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Polynomial Model of Blocker Effects on Small Signal Gain and Noise Figure for LNA/Mixer Devices Used in Wireless Receivers


Polynomial Model of Blocker Effects on Small Signal Gain and Noise Figure
for LNA/Mixer Devices Used in Wireless Receivers

Authors: William Domino, Nooshin Vakilian, & Darioush Agahi
             (all currently work for Skyworks Solutions, Inc.)

This article was previously published in the June 2001 edition of Applied Microwave & Wireless (which is no longer in print), and is reproduced here with the permission of the authors.


In designing today’s wireless handset receivers, it is important to maximize both receive sensitivity and resistance to undesired signals, also called “interferers”, or “blockers”. The starting place for receiver design is the calculation of budgets for noise figure and linearity, usually facilitated by a spreadsheet. While it is straightforward to find the cascaded noise figure (NF) and 1dB compression point (P1dB) using a spreadsheet calculation, it is often not clear how to use these to predict the actual performance of the receiver in the presence of a large blocker. To obtain a reasonably accurate prediction may instead require an inconvenient co-simulation of the system with circuit models embedded. However, a simpler approach is possible, which is still performed at the level of cascade calculations rather than simulation.




For a digital cellular system such as GSM (Global System for Mobile Communications), there are well-specified blocking tests, that include both inband and out-of-band interferers. In these tests, the receiver front end must be able to reject the blocker while amplifying the desired signal, without violating the maximum allowed bit error rate. For out-of-band blockers, much of the rejection comes from a receive-band filter placed in front of the low-noise amplifier (LNA). Some architectures also place a similar filter after the LNA and preceding the mixer, while others utilize an image-reject mixer. In the latter case, the LNA/mixer combination is often implemented as a single IC, and it must exhibit particularly good blocker resistance, as there is only one receive-band filter placed ahead of it.




In this article, the effect of blockers on LNA/mixer performance is studied. The objective is to produce a model, based on empirical measurements, of how an LNA/mixer’s small-signal gain and noise figure degrade in the presence of large blocking signals. Once such a model is made, it can be used to accurately predict the amount of receiver desensitization that results from varying blocker levels. The LNA/Mixer device used as an example is the Conexant RF212 dual-band image-reject downconverter for GSM.




Gain Compression


Typically, gain compression is modeled as only a 3rd-order behavior, that is,




                                              Vo = k1 Vin + k3 Vin3                                                         (1)



But gain compression is generally a saturation-type function that is not well modeled by the 3rd-order component alone, which causes a downward turn of the gain curve. Figure 1 is an illustration of how the addition of higher order terms can produce a curve that saturates. Of course, to truly model a saturation condition, one would require an infinite number of terms, however a few terms




Polynomial Compression Models - RF Cafe

Figure 1  Polynomial Compression Models


are enough to produce an adequate model. In all cases the use of the model must be stopped above the point where it strays from true saturation.



With 1st, 3rd, 5th, and 7th terms:



                               Vo = k1 Vin + k3 Vin3 + k5 Vin5 + k7 Vin7                                  (2)



To obtain the non-linear gain, the above equation is divided by the input voltage, which yields



                                 Gain = k1 + k3 Vin2 + k5 Vin4 + k7 Vin6                                   (3)



Note that the gain equation has only even-order terms. An equation of this type is particularly useful when Vin is a large blocker, and the gain is the small-signal voltage gain in the presence of this blocker. Of course, with Vin always representing the blocker, the coefficients will be different for the blocker gain and the small-signal gain, since the small signal always is compressed faster than the large signal. (Refer to appendix A.)




If the transfer function model is limited to 3rd-order and 5th-order non-linearity, and the coefficients are defined as positive quantities, then one can write the following equation for the large signal gain (LSG):



                           LSG =  k1 -   3/4 k3 (VLarge)2 +  5/8 k5 (VLarge)4                       (4)


Where VLarge is peak amplitude of the large signal blocker. Similarly the small signal gain (SSG) is:




                        SSG =  k1 -  3/2 k3 (VLarge) 2 +  15/8 k5 (VLarge )4                    (5)


Note that the 2nd order term is doubled for the small signal gain, while the 4th order term is tripled. The k3 term causes the small signal to be compressed faster than the large signal. The k5 term is the one that pulls the gain curve back up and keeps it from turning downward. Even though this term is tripled for the small signal gain, it is generally not enough to keep the k3 term from causing the faster compression.




Below in Figure 2 and Figure 3 are given some example results of compressions that occur according to these equations, where k1 is unity.




Small Signal Gain Compression with Coefficient K3 = .0025 - RF Cafe

Figure 2  Small Signal Gain Compression with Coefficient K3 = .0025



Small Signal Gain Compression with Coefficient K3 = .0050 - RF Cafe

Figure 3  Small Signal Gain Compression with Coefficient K3 = .0050

A couple of things become noticeable. First is that when there is only a 3rd-order term, the relation between SSG and LSG compression is independent of the 3rd-order term. For instance, it can be seen in the curves that a compression of 1.0dB in LSG causes a compression of about 2.1dB in SSG, for either case of k3, as long as k5 = 0. Secondly, the 5th-order term has only a small influence on the relation between SSG and LSG compression until the amount of compression becomes large. This is why compression is often modeled using 3rd-order non-linearity only.




In the method to be described, the coefficients of the SSG compression are directly determined by measurement and curve fit, rather than assuming they keep the precise relationship with the LSG coefficients that is seen in eq. (4) and (5). The noise figure increase that occurs is also measured and related to the small signal gain.



System Gain and Noise Model


Figure 4 is a diagram of our model showing how the blocker affects the gain and noise of the system.




Model for Blocker Effects - RF Cafe

Figure 4  Model for Blocker Effects



Based on equation (5), the blocker amplitude affects the small-signal voltage gain, as:




                                          SSG = a0 - a2(Blocker)2 + a4(Blocker)4                                  (6)



where a0, a2, and a4 take the place of k1, 3/2 (k3), and 15/8 (k5), respectively.




The three noise contributors are the basic noise figure of the system, the noise figure degradation due to the blocker, and the LO phase noise mixed onto the blocker. It can be seen that the blocker amplitude affects the last two of these. In our modeling exercise, it is most convenient to relate the noise figure degradation to the small-signal gain, which is compressed by the blocker. This relationship is best represented using 0th, 1st, and 2nd order terms:




                                        NoiseFactor = n0 - n1(SSG) + n2(SSG)2                                (7)



Actually the blocker causes the small signal gain to be reduced while the system noise increases, causing a composite degradation in the noise figure of the system. This is taken into account when the above equations are fit to actual measurements.



Finally, after the blocker itself sees some compression, the LO noise is reciprocally mixed onto it (refer to appendix B), and the noise at the blocker-desired frequency offset falls into the desired band. This noise is then summed in with the other contributors.



Figure 5 shows the test setup. Small-signal gain and NF are both measured on




Test Setup - RF Cafe

Figure 5  Test Setup



the HP8970B noise figure meter. The blocker generator is filtered so as not to emit noise in the desired band, and the LO generator is filtered so as not to emit noise that would mix with the blocker. Also, the IF output is filtered so the blocker does not hit the NF meter with excessive power. The combiner has isolators on either side of it. On the noise source side, the isolator protects the noise source from the blocker. On the blocker side, the isolator insures that the port sees 50W both inside and outside the passband of the blocker filter.



The gain and NF with no blocker is measured, then a blocker is applied and the measurement is repeated for different blocker amplitudes. The measurements are stopped once the blocker reaches the highest value expected in the GSM system, or once the noise figure degrades by more than about 6-8dB.



It should also be noted that the frequencies of the measured noise band and of the blocker need to be chosen to avoid mixer spurs. If the blocker is located on or near a low-order mixer spur, then the NF meter will register an incorrectly high measurement.



Generating the Model from the Data


The gain data is converted to voltage gain, and the noise figure data to noise factor, since the polynomial equations need to act upon linear quantities rather than dB. A spreadsheet is used to plot the data and produce best-fit curves. Figure 6 is the curve for the small-signal gain vs. blocker voltage for the Conexant RF212 LNA/Mixer in its GSM900 path. The left-hand side of the curve is artificially constructed by folding the data over, resulting in a fit that uses all even coefficients, to fit with equation (6).




Small Signal Gain vs. Blocker Voltage - RF Cafe

Figure 6  Small Signal Gain vs. Blocker Voltage



In the equation for the best-fit curve, only the even terms are significant because the curve was forced to be even. The orders of the significant terms are 0th, 2nd, and 4th. The 0th-order term is forced to be the same as the no-blocker gain. The equation for this curve defines the blocker dependence of the “small signal gain” box in Figure 4.




Figure 7 is a plot of the noise factor vs. small signal gain for the Conexant RF212 LNA/Mixer. The equation has terms of order 0th, 1st and 2nd. This equation defines (indirectly) the blocker dependence of the “noise figure degradation” box in Figure 4.




Noise Factor vs. Small Signal Gain - RF Cafe

Figure 7  Noise Factor vs. Small Signal Gain



Making Use of the Model


Once these polynomial equations are generated, they are used in a process where all of the noise contributions are summed, to find the carrier/noise ratio (C/N) at the LNA/mixer output. An example case is shown in Figure 8, where a desired signal of –102dBm and a blocker of –16dBm are incident on the LNA/mixer input.



To find the composite C/N, the basic quantities of gain, noise figure, and P1dB are required, as are the coefficients of the small-signal gain polynomial (a0, a2, a4), and the noise factor polynomial (n0, n1, n2). We find the small signal gain and the noise figure based on the level of the blocker, and then add the reciprocally mixed LO phase noise at the end.



We must apply the large signal compression to the blocker itself, since in our model this compression occurs before the LO noise reciprocal mixing is applied. A polynomial with higher orders can be applied for the LSG just as for the SSG, but in our experience it is adequate to apply 3rd-order distortion only for the LSG, as long as the large signal does not go far beyond the P1dB point of the system.  Therefore the LSG coefficients can be derived either in the same manner as the SSG coefficients, or they can be taken from the measured P1dB and the relationship in eq. (4) where k5=0. Appendix C details the P1dB derivation.



Example of Model's Prediction of C/N - RF Cafe

 Figure 8   Example of Model's Prediction of C/N (click to enlarge)


For our example, the –16dBm blocker at the input of the Conexant RF212 LNA/Mixer causes the noise figure to degrade from 2.5dB (the typical value with no blockers present) to 6.5dB. The small signal gain drops in the process from 21.6dB to 16.75dB. Then the cumulative effects of the compressed SSG and NF result in a 12.5dB C/N before the LO noise is added, reciprocally mixed onto the blocker which has been amplified by the LSG. The sum total C/N is 7.8dB.




What makes the approach powerful is that once the model is derived, in can be plugged into the chain calculations for a complete receiver. Then, various what-if analyses can be done with accurate results for any blocker level hitting the LNA/mixer. For example, the effect of different front-end SAW filters with different levels of stopband attenuation for out-of-band blockers can be checked, and an accurate trade-off can be made between the SAW’s passband insertion loss and its stopband selectivity.



Furthermore, the approach can be used to accurately estimate the sensitivity level for a receiver in the presence of a blocker. In the typical GSM receiver, the sensitivity level is where the C/N drops to about 6.0dB. For our example with a –16dBm blocker, the sensitivity level estimate is –103.8dBm.




The calculation can also show which contributors are the most important. In this example, it turns out that even with the seemingly high noise figure of 6.5dB, the LO phase noise floor of –150dBc/Hz is still the most significant contributor to the system noise, due to the blocker’s presence. If the LO phase noise improves by 1dB, then the sensitivity improves by 0.7dB.









Presented in this article were steps in generating a polynomial model of blocker effects on small signal gain and noise figure for LNA/Mixer devices used in wireless receivers.   Based on empirical measurements of gain and noise figure of the device, the polynomials relating gain compression and noise figure degradation to blocker level at the input of device were generated.  The polynomial coefficients then were applied to the calculation of carrier-to-noise ratio in the presence of a blocker. The method makes it possible for a variety of what-if analyses to provide accurate results in predicting blocker-degraded C/N.







1)     W. E. Sabin and E. O. Schoenike, “Single Sideband Systems and Circuits”, second edition, McGraw Hill, 1995



2) Behzad Razavi, “RF Microelectronics”, Prentice Hall, 1998





William Domino is Principal Engineer for GSM RF Systems Engineering at Conexant Systems in Newport Beach, CA. He may be reached via email at




Nooshin Vakilian is Systems Engineer for GSM RF Systems Engineering at Conexant Systems. She may be reached via email at




Darioush Agahi is Director of GSM RF Systems Engineering at Conexant Systems. He may be reached via email at




Appendix A:  Non-Linear Analysis for Large and Small Signals



Using a power series expansion, the output of a gain stage can be related to its input as:




Vo(t) = k1 vi(t) + k2 vi2(t)  + k3 vi3(t) + k4 vi4(t) + k5 vi5(t) + …………………….                                    (a1)




Note that if the gain were perfectly linear, then k1 would be the only non-zero coefficient, and the gain would be identical to k1.




For a two-tone input, Vi(t) is:




Vi(t) = A  Cos(w1t) + B  Cos(w2t)                                                                                                  (a2)




Inserting (a2) into (a1) and using the well-known trigonometric equalities, one can expand the expression for Vo(t) to the following:






Vo(t) = 1/2 k2 A2 + 1/2 k2 B2 + { k1 A + 3/4 k3 A3 + 3/2 k3 AB2 + 5/8 k5 A5 + 15/4 k5 A3B2 + 15/8 k5 AB4 } Cos(w1t) +




            {k1 B + 3/4 k3 B3 +  3/2 k3 A2B + 5/8 k5 B5 + 15/4 k5 A2B3 + 15/8 k5 A4B} Cos(w2t)  + 




           {1/2 k2 A2 + 1/2 k4 A4 + 3/2 k4 A2 B2} Cos(2w1t) + { 1/2 k2 B2 + 1/2 k4 B4 + 3/2 k4 A2 B2} Cos(2w2t) +




          {k2 AB + 3/2 k4 A3B +  3/2 k4 AB3} Cos((w1 + w2) t ) + {k2 AB + 3/2 k4 A3B + 3/2 k4 AB3} Cos((w1 - w2) t )   +




          {1/4 k3A3 + 5/16 k5A5 + 5/4 k5A3B2} Cos(3w1t)  + {1/4 k3B3 + 5/16 k5B5 + 5/4 k5A2B3} Cos(3w2t)  +




         {3/4 k3 A2B + 5/4 k5A4B + 15/8 k5 A2B3} Cos((2w1 ± w2) t )  +




          {3/4 k3 AB2 + 5/4 k5AB4 + 15/8 k5 A3B2} Cos((w1 ± 2w2) t )  +




            1/2 k4 A3B Cos((3w1 ± w2) t )  + 1/2 k4 AB3 Cos((w1 ± 3w2) t ) + 3/4 k4 A2B2 Cos((2w1 + 2w2) t )  +




            1/8 k4A4 Cos(4w1t)  + 1/8 k4B4 Cos(4w2t) …………………….                                                                                          (a3)




The two terms that are of interest are the first-order gain terms. At frequency w1 the output voltage is:




Vo(w1) =  k1 A +  3/4 k3 A3 + 3/2 k3 AB2 + 5/8 k5 A5 + 15/4 k5 A3B2 + 15/8 k5 AB4                                                   (a4)




And similarly at w2 the output voltage is:




Vo(w2) =  k1 B +  3/4 k3 B3 + 3/2 k3 A2B + 5/8 k5 B5 + 15/4 k5 A2B3 + 15/8 k5 A4B                                                              (a5)




Dividing both sides of equations (a4) and (a5) by their respective inputs would yield gain at the corresponding frequencies:




G(w1) =  k1 +  3/4 k3 A2 +  3/2 k3 B2 + 5/8 k5 A4 +  15/4 k5 A2B2 + 15/8 k5 B4                                                                     (a6)




G(w2) =  k1 + 3/4 k3 B2 +  3/2 k3 A2 + 5/8 k5 B4 + 15/4 k5 A2B2 + 15/8 k5 A4                                                                      (a7)




Let’s assume A represents the large signal blocker and B the small desired signal. This means A>>B, therefore we can approximate the above gain terms by letting B go to zero:




G(w1) =  k1 +  3/4 k3 A2 + 3/2 k3 B2 +  5/8 k5 A4 +  15/4 k5 A2B2 + 15/8 k5 B4                                                                   (a8)




G(w1) =  k1 +  3/4 k3 A2 + 5/8 k5 A4                                                                                                                                           (a9)




Similarly we have;




G(w2) =  k1 +  3/4 k3 B2 +  3/2 k3 A2 +  5/8 k5 B4 +  15/4 k5 A2B2 +  15/8 k5 A4                                                                (a10)




G(w2) =  k1 + 3/2 k3 A2 +  15/8 k5 A4                                                                                                                                        (a11)




Equations (a9) and (a11) relate the large signal gain and small signal gain respectively of an amplifier. The interesting point is that both gains depend on the large signal amplitude, and further that under large signal interference, the small signal gain suffers faster. This is apparent by comparing the coefficients of A2 and A4 in the above equations.




Appendix B:  Reciprocal Mixing



In a receiver, a small desired signal may be accompanied by a large blocking signal at some frequency offset. The local oscillator that is used to mix the desired channel to IF exhibits finite phase noise at this frequency offset. When the two signals are mixed by the LO, each one has the LO’s phase noise spectrum modulated onto it. This process is referred to as “reciprocal mixing”. Therefore the downconverted band consists of two overlapping spectra, with the wanted signal suffering from significant noise overlap due to the tail of the


blocking signal’s spectrum.






RX Input Signals, and LO with Phase Noise Spectrum - RF Cafe

Figure B1  RX Input Signals, and LO with Phase Noise Spectrum



Signals Downconverted to IF, with Overlap of Reciprocally-Mixed Noise - RF Cafe

Figure B2  Signals Downconverted to IF, with Overlap of Reciprocally-Mixed Noise


Appendix C:  P1dB Point from 3rd-Order Coefficient



To obtain the value of single-tone P1dB gain compression induced by only 3rd-order non-linearity, equation a3 of Appendix A is used, setting higher order terms as well as signal “B” to zero.




Vo(w1) =  k1 A +   3/4 k3 A3 +  3/2 k3 AB2 +  5/8 k5 A5 +  15/4 k5 A3B2 +  15/8 k5 AB4             (c1)




Setting the higher order terms equal to zero yields




Vo = { k1 A +  3/4 k3 A3 +  3/2 k3 AB2 }                                                                                  (c2)




Setting B = 0 and dividing both sides by A yields




Vo = { k1 A +  3/4 k3 A3 }                                                                                                       (c3)




G =  Vo/A= k1 +  3/4 k3 A2                                                                                                      (c4)




Equation (c4) is the gain with third-order non-linearity.




At the P1dB point, the overall gain is reduced by 1 dB from the linear gain, that is, the voltage gain becomes k1*(10-1/20). To find the amplitude at the P1dB point occurs, one needs to solve the following:




k1 +  3/4 k3 A2 = 10-1/20 k1     Þ       A2   =   4/3 { 10-1/20  -  1 } (k1/k3                             (c5)




Note that at this point, “A” represents amplitude at which P1dB occurs.




For ease of manipulation, we set




a    =   4/3 { 10-1/20  -  1 }                                                                                                       (c6)







A   =    √(a  k1/k3)                                                                                                                  (c7)




Equation (c7) represents the amplitude at which gain is compressed by 1dB.


To find 1dB compression point in terms of power, we can start with equation (c3) again:




Vo = { k1 A +  3/4 k3 A3 }




Next raise both sides to power 2, which yields




Vo2  = { k1 A +  3/4 k3 A3 }2                                                                                                 (c8)




After some routine arithmetic and replacing A with its equivalent a,




Vo2  = { a +  3/2 a2   +   9/16 a3}  (k13/k3)                                                                           (c9)




However a can be numerically evaluated as




a =  4/3 { 10-1/20  -  1 } = - 0.145




And Vo2 becomes




 Vo2  =  - 0.11518 (k13/k3)                                                                                                  (c10)




Now Vo is a peak voltage (call it Vp). Converting to dBm yields




PdBm =  10 Log {  (Vp2/2R) 1000 }  =  10 Log {Vp2   50/R 10}                                                 (c11)




where R is the system source resistance            .




Inserting (c10) into (c11) gives P1dB in terms of the amplifier’s coefficients:




P1dB  = 10 Log {- 0.11518 (k13/k3)  50/R  10 }                                                                      (c12)






Since an amplifier’s k3 is a negative term, its sign can be absorbed and the term can be presented in the absolute form, which then results in:




P1dB  = 10 Log { (k13/|k3|) 50/R }  + 0.614                                                                         (c13)




In a 50 W system the R term vanishes and P1dB reduces to:




P1dB  = 10 Log {k13/|k3|}  + 0.614                                                                                     (c14)