Scanning spectrometer with multiple photodetectors
View Patent ↗A scanning optical spectrometer with a detector array is disclosed, in which position of focused spot of light at the input of a dispersive element such as arrayed waveguide grating (AWG) with a slab input, is scanned using a micro-electro-mechanical (MEMS) tiltable micromirror so as to make the dispersed spectrum of light scan over the detector array coupled to the AWG. Sub-spectra recorded using individual detectors are concatenated by a processor unit to obtain the spectrum of input light.
1. A spectrometer for measuring a spectrum of light having a frequency range Δf, the spectrometer comprising:
M input ports P m for receiving the light and relaying it to M source points S m , wherein M≧1; and m is an integer number satisfying the following condition: 1≦m≦M;
an input scanning means coupled to the M input ports P m , for relaying the light from any of the M source points S m to an intermediate point, wherein in operation, a location x of the intermediate point is scanned by the scanning means from a value x 1 continuously to a value x 2 within a scanning range δx=|x 2 −x 1 |;
a dispersing means coupled to the input scanning means, for spatially separating frequency components of the light in dependence upon the location x of the intermediate point of the light;
N detectors D n coupled to the dispersing means, for detecting the light in dependence upon the optical frequency thereof, wherein N≧2; n is an integer number satisfying the following condition: 2≦n≦N; and each detector D n is disposed to receive the optical frequency component at a central frequency f n (x), so that, when x is scanned between values x 2 and x 1 , the central frequency f n (x) is scanned within a range δf=|f n (x 2 )−f n (x 1 )|;
wherein, for any central frequency f 0 within the range Δf of optical frequencies, there is at least one such n=n 0 and at least one such x=x 0 that f n0 (x 0 )=f 0 .
2. A spectrometer of claim 1 wherein δf is substantially equal to Δf/N.
3. A spectrometer of claim 1 wherein δf>Δf/N and wherein for each detector D n there is an associated spectral band B n limited by the respective central frequencies f n (x 2 ) and f n (x 1 ), and each said spectral band B n overlaps with another said spectral band B i , wherein |i−n|=1.
4. A spectrometer of claim 1 , further comprising a controller, for controlling the scanning means and for collecting signals from the N detectors D n during the scanning of the scanning means within the scanning range δx=|x 2 −x 1 |, and for combining said signals within respective frequency ranges δf=|f n (x 2 )−f n (x 1 )|, so as to obtain the spectrum of the light within the frequency range Δf.
5. A spectrometer of claim 1 , wherein the input scanning means includes a micro-electro-mechanical (MEMS) tiltable mirror.
6. A spectrometer of claim 5 , wherein, for every m corresponding to a source point S m , said scanning of the location x of the intermediate point from a value x 1 to a value x 2 is performed by tilting the MEMS mirror from an angle α m1 to an angle α m2 .
7. A spectrometer of claim 6 , wherein:
M≧2; and
for an integer number k corresponding to a source point S k , wherein 1≦k≦M, and wherein k≠m, said scanning of the location x of the intermediate point from a value x 1 to a value x 2 is performed by tilting the MEMS mirror from an angle α k1 to an angle α k2 , wherein the following conditions are fulfilled: |α m1 −α m2 |<|α m1 −α k1 |; |α k1 −α k2 |<|α m1 −α k1 |; |α m1 −α m2 |<|α m2 −α k2 |; and |α k1 −α k2 |<|α m2 −α k2 |.
8. A spectrometer of claim 1 , wherein the dispersing means includes a diffraction grating.
9. A spectrometer of claim 8 , wherein the diffraction grating is a concave diffraction grating.
10. A spectrometer of claim 8 , wherein the diffraction grating is flat, and the dispersing means further includes at least one element having optical power, for coupling the light from the input scanning means to the flat diffraction grating, and from the flat diffraction grating to each of the N detectors.
11. A spectrometer of claim 1 , wherein the dispersing means includes an arrayed waveguide grating (AWG) comprising:
an input slab coupled to the input scanning means, wherein said coupling is realized through free space propagation of the light;
an array of grating waveguides coupled to the input slab;
an output slab coupled to the array of the grating waveguides; and
a star coupler coupled to the output slab, wherein the star coupler has N output waveguides, wherein each of said output waveguides is coupled to one of the N detectors.
12. A spectrometer of claim 11 , wherein the AWG is a part of a planar lightwave circuit (PLC) and the M input ports P m are input waveguides of said PLC.
13. A spectrometer of claim 12 , wherein the PLC has an input facet, and the input waveguides are fanned in at the input facet to a distance of between 20 and 40 microns, and the M source points S m are ends of the fanned-in input waveguides, wherein said ends are located at the input facet, and wherein the input facet runs through the input slab from x 1 to x 2 .
14. A spectrometer of claim 13 , further comprising a mask abutting the input slab, wherein the mask is opaque to the light having the frequency range Δf, and wherein the mask has an opening extending from x 1 to x 2 .
15. A spectrometer of claim 11 , further comprising a temperature sensor, for compensating a temperature drift of the AWG.
16. An optical performance monitor comprising a spectrometer of claim 1 , for measuring optical power, or central wavelength, or optical signal-to-noise ratio of optical signals in a fiberoptic network, wherein the value of δf is selected from a group of values consisting of 200 GHz; 100 GHz; 50 GHz; and 25 GHz.
17. A method of measuring a spectrum of light having a frequency range Δf, the method comprising:
receiving the light at any of M source points S m , wherein M≧1; and m is an integer number satisfying the following condition: 1≦m≦M;
relaying the light from any of the M source points S m to an intermediate point at a location x;
scanning the location x of the intermediate point from a location x 1 continuously to a location x 2 within a scanning range δx=|x 2 −x 1 |;
spatially separating frequency components of the light in dependence upon the location x of the intermediate point of the light;
detecting the frequency components of the light using N detectors D n , wherein N≧2; n is an integer number satisfying the following condition: 2≦n≦N; wherein each detector D n is disposed to receive the optical frequency component at a central frequency f n (x), so that, when x is scanned between values x 2 and x 1 , the central frequency f n (x) is scanned within a range δf=|f n (x 2 )−f n (x 1 )|;
wherein, for any central frequency f 0 within the range Δf of frequencies of the light, there is at least one such n=n 0 and at least one such x=x 0 that f n0 (x 0 )=f 0 ; and
collecting signals from the N detectors D n during the scanning of the scanning means within the scanning range δx=|x 2 −x 1 |, and combining said signals within respective frequency ranges δ=|f n (x 2 )−f n (x 1 )|, so as to obtain the spectrum of the light within the frequency range Δf.
18. A method of claim 17 wherein δf is substantially equal to Δf/N.
19. A method of claim 17 wherein δf≧Δf/N and wherein for each detector D n there is an associated spectral band B n limited by the respective central frequencies f n (x 2 ) and f n (x 1 ), and each said spectral band B n overlaps with another said spectral band B i , wherein |i−n|=1.
20. A method of claim 17 , wherein the scanning is performed using a micro-electro-mechanical (MEMS) tiltable mirror.
21. A method of claim 17 , wherein the separating of the frequency components is performed using a diffraction grating.
22. A method of claim 17 , wherein separating the frequency components is performed using a planar arrayed waveguide grating (AWG) comprising an input slab having a continuous light entrance region, and wherein the MEMS tiltable mirror is used to scan the intermediate point along the light entrance region.
23. A method of claim 17 , wherein the spectrum of the light is a spectrum of optical signals in a fiberoptic network.
24. A method of claim 23 , further comprising a step of analyzing the measured spectrum of the light to obtain optical power, or central wavelength, or optical signal-to-noise ratio of optical signals in the fiberoptic network.