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Low noise amplifiers (LNA)

A low-noise amplifier (LNA) is a special electronic signal amplifier that boosts very weak signals while adding minimal noise, thereby preserving the incoming signal's signal-to-noise ratio (SNR). It is primarily used at the front end of RF and wireless receiver chains, where incoming signals typically have very low SNR.

LNA pin outs

LNA architectures

LNAs are typically designed with a 50 Ω input resistance and minimal input reactance. This requirement decides LNA architecture1. The gain stage is made using a single transistor with inductive loading. Cascodes are added to provide better reverse isolation.

LNA architectures

Cascode-type LNA with inductive degeneration

Inductive degenerated and cascode LNA

The cascode type LNA with inductive degeneration is the most popular topologies because it offers best noise figure while matching the input among all narrow band LNA types. Cascoding helps achieving high reverse isolation2.

Important LNA parameters

Low noise amplifier signal chain

Amplifier S-matrix

$$[S]=\begin{bmatrix}s_{11} & s_{12} \\ s_{21} & s_{22}\end{bmatrix}$$

Input matching

Input matching is required to achieve maximum power gain and avoid reflections. In addition, preceding transmission line need a 50Ω termination to operate correctly. Proper matching also allows the LNA to be connected to an antenna at an unknown distance without concern for the transmission line length.

Return loss

Return loss indicates how of the incident signal is reflected back. Ideally, return loss should be zero. It is represented by reflection coefficients.

Input reflection coeffcient

$$\Gamma{}_{in}=s_{11}+\cfrac{s_{12}s_{21}\Gamma{}_L}{1-s_{22}\Gamma{}_L}$$

Γin is the input reflection coefficient and represents input return loss. It equals s11 if ΓL is zero (load is matched). ΓL is the load reflection coeffcient.

Input return loss vs frequency

Datasheet plot of Input return loss.

Output reflection coeffcient

$$\Gamma{}_{out}=s_{22}+\cfrac{s_{12}s_{21}\Gamma{}_S}{1-s_{11}\Gamma{}_S}$$

Γout is the output reflection coefficient and represents output return loss. It equals s22 if ΓS is zero (Source is matched). ΓS is the source reflection coeffcient.

output return loss vs frequency

Datasheet plot of output return loss.

Noise

Noise factor is defined by the ratio of output SNR and input SNR. It shows the degradation of signal's SNR due to the circuits that the signal passes through. Noise figure is the dB form of noise factor.

Noise factor of cascaded system

An RF receiver signal chain consists of a cascaded set of components, with the antenna and LNA positioned at the front end.

$$F_{total}=F_{LNA}+\cfrac{F_{postLNA}-1}{Gain_{LNA}}$$

The LNA’s noise factor directly contributes to the overall system noise factor, while its gain reduces the impact of noise from subsequent stages.

Noise figure of basic LNA

Basic LNA noise model

$$\text{F}=1+\cfrac{R_g}{R_s}+\left(\cfrac{\gamma{}}{\alpha{}}\right)\left(\cfrac{\omega{}}{\omega{}_T}\right)^2g_mR_s$$

For long channel MOS devices, γ=2/3 and α=1. γ is the noise modeling factor in: $$\bar{i_d}^2=4kT\gamma{}g_m$$

ωT is transistor's unity gain bandwidth. Rg is the distributed gate resistance which can be reduced by increasing the number of fingers. The above LNA architecture is not matched for a transmission line at the input. Matching the input for transmission lines poses limitation of achievable noise figure. These are discussed in LNA architecture section.

Noise figure vs Frequency

Gain

Gain is used to amplify signals which helps to reduce input referred noise of he subsequent stages. This gain is the small signal gain of the amplifier. It is represented by s-parameter s21. For integrated circuit implementation, the input of the LNA is interfaced off-chip and usually matched to 50 Ω impedance. Its output is necessarily not matched if directly interfacing inside the integrated circuit to a load (e.g., input of mixer or a filter).

Gain vs Frequency

Datasheet plot of gain across frequency.

Power gain

For a unilateral device (s12=0) power-gain is defined as power delivered to the load divided by the power available from source.

$$G_T=\cfrac{1-|\Gamma{}_S|^2}{|1-s_{11}\Gamma{}_S|^2}|s_{21}|^2\cfrac{1-|\Gamma{}_L|^2}{|1-s_{22}\Gamma{}_L|^2}$$

Linearity

The system's DC-transfer function can be modeled as :

$$Y_t=a_0+a_1X_t+a_2X_t^2+a_3X_t^3$$

If two strong slightly out of band inteferers appear at the LNA input, intermodulation distortion (3rd order nonlinearity) comes inside the band as shown below:

Intermodulation distortion effects

These large in-band blocker can desensitize the circuit.

Two-tone test is deployed to measure intermodulation distortion. Interferer can be modeled as :

$$X_t=A_1\cos(\omega{}_1t)+A_2\cos(\omega{}_2t)$$

P1dB and Psat

The third order nonlinearity is compressive in nature because the output cannot go beyond supply voltage (or 2X of supply voltage is case of inductive load). Mathematically, compression happens when the third-order coefficient is negative when the linear coefficient in positive (a3a1 < 0).

P1dB is the output power when the amplifier is at the 1 dB compression point.

1dB compression point

As shown in the graph above, the P1dB is measured by plotting output power vs input power and marking the point when the real curve is 1dB away from the ideal curve.

Psat is the output power when the amplifier is saturated. The output stops changing with increase in input power.

P1dB vs Frequency

Datasheet plot of P1dB across frequency.

Psat vs Frequency

Datasheet plot of Psat across frequency.

Output IP3 (OIP3)

When two-tone test is done, following fundamental and IM3 components are obtained :

Fundamental components

$$v_{fund}=a_1A_1+\cfrac{3}{4}a_3A_1^3+\cfrac{3}{2}a_3A_1A_2^2$$

If both amplitudes are equal,

$$v_{fund}=a_1A+\cfrac{9}{4}a_3A^3$$

The above term will compress when A starts becoming large. We will take only the linear extrapolated term for OIP3 calculation,

$$v_{fund}=a_1A$$

IM3 components

$$v_{im3}=\cfrac{3a_3A_1^2A_2}{4}$$

If both amplitudes are equal,

$$v_{im3}=\cfrac{3a_3A^3}{4}$$

Intermodulation distortion

At lower amplitude, the fundamental component dominates over the IM3 products. However, at higher amplitudes, the IM3 components grow to become equal to or even exceed the fundamental amplitude. The interection point is called IP3.

$$v_{im3}=v_{fund}$$

$$\implies{}A=\sqrt{\cfrac{4a_1}{3a_3}}$$

$$I_{IP3}=10\log_{10}\left(\cfrac{A^2}{R_0}\right)$$

The above amplitude is called output intermodulation intercept point. This is the input amplitude where the linear and intermodulation-3 distortion meet.

OIP3 vs Frequency

Datasheet plot of output intermodulation intercept point across frequency.

Reverse isolation

Reverse Isolation is a measure of the ability of an LNA to prevent signals from leaking or coupling back into its input port from its output port. In simpler terms, it quantifies how effectively an LNA isolates its output port from the input port. S12 of an LNA indicates reverse isolation. In real world LNA, S12 is near -40dB, This means that the signal leaks from the output port back to the input port with only 1/10,000 of the output power. More negative dB values indicate better isolation.

Reverse isolation vs Frequency

Datasheet plot of reverse isolation.

Unconditional stability of LNA

To ensure un-conditional stability of LNA, Stern factor is used3. The formula is:

$$K=\cfrac{1+|\Delta{}|^2-|s_{11}|^2-|s_{22}|^2}{2|s_{21}||s_{12}|}$$

Where Δ(=s11s22-s12s21) is the determinant of the s-matrix. For the LNA to be unconditionally stable, K should be greater than unity and |Δ| < 1. When the LNA’s input and output are matched to the source and load impedances, S11 and S22 approach zero. As S12 decreases, |Δ| also decreases, indicating improved stability of the LNA.

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