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9.2.2 RF Stage

The incoming signal is very weak—often at the microvolt or nanovolt level—and must be amplified by the RF stage before being passed to the mixer. In doing so, it is important that the RF stage not add any noise to what is already a weak noisy channel—as it amplifies the weak signal, it will also amplify the channel noise as well as the amplifier noise. The RF stage must also prevent certain troublesome frequencies such as image channels, harmonics, and other interference. The RF stage therefore performs the functions of low-noise pre-selection and RF amplification, which may be separate or combined circuits.

9.2.2.1 RF Amplification

A well-designed RF amplifier typically provides 10–30 dB of gain (corresponding to 10–1000 × voltage amplification). Multiple cascaded RF stages can improve sensitivity but make tracking between tuned circuits more complex. In some low-frequency or high-noise environments (for example, the LF and MF broadcast bands), an RF amplifier may actually degrade the signal-to-noise ratio because external noise dominates; such designs may therefore not include any amplification and simply couple the antenna directly to the mixer through a passive filter.

Because the RF stage is the first active stage encountered by the RF signal, it is the primary contributor of noise in the receiver and therefore to the receiver’s overall noise figure—it must therefore introduce the minimum possible internal noise. Modern receivers employ low-noise amplifiers (LNAs) with noise figures (see Section 0) often below 1 dB at microwave frequencies, implemented using GaAs, GaN, or CMOS front-end integrated circuits.

Because the RF amplifier is the first active stage encountered by the signal, its noise performance is critical. According to Friis’ formula for cascaded stages, the overall noise figure of a receiver is dominated by the noise figure of the first stage and the gain preceding subsequent stages. Any noise added at this point is amplified by all following stages and cannot be removed later in the signal chain.

For this reason, the first amplifier in modern receivers is specifically designed as a low-noise amplifier (LNA). An LNA is optimized to provide high gain with minimal internally generated thermal and shot noise. It must also maintain adequate linearity so that strong nearby signals do not drive it into compression or generate intermodulation products.

LNA design involves trade-offs among noise figure, gain, bandwidth, stability, power consumption, and dynamic range. In satellite and deep-space receivers, cryogenic LNAs may be employed to approach the thermal noise limit. In terrestrial and commercial systems, integrated CMOS or GaAs LNAs typically achieve noise figures well below 2 dB while maintaining sufficient linearity for operation in crowded spectral environments.

Modern systems further enhance RF performance through adaptive gain control, band-select filters, and automatic impedance matching circuits controlled by embedded microprocessors or digital signal-processing (DSP) units.

9.2.2.2 Pre-Selection

The pre-selection section of the RF Stage suppresses unwanted signals that could interfere with the IF stages. Its key functions include rejection of image channels, suppression of IF breakthrough, and reduction of intermodulation and cross-modulation effects.

9.2.2.3 Functions Of The RF Stage

In summary, the RF stage of a superheterodyne receiver provides a number of advantages: greater gain and therefore better sensitivity, better signal-to-noise ratio, and better selectivity. To achieve those aims, the stage must perform the following principal functions:

Modern receivers often integrate these functions into a single front-end module comprising an LNA, band-pass filter, and automatic gain control (AGC) circuitry under microcontroller supervision.