This disclosure relates to vibration compensation of loop oscillators and more particular to vibration compensation of interferometric noise suppressed oscillators (INSOs).
Phase noise is an important property of oscillators in general and low phase noise oscillators find application in precision timing and radar systems, for example. In mobile applications, such as mobile radars, oscillators are often subjected to mechanical vibrations. Accelerations associated with these vibrations cause stresses and mechanical distortions in the oscillator, particular in the resonator components which determine the oscillator frequency. These distortions result in small variations in the oscillator frequency. The so-called vibration sensitivity of an oscillator is generally assigned the symbol F with the relationship Δf=Γ·f0·a where f0 is the normal oscillator frequency, a is the acceleration and Δf is the resulting change in frequency. As an example, a high quality, low vibration sensitivity oscillator, with f0=10 GHz, may have Γ=1×10−10 g−1 so that its frequency changes by 1 Hz for every 1 ‘g’ of acceleration, ‘g’ being the normal acceleration due to the earth's gravity. More commonly, the vibration sensitivity is used to predict phase noise under vibration using the relationship L(fm)=20·log10(Γ·|A|/2fm), where fm is the vibration frequency and A=(2·PSD)1/2 and PSD is the power spectral density of acceleration in g2/Hz (See for example A. Hati et al., “Vibration Sensitivity of Microwave Components,” 2007 IEEE International Frequency Control Symposium Joint with the 21st European Frequency and Time Forum, Geneva, Switzerland, 2007, pp. 541-546). The effect of vibration is illustrated in general terms by
Vibration sensitivity of oscillators is well known in the art and efforts have long been made to reduce F, frequently by means of mechanical design and selection of rigid components. When vibration degradation of phase noise remains an issue despite design efforts, steps are usually taken to isolate the oscillator from the vibration using a mechanical isolation system comprising interconnected springs and dampers. However, the design of vibration isolation systems can be challenging for low vibration frequencies, for example between 10 Hz<=fm<=100 Hz. Hence schemes have been proposed to further reduce the vibration sensitivity of oscillators by electronic compensation means to reduce the reliance on and design effort required for isolation systems.
U.S. Pat. No. 4,891,611, for example, describes such a system which is illustrated in simplified form in
Most oscillators exhibit behavior in which F can be assumed to remain constant over a very wide range of accelerations, (See for example John Vig “Quartz Crystal Resonators and Oscillators for Frequency Control and Timing Applications—A Tutorial” US Army Communications-Electronics Research, Development & Engineering Center Fort Monmouth, NJ, USA, 2004). In some cases, Γ may vary with vibration frequency fm so that f will be written as Γ(fm) and it will be understood that filtering would need to be incorporated into the gain G so that variations in G=G(fm) match variations in Γ=Γ(fm) as discussed in U.S. Pat. No. 4,891,611. It is important to understand that this is an “open-loop” compensation system; the gain G(fm) must be determined experimentally and set during manufacture or tuning, the degree of reduction in apparent vibration sensitivity at the oscillator output depending on how well this is done.
Persons skilled in the art will understand that the discussion so far can be applied to any of the three orthogonal axes: X, Y & Z and that the outputs of three orthogonally-mounted accelerometers may be used and summed with independent gains GX, GY and GZ to reduce the apparent vibration sensitivity simultaneously in all three directions.
In many systems it is a requirement that the oscillator be phase locked to an external reference signal using a phase locked loop (PLL). As shown in
In an arrangement such as
Consider for example a simple loop oscillator 400 as shown in
In such a loop oscillator the frequency variation as a function of VCP phase shift depends on the insertion phase of the resonator 406 which is quite linear over the bandwidth of the resonator. However, the VCP 404 in such an arrangement designed for low phase noise applications will typically utilize reverse biased varactor diodes within the phase shift circuitry, usually resulting in a non-linear variation of phase shift, and hence oscillator frequency, with tuning voltage as shown by the representative tuning sensitivity curve 500 in
If the vibration compensation circuitry is adjusted at the nominal tuning voltage input VNom as shown in
A particular class of oscillator, often selected for use in high fidelity systems may be referred to as an Interferometric Noise Suppressed Oscillator (INSO). An INSO may utilize a sapphire-loaded cavity as the resonator and incorporate a noise degeneration circuit to suppress phase noise. An example of an INSO is described in U.S. Pat. No. 5,841,322 entitled “Phase Detector Using Carrier Suppression and Oscillator Using the Phase Detector” issued Nov. 24, 1998. As shown in FIG. 1 of U.S. Pat. No. 5,841,322, a microwave loop oscillator 10 includes a microwave amplifier 12, a high-Q resonator 14 and a phase shifter 18 among other components. A phase detector 28, which may also be referred to as an “interferometric bridge” is used to detect phase fluctuations in the oscillator loop and generate an error signal at the output of mixer 32. The error signal being a measure of frequency fluctuations from the nominal oscillation frequency. This error signal is amplified (and possibly filtered) by the control signal generator 62, which includes a low noise amplifier 13, before being fed back as a control signal into the loop phase shifter 18 to cancel the phase noise in the loop. The phase shifter 18 induces a phase shift in the loop in response to the control signal such that the noise close to the carrier frequency in the loop is suppressed. Flicker noise associated with microwave amplifier 48 would be detrimental to the operation of the oscillator. Carrier suppression ensures small signal operation of microwave amplifier 48, which reduces the amplifier's flicker noise in proportion to the signal power at the amplifier 48 input.
A phase-locked INSO locks the oscillator 10 to an external reference signal using a PLL. In a phase-locked INSO, the loop phase shifter 18 is not used to provide the VCO tuning port as in
The following is a summary that provides a basic understanding of some aspects of the disclosure. This summary is not intended to identify key or critical elements of the disclosure or to delineate the scope of the disclosure. Its sole purpose is to present some concepts of the disclosure in a simplified form as a prelude to the more detailed description and the defining claims that are presented later.
The present disclosure provides for active vibration compensation of Interferometric Noise Suppressed Oscillators (INSOs). In an INSO the error signal at the mixer output responds linearly to changes in carrier frequency. A vibration compensation signal is summed with the error signal at the input to the feedback amplifier to provide the control signal to the loop phase shifter to suppress close-in phase noise near the carrier frequency and to reduce the effects of mechanical vibrations on oscillator phase noise. The addition of the vibration compensation signal does however degrade carrier suppression, hence increases the flicker noise contributed by the INSO's LNA but does so without degrading overall oscillator phase noise. In a frequency tuned configuration such as a phase-locked INSO, the vibration compensation signal reduces the effects of mechanical vibrations on oscillator phase noise independent of the tuning voltage applied to the phase shifter.
These and other features and advantages of the disclosure will be apparent to those skilled in the art from the following detailed description of preferred embodiments, taken together with the accompanying drawings, in which:
Although an INSO provides much higher fidelity (i.e., much lower phase noise) than a standard loop oscillator and exhibits very low vibration sensitivity because of the combination of noise suppression and rigid, high-Q resonators (e.g., Sapphire resonators) that are typically used, certain applications may require even greater immunity to mechanical vibrations. One technique is to add active vibration compensation to reduce the effects of external vibrations on oscillator phase noise.
The vibration compensation signal cannot be input to loop phase shifter as in
The vibration compensation signal could be input to the phase shifter 42 in the carrier suppression block of phase detector 28 of the oscillator as shown in FIG. 1 of U.S. Pat. No. 5,841,322. However, phase shifter 42 has a non-linear tuning sensitivity that produces a tuning slope KVCO that varies over the tuning range of phase shifter 42. Vibration compensation is an “open-loop” compensation system. The overall gain must be determined experimentally and be stable over the tuning range to provide vibration compensation that reduces the effects of vibration on oscillator phase noise over that tuning range. The variation of KVCO over the tuning range of the vibration compensation signal will degrade the phase noise. Because the of the already low vibrations sensitivity, the vibration compensation may be understood to apply VComp of a magnitude that would make very small changes in oscillator frequency. For example, in a 10 GHz oscillator with Γ=10−10 g−1 undergoing a 1 g acceleration, VComp·kVCO would be equivalent to only 1 Hz. Addition of the vibration compensation voltage, VComp to VTune, therefore doesn't change VTune significantly in an oscillator that might typically have a full tuning range of several kHz. However, any non-linearity in the tuning curve of the oscillator will result in generation of unwanted harmonic effects.
In a frequency-tuned INSO, a tuning voltage such as VPLL is also applied to the phase shifter 42. The tuning range of the tuning voltage is much larger than that of the vibration compensation signal. For example, the tuning voltage may need to induce a 1 kHz change in the carrier frequency to compensate for thermal drifts. As such the magnitude of variations in Vtune may be 1,000× that of the variations in VComp. Hence problems associated with non-linearity are of paramount importance in applications requiring the INSO to be tuned such as when phase locked using a PLL and the open-loop vibration compensation system will fail to suppress the effects on phase noise caused by external vibrations across that tuning range as shown by curve 600 in
More specifically, for the purposes of discussion, with reference to FIG. 1 of U.S. Pat. No. 5,841,322 two arms of the interferometer are identified: the first comprising the attenuator 44 and phase shifter 42 referred to as the “reference arm”, and the second comprising the connection between the circulator 22 and combiner 46 as the reflection arm. To maintain balance in the interferometer, the signals from both reference and reflection arms must arrive at the combiner 46 with the same amplitude but out of phase so that cancellation occurs. Hence, any phase shift in the reference arm must be matched by an equal and opposite phase shift in the reflection arm signal. In response to a phase shift in the reference arm and operation of the feedback circuit, the equal and opposite phase shift in the reflection arm comes about by virtue of a change in oscillation frequency and the reflection phase characteristics of the resonator. Again, the phase shift in reflection versus frequency is quite linear over a significant fraction of the resonator bandwidth. However, just as the non-linear voltage to phase relationship of the VCP in
In accordance with present disclosure, a vibration compensation signal is summed with the error signal at the output of mixer 32 in FIG. 1 of U.S. Pat. No. 5,841,322 at the input to amplifier 64 of the control signal generator. The error signal responds linearly to changes in carrier frequency and thus the KVCO at this point in the oscillator is constant. Because vibration compensation operates “open-loop” this greatly increases the utility of the vibration compensation as it allows the oscillator to be tuned independently by the phase shifter while maintaining the desired constant value of kVCO relevant to the vibration compensation signal. However, inserting an additional signal into the oscillator loop at this point goes against long-established practice taught by U.S. Pat. No. 5,841,322 because doing so degrades carrier suppression, increasing the flicker noise contribution of amplifier 48.
A simplified schematic of a vibration-compensated phase-locked INSO 700 is shown in
Phase detector 708 includes a carrier suppression circuit 716 responsive to a first signal 718 at a carrier frequency that propagates around the loop and a second signal 720 that is a reflection of first signal 718 off of resonator 706 to produce a carrier suppressed signal 722, a mixer 724 responsive to the carrier suppressed signal 722 and the first signal 718 to produce the error signal 710 corresponding to the phase difference between the first and second signals.
Carrier suppression circuit 716 includes a “reference arm” and a “reflection arm”. The reference arm includes a reference arm coupler 728 to couple a portion of first signal 718 out of the loop, a variable attenuator 730 and a phase shifter 732. The reflection arm includes a connection between circulator 734 that couples second signal 720 out of the loop. To maintain balance in the interferometer, the signals from both reference and reflection arms must arrive at a combiner 736 with the same amplitude but out of phase so that cancellation occurs. Hence, any phase shift in the reference arm is matched by an equal and opposite phase shift in the reflection arm signal due to the action of the feedback. Combiner 736 produces carrier suppressed signal 722 that is fed to a low noise amplifier 738 that amplifies the carrier suppressed signal 722. A mixer local oscillator coupler 740 couples a portion of first signal 718 from the loop that is fed through a mixer local oscillator phase shifter 744 to mixer 724.
To phase-lock the INSO, PLL circuitry 750 is responsive to an output signal 752 extracted from the oscillator loop via coupler 754 and a reference signal 756 to produce a PLL tuning signal, VPLL that is applied to the tuning port of phase shifter 732 in the reference arm of the carrier suppression circuit. Although the tuning slope KVCO1 associated with phase shifter 732 is not constant over the tuning range, the closed-loop characteristics of the PLL are insensitive to variations in KVCO1 and the oscillator frequency will be locked to the reference signal frequency.
To provide active vibration compensation for the INSO 700, a vibration sense circuit 760 including one or more accelerometers 762 (e.g., one or more of the orthogonal X, Y, Z axes summed together) and gain G 764 is configured to produce a vibration compensation signal VComp 766 (e.g., G·ka·a) indicative of mechanical vibrations and as a function of an oscillator tuning slope Kvco2 that is summed with the error signal 710 by summer 768 and fed to the feedback amplifier 714. The linearity of the error signal 710 to changes in oscillator frequency at the output of the mixer maintains a constant value of oscillator tuning slope Kvco2 to suppress the effects of mechanical vibrations on oscillator phase noise over a tuning range of the oscillator.
An accelerometer aligned with the earth's gravitational field will produce a constant DC output in addition to the response to vibrational accelerations. This will produce a constant degradation of the flicker noise in amplifier 738. By integrating the mixer error signal 712 via integrator 770 and summing it via summer 772 into either the feedback amplifier input or the loop phase shifter input (shown here), this DC offset can be removed on time scales longer than the integrator time constant.
To understand the operation of this arrangement, consider the voltage 710 generated at 712 in the absence of the feedback being applied between amplifier 714 and phase shifter 704. At the nominal oscillating frequency, f0, at or near the center of resonance, the signal in the reference arm, PREF (Bold used to indicate a phasor or vector quantity having magnitude and phase) and the reflection arm, PRFL, are equal and opposite, PREF=−PRFL and cancel at the combiner 736 leading to zero carrier power at the output of LNA 738 and zero voltage at the mixer output 712. However, if the frequency of oscillation varies by an amount much less than the bandwidth of the resonator, Δf<<BWRES, (for example because of a small fluctuation in loop phase caused by noise) then the power in the reflection arm becomes PRFL (1+Δf·kRflPh) where kRflPh=dS11</df is the slope of the resonator reflection phase with respect to frequency. Hence the input power at LNA 738 becomes PREF−PRFL=PRFL Δf·kRflPh and correct adjustment of the LO Phase shifter 742 results in a voltage at the mixer output 712 directly proportional to Δf·kRflPh. In typical applications the tuning range of the oscillator will be of order kHz while the BW of the resonator will be ˜100 kHz and in such cases kRflPh remains linear over the tuning range and the error signal voltage 710 at 712 is linearly related to a frequency error in the oscillator.
The normal action of the noise degeneration circuit when the feedback between amplifier 714 and phase shifter 704 is connected, is to reduce the error signal 710 at mixer output 712 (the input to amplifier 714) to very close to zero, the reduction depending on the gain around the feedback loop. Adding a voltage Vcomp 766 means the circuit will instead produce an equal and opposite voltage at mixer output 712, and a proportional change in oscillator frequency depending principally on kRflPh and being independent of any phase shifter characteristic. Thus, an alternative means of tuning the oscillator frequency is available, one that is highly linear in voltage. This has the effect of holding tuning slope KVCO2 at this point in oscillator constant.
In a frequency-tuned (e.g., phase-locked) INSO configuration, summing the vibration compensation signal to the error signal reduces the effects of mechanical vibrations on oscillator phase noise independent of the tuning voltage applied to the phase shifter 732. Even though KVCO1 at reference arm phase shifter 732 varies by perhaps 2× over the full tuning range this has no effect on the vibration compensation. KVCO2 characterizes a tuning slope relating the carrier frequency to the summed voltage of the error signal and the vibration compensation signal. Because the error signal responds linearly to changes frequency under open-loop conditions, KVCO2 remains constant. This is true independent of fixed or variable tuning voltage applied to reference arm phase shifter 732.
Referring now to
Referring now to
Although the application of Vcomp to mixer output 712 instead of the tuning port of phase shifter 732 achieves a marked improvement in phase noise in the presence of external vibration, the insertion of an additional signal into the oscillator loop at this point goes against long-established practice taught by U.S. Pat. No. 5,841,322 because doing so degrades carrier suppression, increasing the flicker noise contribution of LNA 738.
However, with many suitable choices of LNA 738 the effectiveness of the carrier suppression results in a flicker noise contribution from the LNA 738 of 10 dB, or more, lower than the noise generated by practical choices for other components such as attenuator 730, phase shifter 732, and mixer 734. For example,
While several illustrative embodiments of the disclosure have been shown and described, numerous variations and alternate embodiments will occur to those skilled in the art. Such variations and alternate embodiments are contemplated, and can be made without departing from the spirit and scope of the disclosure as defined in the appended claims.
Number | Name | Date | Kind |
---|---|---|---|
4318063 | Przyjemski | Mar 1982 | A |
4453141 | Rosati | Jun 1984 | A |
4891611 | Frerking | Jan 1990 | A |
5841322 | Ivanov et al. | Nov 1998 | A |
9350293 | Desrochers, II | May 2016 | B1 |
20050007204 | Howe | Jan 2005 | A1 |
20140104006 | Clark | Apr 2014 | A1 |
20160226500 | Zhao | Aug 2016 | A1 |
20170257105 | Patrizi | Sep 2017 | A1 |
Entry |
---|
Bloch, M., et al., “Acceleration “G” Compensated Quartz Crystal Oscillators”, 2009 IEEE International Frequency Control Symposium Joint with the 22nd European Frequency and Time forum, (Apr. 20, 2009), 6 pgs. |
Colson, Carl, “Vibration Compensation of the Seektalk Rubidium Oscillator”, 36th Annual Frequency Control Symposium, (Jun. 2, 1982), 3 pgs. |
Hati, A., et al., “Vibration Sensitivity of Microwave Components”, 2007 IEEE International Frequency Control Symposium Joint with the 21st European Frequency and Time Forum, Geneva, Switzerland, 541-546. |
Vig, John R., “Quartz Crystal Resonators and Oscillators”, For Frequency Control and Timing Applications—A Tutorial, (Jan. 2004), 21 pgs. |
Wanner, Shannon, “Vibration Correction of Oscillator for Phase Noise Impairments Utilizing MEMS Accelerometer”, 2017 Texas Symposium on Wireless and Microwave Circuits and Systems (WMCS), 5 pgs. |
Yoneoka, Shingo, et al., “Active Electrostatic Compensation of Micromechanical Resonators Under Random Vibrations”, Journal of Microelectromechanical Systems, vol. 19, No. 5, (Oct. 2010), 1270-1272. |