonance of the dielectric slab is tuned by temperature, ii) a gap between two cleaved fiber ends, with the gap distance tunable by the piezo-electric effect, and iii) a liquid-crystal slab in which the index of the liquid crystal is changed by an applied variable electric voltage.
For many widely used applications a large free-spectral-range (FSR) is required. An important application, a C-band scanning spectrometer, requires an FSR which is greater than the C-band (>5 THz), so that at all tuning points it only passes one segment of the C-band spectrum. For applications requiring low-cost and high reliability, tunable filter implementations identified as category ii) above have the disadvantage that the piezoelectric effect suffers from hysteresis, sticking, and unrepeatability over life. Implementation identified as iii) above presents difficult challenges in manufacture, involving for example engineering the parallelism and reflectivity of the reflective surfaces in the presence of coated dielectric electrodes. Another category of tunable filters found in industry are tunable planar-lightwave-circuit (PLC) ring resonator filters. In the ring-resonator architecture the resonance can be tuned by temperature, or by changing the material above the ring that is seen by the evanescent optical field. However, this architecture suffers from the primary disadvantage that PLC devices are costly to fabricate. Finally, recent industry mass-deployment of tunable dispersion compensators based on precisely-temperature-tuned dielectric slab etalons, has lowered the cost of fiber lens collimators, and the cost of packaging of fiber/dielectric-slab etalon devices. The temperature-tuned dielectric slab implementation is thus the focus of this invention, due to simplicity and reliability combined with good performance.
For applications of main interest, a challenge that remains with temperature-tuned dielectric slab devices is the large temperature range required to sweep the filter over the entire frequency band of interest, for example, 5 THz to sweep the C-band as mentioned above. For temperature tuned dielectric slab devices, silicon is the industry-standard substrate material. Typically, temperature ranges of >300° C. are required to tune a silicon slab filter over 5 THz. The structure also requires a stack of 10 to 20 thin layers of materials with differing refractive indicies. To avoid structural degradation these layers require thermal expansion coefficients that precisely match that of the silicon substrate. For applications such as optical channel monitoring (OCM) in multiplexed optical communications networks, one sweep every few seconds over a device lifetime of 15-20 years may be used. Complex and expensive fabrication processes are required to construct and package such a structure so that it does not exhibit performance degradation or failure with such stressful temperature cycling. Additionally, fabrication is complicated by the requirement that the thickness of the slab must be large (e.g., ˜10 mm) for an FSR of 5 THz.
A temperature-tuned dielectric-slab-etalon scanning spectrometer that is low cost and simple to fabricate uses cascaded etalon modules, each module comprising a Fabry-Perot (FP) etalon having a relatively small Free Spectral Range (FSR), with at least two modules provided with a temperature control. According to the invention, the multiple FP modules produce Vernier tuning control. Devices with this characteristic are referred to below as Vernier Tuning Fabry-Perot Filters (VTFPFs). In these devices, the tuning temperature range may be less than 10° C., and the required slab thickness may be less than 1 mm. This drastically reduces the fabrication and material requirements, and results in lower device cost and improved reliability.
The invention may be more easily understood when considered in conjunction with the drawing in which:
The etalons in the VTFPF devices of the invention are shown as Fabry-Pérot etalons operating according to known principles of optics. A Fabry-Pérot etalon is typically made of a transparent plate with two reflecting surfaces. An alternate design is composed of a pair of transparent plates with a gap in between, with any pair of the plate surfaces forming two reflecting surfaces. From the standpoint of cost and manufacturability the preferred plate material is silicon. The transmission spectrum of a Fabry-Pérot etalon as a function of wavelength exhibits peaks of large transmission corresponding to resonances of the etalon.
Referring to
Maximum transmission (Te=1) occurs when the difference in optical path length between each transmitted beam (2nl cos θ) is an integer multiple of the wavelength. In the absence of absorption, the reflectivity of the etalon Re is the complement of the transmission, such that Te+Re=1, and this occurs when the path-length difference is equal to half an odd multiple of the wavelength.
The finesse of the device can be tuned by varying the reflectivity of the surface(s) of the etalon. The finesse of the etalon is related to the etalon reflectivities by:
where F is the finesse, R1, R2 are the reflectivity of facet 1 and facet 2 of etalon.
The wavelength separation between adjacent transmission peaks is the free spectral range (FSR) of the etalon, Δλ, and is given by:
Δλ=λ02/(2nl cos θ)
where λ0 is the central vacuum wavelength of the nearest transmission peak. The FSR is related to the full-width half-maximum by the finesse of the etalon. Etalons with high finesse show sharper transmission peaks with lower minimum transmission coefficients.
The FSR of an etalon is temperature sensitive because the optical length of the etalon or the refractive index within the etalon is typically temperature sensitive. This temperature sensitivity, frequently unwanted, can be used to advantage, if controlled, to tune a device that incorporates an etalon.
The VTFPF of this invention comprises a cascade of N>1 single Fabry-Perot etalon filter modules. An embodiment of a VTFPF is shown in
N=2 etalons
The reflectance of the facets of the etalons in this example is 0.95. The VTFPF of this example creates a filter having a scan FSR of 8 THz, and 7 dB adjacent channel rejection (ACR) for neighboring 100 GHz WDM channels.
N=3 etalons
The reflectance of the facets of the etalons in this example is 0.95. The VTFPF of this example has an overall FSR of 8 THz, and provides 16 dB ACR.
Simulated filter transmittances for the VTFPFs described above are shown in
The finesse of the device may be increased by changing the reflectance of the facets from 0.95, as in Example 1, to 0.99. The result of this, for a N=2 device is shown in
As described earlier, the main resonance frequency of the VTFPF is temperature sensitive and the VTFPF is tuned by changing the temperature of the N modules of the VTFPF. A feature of the VTFPF of the invention is that the temperatures of the N modules are independently controlled and independently changed. The underlying mechanism is illustrated in
Multiple temperature states are used to scan the VTFPF over the frequency band of interest. In the embodiments shown here that band is approximately 191.5 THz to 196.5 THz (see
The temperatures are shown as deltas from a base temperature. This is intended to indicate that the base temperature may vary over a wide range, e.g., 0-400 degrees C. The base temperature may also be below room temperature. For clarity, the temperature cycles of the two etalons are shown on separate temperature scales, with the temperature cycle of etalon 1 referenced to the scale to the left of the figures and the temperature of etalon 2 is referenced to the scale on the right.
The cycles shown in
The absolute temperature range of the temperature cycles in
A temperature cycle is defined as a change in temperature from T1 to T2. At any given time during a scan the temperature of etalon N1 is defined as TN1 and the temperature of etalon N2 is TN2. Etalon N1 is cycled between T1N1 and T2N1. The range for that cycle is ΔTN1. Etalon N2 is cycled between T1N2 and T2N2. The range for that cycle is ΔTN2.
Close inspection of the cycles in
The temperature difference increment between cycles may vary substantially depending on the number of cycles used, which in turn depends on the application and the precision of the scan. Typically the temperature difference increment from cycle to cycle in a stepped or other cycle pattern in likely commercial applications will be less than 1.0 degree C.
Two modules (N=2) in the device is the minimum for the devices described here. It is anticipated that more demanding applications may require at least three modules.
The temperature of each module should be aligned to match the FSR peak of the associated etalon at the desired tuning frequency. To maintain the filter shapes and the FSR alignment such that the ACR degrades by, for example, less than 1 dB, the tuning temperatures is preferably accurate to ±0.01° C. The accuracy may vary significantly depending on the application. In general, devices constructed according to the invention will have VTFPF modules with a temperature variation tolerance of less than ±0.1° C. It should be understood that when temperatures are referred to as “equal” or “the same” these tolerances are to be inferred.
It will be understood that since the temperature of each module is independently controlled, each module should be physically separate from other modules, and sufficiently removed to allow the temperature of the etalon(s) in each stage to be independently controlled.
The VTFPFs of primary interest here are for optical transmission systems that typically operate with a wavelength band centered at or near 1.55 microns. The wavelength range desired for many system applications is 1.525 to 1.610 microns. This means that the materials used for the etalons should have a wide transparent window around 1.55 microns. However, VTFPF devices are useful for other wavelength regimes as well, such as 1.310 microns.
The structure of the Fabry-Perot etalons is essentially conventional, each comprising a transparent plate with parallel boundaries. A variety of materials may be used, with the choice dependent in part on the signal wavelength, as just indicated, and the required temperature tuning range. The optical characteristics of etalons vary with temperature due to at least two parameters: the variation of refractive index with temperature, commonly referred to as the thermo-optic effect, and written as dn/dt, which changes the optical path length between the optical interfaces, and the coefficient of thermal expansion (CTE) which changes the physical spacing between the optical interfaces. In standard etalon device design, the optical sensitivity of the device to temperature changes is minimized. Materials may be chosen that have low dn/dt, and/or low CTE. Materials may also be chosen in which the dn/dt and the CTE are opposite in sign and compensate. Common materials for etalons are fused quartz, tantalum pentoxide or niobium pentoxide. Semiconductor materials or glasses may also be used.
It is preferred that the VTFPFs of this invention be based on silicon as the bulk etalon substrate material. Silicon has a large thermo-optic coefficient and therefore is contra indicated for most optical devices. However, amorphous silicon, polysilicon, and preferably single crystal silicon, are recommended for the methods described here because a large thermo-optic coefficient is desirable. The thermo-optic coefficient of single crystal silicon is approximately 1.9 to 2.4×10−4 per degree K. over the temperature ranges used for tuning the etalons.
Typical cross section dimensions for the etalons are 1.8 mm square, with the optical active area approximately 1.5 mm square. As indicated above the thickness of the VTFPF etalons may be less than 1 mm, typically 0.05 to 1 mm. The dimensions of the etalons will affect how rapidly the temperature may change and thus the cycle time. The cycle time may vary widely depending on this and other variables. For most applications where the band pass of the filter is scanned the objective will be a rapid scan time. In these applications a scan time of less than 10 seconds may be used and is easily realized with state of the art etalon temperature controls.
The embodiments shown in
Another option for more rapid tuning is to divide the scan into fewer cycles and use etalons with larger FSRs. This option is illustrated in
As should be evident, the number of temperature cycles S used to scan a given frequency band may vary widely. The presence of any given number of cycles can be a useful indication of operation of the VTFPF according to the invention. Since the principle of the invention is, for a given frequency scan band, to divide the band into S sub-bands and cycle the temperature of the N etalons for each sub-band, the advantages of the invention may be considered realized if the scan is divided into at least three sub-bands and the temperature of the etalons is cycled at least three times (S=3) during the scan. However, more optimum vernier operation will be realized if the overall scan is divided into a larger number of sub bands. Typically this will be more than 7 and the N etalons will be cycled more than 7 times for each scan.
Other alternative embodiments include the use of multiple cavity etalons. For example, for a VTFPF device having N=2, a twin cavity etalon may be used. However the presence of a third inter mirror cavity creates a higher-order modulation on the filter transmittance, and unwanted coupling between the individual FP cavities becomes more severe as the spacing between etalons is reduced. Moreover, spacing the etalons closely interferes with the independent temperature control mentioned earlier. Accordingly it is preferred that the etalons be spaced apart by at least 1 mm. Also, with the etalon cavities separated one or more fiber-optic isolators may be used to control inter cavity coupling.
Other alternative embodiments may be designed with reflecting surfaces to fold the optical path. Supplemental lens arrangements may be used for steering or focusing the beam as desired. These kinds of device modifications are within the contemplation and scope of the invention.
Various additional modifications of this invention will occur to those skilled in the art. All deviations from the teachings of this specification that basically rely on the principles and their equivalents through which the art has been advanced are properly considered within the scope of the invention as described and claimed.