Politecnico di Milano Dipartimento di Elettronica e Informazione

Alfio Zanchi

Research History

 
 
 

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Jitter vs. Phase noise
Sensitivity analysis 
for the SSCR
Fast simulation techniques for
phase noise prediction
Time-varying 
noise analysis
for AAC loop
Layout 
and RF Board 
design
Experimental results

 



 
 

Jitter vs. Phase noise

Up to now, Alfio Zanchi has been involved in theoretical, simulation and experimental activity in the field of RF circuits for wireless front-end. This  research work is documented in some peer-reviewed scientific publications; some interesting topics are outlined here in the following.

The former section of the Ph.D. work led to devise a simple relationship between the Single Sideband to Carrier Ratio (SSCR) taken at offset fn away from the carrier at f0, and the cycle-to-cycle time jitter (sTo) of the period of an oscillator. The relationship found holds for the classical 1/fn2 shape of the phase noise:

Jitter vs. SSCR relationship IF the phase noise goes down as fn^-2


This link was experimentally verified by means of a CMOS ring oscillator, by adopting a spectrum analyzer to assess the SSCR (frequency domain), and a Time-to-Amplitude Converter (TAC) in order to measure the jitter of the period (time domain) [J1].

 

SSCR from the spectrum analyzer
The period duration histogram - its RMS gives the time jitter
Output spectrum of a ring CMOS oscillator :
SSCR(40 kHz) = -98 dBc/Hz
Time jitter of the oscillation period (1 ch. = 5.44 ps). 
The intrinsic uncertainty of the measurement system 
amounts to 3.4 ps rms
The frequency-time domain link has been extended then to a general phase noise shape, by resorting to a slightly more complex relation that can be efficiently exploited in numerical way:


Extended relationship, holding for ANY phase noise behavior (e.g, PLL)

This general formula has been successfully validated through the simulation (with Matlab®) of the popular case of PLL-based frequency synthesizers. The phase noise spectrum near the carrier is filtered by the loop action, and the time jitter of the period diminishes accordingly (14% with a PLL bandwidth as high as f0/10) [S4] .

Phase noise spectra for free-running VCO and PLL-constrained one
The details of spectra of the simulated signals close to the carrier frequency (1 GHz). 
The upper spectrum refers to the case of oscillators affected by 
white frequency noise (free-running VCO), 
the lower one to a highpass-filtered frequency noise (PLL synthesizer)

 
 
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Sensitivity analysis for the SSCR





From a more practical standpoint, the dominant part of the work concerned the effects that cause a phase noise degradation in LC-Tuned VCO’s, when they are forced to operate at high oscillation amplitudes. In effect, despite the general formula for the accounting of the SSCR reads [J2] :


SSCR formula: F accounts for the non-linearities of the loop, Q is the quality factor

thus indicating an improvement when the carrier power is raised, from the measurements performed on some RF demonstrators for DAB applications (Digital Audio Broadcasting) the SSCR was observed to reach a minimum and then steeply rise as the oscillation amplitude increased. This behavior sets a limit to the range where better performance can be traded against higher power dissipation.
 
On a differential LC-tuned VCO fabricated in high-speed bipolar technology, whose schematic is depicted here aside, we tried to carry on further attempts to quantitatively explain the SSCR behavior against the amplitude. 
At a first glance, the most likely source of amplitude-dependent phase noise instability was the AM-to-PM conversion [P1]. A preliminary theoretical study on the static characteristic of the tank was made, that proved to be consistent with the results of simulations both at behavioral level (Matlab modeling and analysis of the non-linearity of the tank) and at circuit level (Eldo software supported by STMicroelectronics models) [S3]. The conversion effect can explain the rise in SSCR at least from a qualitative point of view; but, once an experimental countercheck was performed through the injection of known amounts of noise in the circuit, it was found to be too small an effect as for quantitative predictions [P2] .

Simple LC-tank VCO schematic

Schematic structure of the tested VCO.
The LC tank is fully integrated on the silicon chip
 

Here below is depicted the AM-to-PM conversion coefficient (that we called KVo) as it was derived after a sensitivity-fashion equation such as:
The senistivity formula as applied to the output amplitude variations
Also, a device-level analysis has been carried out on the varactors of the tank, to clarify whether they could give rise to Q-loading effects [P1]. During the instants in which the varactor diodes are almost forward-biased, due to the positive peak of the oscillating voltage on the tank, direct currents can flow in fact into them, and load the quality factor of the resonator.

AM-to-PM coefficient vs. oscillation amplitude
Doping profiles of the varactorThe doping legend

KVo : AM-to-PM conversion factor on the tank
as simulated by using the charge-control 
varactor model of Anacad Eldo

Half-map of the dopant concentration regions issued in the vertical varactor structure,
with the  metallurgical boron-phosphorus junction and the lateral anode sinker
The in-depth simulations performed with TCAD Dessis® onto the device structure reported in the figure above, indicated however that the slight worsening in the AM-to-PM conversion efficiency could not account for the phase noise degradation actually noticed at high values of A0. The SSCR vs. amplitude dependence was instead fully explained by taking into account the low-frequency noise coupling to the tail of the differential VCO topology under test.

Not only noise and disturbances are transferred to the tank, but they also modulate the phase delay of the VCO loop due to the presence of active elements. Experimental and simulation procedures for the evaluation of this effect and of their impact on the circuit performance were considered, and are summarized in the next figure [J2] .

The solid curves show the SSCR vs. A0 as measured on the VCO, with the lower rail VEE connected to a band-gap voltage reference with SnV = 120 nV/éHz (solid curve with triangles) and directly to a cleaner ground (solid curve with circles). 

The base-line A was derived from the traditional non-linear theory that takes into account the switching regime of the circuit, and keeps decreasing. 
Curves B and C have been evaluated considering also the modulation of the phase delay of the transconductor due to the low-frequency noise.


SSCR vs. oscillation amplitude, with different amount of noise coupling to the VCO tail
Why does the circuit seem sensitive to the low frequency noise coming from the tail? The answer is found in the two pictures reported beneath :

Frequency vs. amplitude behavior, and the sensitivity according to
Dependence of the oscillation frequency on IT (solid line, referred to the left axis). 
The triangles (referred to the right axis) show 
the coefficient KIT as evaluated from the derivative 
dw0/dIT of the frequency curve. 

The squares are the values obtained by injecting 
harmonic current tones into the tail and computing the magnitude of the phase transfer: the results of the two methods match each other


A simplied single-ended model of the transconductor

Schematic representation of the LC-tuned oscillator, highlighting the load due to the transconductor and 
its internal delay.

The transconductor input impedance, in parallel 
to the tank, is essentially due to the base spreading
resistance rbb' and to the diffusion capacitance Cp
In fact, at w0 the base resistance rp is much larger 
than the impedance of Cp.. In effect, both the 
input impedance of the transconductor and the 
transistor transit time depend on IT and add a phase delay 
Dqloop to the feedback loop. According to the Barkhausen 
criterion, the oscillation frequency is therefore 
shifted away from the resonance frequency of the tank.
 

The oscillation frequency is a function of the phase delay met within the loop, Dqloop, and is obviously expected to depend on IT since it is [P2] :

Corrections on the oscillation frequency due to additional delays in the loop







This is exactly what we observe in the first graph. Taking the current noise SIT = 2.4 nA/éHzdue to the band-gap, and converting it into phase noise via the KIT sensitivity coefficient, the dashed line (B) previously highlighted is recovered, that perfectly matches the experimental values.
When taking the phase delay Dqloop obtained changing the tail current IT in the simulation of the open-loop circuit for computing the actual w0, we obtain again the frequency vs. amplitude dependence already observed from the circuit-level simulations.

In summary, the results confirm that the SSCR performance of the VCO is limited by the frequency sensitivity to the low frequency noise affecting the biasing current.
 
 
 
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Fast simulation techniques for phase noise prediction

As a byproduct of the simulation activity, some experimental and simulation techniques were devised that can be adopted to assess the importance of the sensitivity effect in other oscillator topologies too [P3]. The sensitivity analysis, based on the evaluation of derivatives like dw0/dIT, was proven equivalent to the traditional time-domain analysis performed by injecting low frequency harmonic tones into the circuit. The same approach can be also adopted in simulation, in place of the more time-consuming tone injection techniques, allowing for fast and accurate predictions of phase noise in oscillators even adopting inexpensive software, such as PSpice®.
Then a first, much faster technique based on sensitivity analysis was proposed, suitable for the estimation of phase noise due to low-frequency sources, e.g. 1/f noise. Finally, the high-frequency noise sources contribution to SSCR was analyzed through another alternative method based on the frequency demodulation of the carrier. Both of these methods allow the designer to quickly identify the noise sources mainly responsible for the instability of the carrier.

CPU load comparison for the different phase-noise assessment methods
Comparison of three simulation techniques for
the estimation of phase noise in oscillators. 
The CPU time required by each method accounts 
for both the Eldo simulation and the post-processing time 
(FFT for the traditional, differentiation for the sensitivity, 
and frequency extraction for the demodulation method)

 
 
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Time-varying noise analysis for the AAC loop

 
A separate branch of the research activity involved the study of the effects on the phase noise of a VCO, due to the presence of an eventual AAC [S1] .
The Automatic Amplitude Control (AAC) system is an increasingly popular servo-circuit for integrated VCOs, that provides control on the A0 in steady state and on the start-up transient. Nevertheless, the noise contributed to the oscillator by the AAC can degrade the phase noise performance of the overall synthesizer. In particular, the time-varying noise transfer function of the switching peak detector needed in the feedback path was analyzed, recognizing it as the critical noise source in the loop.
The circuit senses the amplitude of the oscillation and can regulate it at the phase noise optimum, by reacting onto the VCO cell bias current.
 
Block diagram of the control system. 
The output noise of the peak detector is not compensated for 
by the loop, as it comes embedded in the feedback path

Essential schematic of the VCO+AAC ensemble
The Matlab-Simulink® simulations of the time-varying noise gave rise to a collection of 2-D autocorrelation Ryy(t0 , t1), one for each trial of the stochastic process, that had to be further processed in order to gain statistical significance and obtain back a 1-D ergodic function.
 
 
The first process trial ...+... the second one ...+... the third one and so on ...+...
_________________________________________________________________________________________________
N
Ensemble average of N single-realization autocorrelations. The surfaces
are obtained in the case of a peak detector with 50% duty cycle
A 2-D time average, which can be performed in lieu of the required ensemble average thanks to the low-pass filtering action of the dominant pole, finally gives the autocorrelation surface :

The final autocorrelation after ensemble average has been performed
Autocorrelation averaged over 1000 statistically independent simulation trials, 
for a peak detector featuring 50% duty cycle
Fortunately enough, such a Ryy(t0 , t1) can be filtered so as to translate it into a numerically manageable 1-D autocorrelation, suitable for Fourier transformation.  The main result of this study concerned the identification of a rule that holds for the noise at the output of the stage: whether it comes from the resistor of the peak detector or from the rectifier diode, the current noise entering the block undergoes a filtering with constant GBWP. Although the noise filtering is quite complex owing to time-variance, this property is transmitted to the spectrum profile at the output of this stage, as clearly shown by the next figure.

Noise spectra at the peak detector output, after the dominant pole time average
Simulated noise power density spectra for increasing 
duty cycles of the peak detector switching regime.

The 0% d.c. level has been set to –54 dBV2/Hz

Further experimental validation of this characteristic was carried out by means of a discrete-components test board.

By exploiting this regularity of the output’s behavior, the seemingly severe problem of predicting the output spectrum can be successfully faced and overcome. From the analysis of the filter mechanisms, fast rules to predict the noise spectral density at the peak detector output can be sought. The final rules that can be used to account for the peak detector output noise are:

Short formula for the peak detector resistor current noise
Short formula for the rectifier diode current noise
where tON and tOFF are determined by the d.c. of the block, and it was defined a = exp(-TOFF/T)  and b = exp(-TON/T) [S1].

 
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Layout and RF board design

The theoretical and simulation work finally culminated in the design of some test structures of VCO. One of the most interesting topologies that were paid attention is the differential Colpitts. It consisted of two Colpitts-Clapp oscillators coupled back-to-back with two common-mode quenching resistors, purposely placed on the symmetry axis of the oscillator.
As for all of the other VCO circuits, the Colpitts stage was accurately sized and simulated, and the layout was finally produced. An example of the final design that has been diffused on silicon is reported in the figure here below:
Cadence layout of the 
mirrored-Colpitts oscillator.
The symmetry principle lies behind
the common-mode damping, 
and is exploited in the synchronization 
of the two halves of the VCO

Double-Colpitts layout
Up to 3 circuits of this kind have been accommodated into a single test chip with TQFP48 package. The final product of the project pursued during the Ph.D. were 6 test chips, arranged as depicted in the first figure below, that allowed separate characterization of the phase noise performance of each VCO. Also shown is a microphotograph of one of the VCOs finally diffused on silicon
 
 

Test Chip-II layout
The test chip CHIP-II as arranged for the eventual 
silicon run. The common substrate has been split apart 
in order to cancel out any noise source that may couple
to the VCO under operation.
The RF oscillation output paths have been kept the shortest,
both from routing and bonding standpoints
Here is a microphotograph of the VCO with 
the AAC system beneath it. The 2-turn spiral inductor 
can be viewed on top of the circuit, along with the 
central column of 12 varactors and 2 fixed-value, 
metal-to-metal capacitors. 
The  block with small vertical pitch placed under the tank 
is the VCO transconductor, holding 6 maximum-size 
bipolar transistors. The large capacitors seen to 
the bottom left of the image make up the dominant pole 
of the AAC, while the capacitor of the passive peak detector 
lies to the bottom right.

VCO and AAC layout as seen on the final silicon wafer

The last step towards the test of the circuits designed is the RF board preparation. The test cards have been realized with 4-layers, in standard FR4 dielectric material, with properly tailored gold-over-copper traces. The large epoxy component screwed over the card is a high-performance RF socket (Johnstech® - Giga3 family) into which the previously chips are inserted and locked.


RF board and socket picture

The RF board with mounted socket, bias voltage soldernails, 
and standard SMA output plugs

 
 
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Experimental results

Since it was observed before how the phase noise performance of the local oscillators used in the RF front-ends is strictly related to the oscillation amplitude, in some test circuits the VCO tank-transconductor core was accompanied with an Automatic Amplitude Control loop (AAC). In the test, the SSCR obtained at the optimal oscillation amplitude condition was measured to reach down to –104.5 dBc/Hz at 100 kHz from the 2.56 GHz carrier. The measurements also show that the AAC assures a wide-range (from 50 mV up to 1.3 V) and fast-settling (<100 ns) amplitude regulation, even with 2.4 V supply [S2].
As compared to a standalone oscillator with the same core, thanks to the loop gain of the AAC regulator the controlled-amplitude VCO features up to 10-dB rejection of the spurious tones, noise and outer interference possibly inserting into the bias nodes of the circuit.

The measured SSCR on the VCO+AAC bipolar technology oscillator

In conclusion, the performance of the structures designed: 
as low as –104.5 dBc/Hz @ 100 kHz from the 2.56 GHz carrier. 

The output spectrum sketched in the figure was measured in the 
Circuits and Systems Lab 
of the Electronics Dept. at the Politecnico di Milano
 


 
 
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He is now on the way to Texas Instruments, Data Converter design Group, where he will give his contribution in a mix of digital and analog design problems.

 
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