Relative intensity noise (RIN) is one of the major contributors to interferometric fiber optic gyro (IFOG) angle random walk (ARW). Electric intensity-noise-subtraction has been used to reduce the RIN in order to improve the gyro performance. However, for depolarized single mode (SM) IFOGs, the RIN subtraction has not been as effective as that for polarization maintaining (PM) IFOGs due to mismatch between the lightwave spectra at the RIN detector and that at the rate detector. This spectrum mismatch is originated from the gyro depolarizer and the birefringence of the single mode coil fiber.
In this prior art, the light source intensity noise is typically measured at a port 124 of the 2×2 fiber coupler 120 by a RIN detector 170 and then electronically subtracted from the gyro rate detector signals after proper delays. This RIN tapping scheme works well for a PM gyro (not shown in
The present invention provides a more effective RIN subtraction method which will significantly improve the ARW performance of the depolarized gyros. This invention uses a scheme that taps the RIN detector light in the sensing loop, after the light transits through the depolarizer and the coil but before it combines with the counter propagating lightwave. The tapped RIN lightwaves are polarized by a following polarizer with pass axis orientated in the same direction as that of the IOC. In this way, the RIN detector receives lightwaves with spectrum substantially identical to that of the rate detector, leading to more effective RIN subtraction. Since the rotation and modulation induced lightwave phase variations are not converted to intensity variations at the RIN detector (interference with the counter propagating light does not happen), only the unwanted intensity noise is subtracted out from the rate signal. This scheme has an additional advantage of easy satisfaction of the delay requirement of the RIN signal relative to the rate signal without using a long delay fiber or additional electronics. Furthermore, since the RIN signals are tapped after the light transit through the coil fiber (up to a few kilometers), the intensity fluctuations originated from changes of coil loss are identical to both rate and RIN detector, leading to more efficient noise subtraction.
In the present invention, there are two preferred embodiments of the invention. One is to insert a PM-coupler at one of the IOC output fibers connected to the depolarizer. This coupler couples a small amount of light that transits through the coil and directs it to the RIN detector. Properly polarizing the RIN light and isolating it from returning to the sensing loop are necessary. Another embodiment requires a new design of the integrated optical circuit (IOC) which incorporates the RIN tap coupler and the polarizer inside the IOC. This scheme increases the level of component integration and helps to realize a more compact gyro design.
Preferred and alternative embodiments of the present invention are described in detail below with reference to the following drawings:
Relative intensity noise (RIN) of a broadband light source originates from beating of the different optical frequency components contained in the light source. For an interferometric fiber optic gyroscope (IFOG), the RIN at the rate detector is determined by the light source spectrum reached the detector. In order to effectively subtract the intensity noise from the rate detector, another detector (RIN detector) dedicated to record the RIN of the light source at a different place of the optical circuit is desirable to receive light with substantially the same spectrum as that of the rate detector. The present invention describes systems and methods for effective RIN subtraction in depolarized gyros using matched light spectra at RIN and rate detectors.
Referring to
Before being coupled into the fiber coil 250, the CW (CCW) light in a waveguide 234 (235) first propagates to an upper (lower) of a depolarizer 240 section that includes a PM fiber 241 (284, 285) and 243 (246). The polarization pass-axis of the IOC 230 is aligned with that of the PM fiber 241 (284, 285), and the polarization axes of 241 (284) and 243 (246) are orientated 45° with respect to each other at the fiber splice 242 (245). In such a configuration, each wavelength component of the broadband light source launched into the coil will have a different polarization state ranging from linear to elliptical to circular shapes that in total form a nearly depolarized light. CW (CCW) lightwaves exiting end 252 (251) of the fiber coil is coupled into the lower (upper) depolarizer section that comprises PM fiber 246 (243), 284 (241) and the 45° splice 245 (242) connecting them.
The CW light recombines with the CCW light at splitter/combiner 232. Only wavelength components with non-zero intensity along the pass-axis of the IOC 230 reach the rate detector 260 after being directed by the coupler 220. A typical light spectrum at the rate detector is shown by the light spectrum 180 in
Different from the prior art shown in
It can be theoretically proved that the lightwave spectrum at the RIN detector 270 is identical to that at the rate detector 260. The lightwaves from the broadband light source 210 are unpolarized. The lightwaves are polarized by the waveguides of the IOC 230. The CW lightwave at the combiner 232 after transmitting through the whole fiber loop 250 can be expressed by the Jones matrix method.
In the above expression, E0x and E0y are the electric field of the input light polarized along pass- and block-axis of the IOC 230. Without lost of generality, it is assumed here that the x-polarized light E0x is orientated along the IOC pass-axis, and the y-polarized light E0y is orientated along the IOC block axis. t1, t2, t3, and t4 are the phase delays incurred by the birefringent slow axis of (234+241), 243, 246 and (235+285+284) relative to their corresponding fast axis. φB is the bias modulation phase applied at a modulator 233, and φR is the rotation induced Sagnac phase. A, B, C, and D are the wavelength dependent Jones matrix elements of the SM coil in the fiber loop 250 which can be measured or simulated. ε is the polarization amplitude extinction ratio of the IOC 230. When the IOC 230 has high polarization extinction ratio, the y-component of the electric field is negligibly small. Only the x-polarized light will reach the detector.
The CCW lightwave at the combiner 232 after it is transmitted through the fiber loop 250 can be similarly expressed as
The total field that reaches the rate detector 260 is
Where β is a coefficient that takes into account the amplitude loss of light propagating from the combiner 232 to the rate detector 260. U is a simplifying symbol that stands for the expression in the first parentheses of the above equation. The intensity at the rate detector 260 is
Since the A, B, C, and D matrix elements of the SM fiber coil 250 depend on wavelength, |U|2 is a function of wavelength and describes the light power spectral distribution at the rate detector 260. The rate signal at the rate detector 260 contains the Sagnac phase that can be demodulated for rotation rate sensing.
The light that reaches the RIN detector 270 does not combine with its counter-propagating part and is not bias modulated. The intensity of the light that reaches the RIN detector 270 is
E
RIN
=αE
0x
e
iφ
(A−Be−it
I
RIN=α2|E0x|2|U|2 (6)
where α is the amplitude loss incurred by the RIN coupler and path to the RIN detector 270. When comparing Equation 4 with Equation 6, the lightwave spectrum reaching the RIN detector 270 is the same as that at the rate detector 260, both described by |U|2. However, the signal produced by the RIN detector 270 does not contain any intensity variation from Sagnac phase and bias modulation. This is ideal for RIN subtraction because the Sagnac phase induced intensity variation shall not be removed during RIN subtraction and are useful in the demodulation process for rate sensing.
The coupler 281 can also be placed between the IOC 230 waveguide 234 and the 45° splice 242 in the upper section of the depolarizer 240. The above theory showed that the spectrum of CW and CCW light tapped between the splitter/combiner 232 and the 45° splices 245 and 242 after transiting through the sensing loop is identical. The two configurations are equivalent and are considered covered by the same embodiment shown in
To reduce the polarization induced bias errors that the PM coupler in the sensing loop might introduce, PM couplers with as small as possible polarization cross-couplings are used, e.g. smaller than −25 dB. The coupler shall be located as close as possible to the 45° splice so that even in cases where polarization cross-couplings cannot be avoided in the coupler, their location can be substantially close to that of the 45° splice and introduce negligible bias errors. This provides easier design for the depolarizer.
Essentially in both embodiments, the RIN light is tapped inside the sensing loop before the light recombines with the counter-propagating lightwave but after the light transits through the coil and the depolarizers. The two embodiments shown in
While the preferred embodiment of the invention has been illustrated and described, as noted above, many changes can be made without departing from the spirit and scope of the invention. Accordingly, the scope of the invention is not limited by the disclosure of the preferred embodiment. Instead, the invention should be determined entirely by reference to the claims that follow.