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Latest News || 27 October 2026: Dr Soumava Mukherjee's invited talk at Queen's University Belfast joined device-level hardware innovation with channel-level control. || 22 October 2026: I received a Certificate of Appreciation for serving as a reviewer for IEEE IMAS 2026. || 15 October 2026: I presented a poster on beam-domain ML fingerprinting for RIS-aided mmWave localisation at the Centre for Wireless Innovation's annual symposium. || 15 October 2026: CWI's annual symposium brought research and industry perspectives on 6G, ISAC, optical wireless, AI, and future networks to Queen's University Belfast. || 14 October 2026: Erik Nordell of Ericsson visited our Keysight Lab for a live RIS-assisted video streaming demonstration.
Knowledge Hubris assisted isac system5. Research Directions and Hardware Trade-offs

ris assisted isac system learning note

5. Research Directions and Hardware Trade-offs

Compare active, STAR and hybrid surfaces using noise and energy budgets, then ask what measurements support a research claim.

At a glance

  • Gain amplifies noise tooAn active stage can overcome downstream receiver noise, but its input-referred noise sets an SNR ceiling.
  • Two sides share energyFor a passive STAR surface, transmitted and reflected power fractions satisfy T + R ≤ 1.
  • Evidence needs a baselineCompare hardware, algorithms and experiments under stated power, aperture, calibration and overhead assumptions.

Active RIS: Signal Gain and Noise Gain

An active RIS supplies amplification; a passive RIS supplies reflection without amplifier gain. Amplification can overcome downstream receiver noise but also forwards upstream noise and adds its own noise.

For an illustrative single-stage model, let SS be signal power, NinN_{\rm in} input noise, NampN_{\rm amp} input-referred added noise, NrxN_{\rm rx} downstream receiver noise and GG linear power gain. Refer all powers to the same output reference plane before applying GG:

γ=GSG(Nin+Namp)+Nrx,lim⁡G→∞γ=SNin+Namp.\gamma=\frac{GS}{G(N_{\rm in}+N_{\rm amp})+N_{\rm rx}},\qquad \lim_{G\to\infty}\gamma=\frac{S}{N_{\rm in}+N_{\rm amp}}.

This is a generic amplifier-noise illustration, not a complete active-RIS radar equation. The lab holds signal and noise reference powers fixed to isolate the ceiling. A physical comparison also needs surface output power, saturation, stability and the actual multi-pass noise paths.

Does more active gain always improve SNR?

1. Formula and symbols
γ=GSG(Nin+Namp)+Nrx\gamma=\frac{GS}{G(N_{\rm in}+N_{\rm amp})+N_{\rm rx}}
  • GG: active linear power gain
  • SS: input signal power
  • NinN_{\rm in}: incident noise
  • NampN_{\rm amp}: input-referred added noise
  • NrxN_{\rm rx}: receiver noise

Convert dBm to linear power before adding noise terms.

-16.0-5.06.0Output SNR (dB); amplified noise sets a ceilingActive gain: 0 dB (left) → 30 dB (right)
2. Work with the current inputs
γ=GSG(Nin+Namp)+Nrx,G=1010/10\gamma=\frac{GS}{G(N_{\rm in}+N_{\rm amp})+N_{\rm rx}},\quad G=10^{10/10}
Nout/mW=1010/10(10−105/10+10−95/10)+10−100/10Nout,dBm=−84.46\begin{aligned}N_{\rm out}/\mathrm{mW}&=10^{10/10}(10^{-105/10}+10^{-95/10})\\&\quad+10^{-100/10}\\N_{\rm out,dBm}&=-84.46\end{aligned}
γdB=(−100+10)−(−84.46)=−5.54 dB\gamma_{\rm dB}=(-100+10)-(-84.46)=-5.54\ \mathrm{dB}
3. Result
Active output SNR-5.54 dB
Passive reference SNR-1.19 dB
High-gain ceiling-5.41 dB
Illustrative single-stage active-return model, not the full four-hop budget. Signal (−100 dBm), surface-input noise (−105 dBm) and input-referred amplifier noise are all referred to the receiver before the adjustable gain. Receiver noise is −100 dBm. Uncorrelated powers add; saturation and power limits are ignored.
References for this section3

STAR-RIS: Two Sides, One Energy Budget

A simultaneous transmitting and reflecting surface can direct energy to either side. For a passive panel, let TT and RR be transmitted and reflected power fractions, η\eta total usable efficiency and ρ\rho the fraction of usable power assigned to transmission:

T=ηρ,R=η(1−ρ),T+R=η≤1.T=\eta\rho,\qquad R=\eta(1-\rho),\qquad T+R=\eta\leq1.

Field-amplitude coefficients have magnitudes T\sqrt T and R\sqrt R. Do not confuse them with power fractions. If an echo traverses the panel twice by transmission, this part of its budget is T2T^2, not TT. Independent amplitude and phase choices are an idealization; physical implementations can impose coupled transmission/reflection phases.

Can both sides receive all the incident power?

1. Formula and symbols
T=ηρ,R=η(1−ρ),T+R=η≤1T=\eta\rho,\quad R=\eta(1-\rho),\quad T+R=\eta\leq1
Ptwo passes/Pincident=T2P_{\rm two\ passes}/P_{\rm incident}=T^2
  • η\eta: total passive power efficiency
  • ρ\rho: split toward transmission
  • TT: Transmitted power fraction
  • RR: Reflected power fraction

T² is the normalized fraction after two independent passages through the transmitting side.

Incident: 100%T: 40.0%R: 40.0%STAR-RIS panelLoss: 20%Two-pass T²: 16.0%
2. Work with the current inputs
T=ηρ=0.80×0.50=0.400,R=η(1−ρ)=0.400T=\eta\rho=0.80\times0.50=0.400,\quad R=\eta(1-\rho)=0.400
T+R=0.80≤1,T2=0.1600T+R=0.80\leq1,\qquad T^2=0.1600
3. Result
Transmitted / reflected40.0% / 40.0%
Absorbed or otherwise lost20%
Two-pass transmission factor16.0%
Passive STAR-RIS energy-splitting model: T and R are power fractions, not field amplitudes. Uniform splitting and independent phase steering are idealizations; real transmission and reflection phases can be coupled. An echo crossing the transmitting surface twice carries a T² penalty before other path losses.
References for this section3

Multifunctional and Hybrid Surfaces

Hybrid and multifunctional architectures add receiving, sensing or other functions to a reflecting surface. Compare what each proposed implementation actually measures, how it is calibrated and how much power and control signaling it needs. More functionality is a hardware design choice, not a free channel-estimation solution.

References for this section3

Learning, NOMA and Near-Field Designs

  • Learning-based control: evaluate beam prediction on unseen geometry and movement; include training data, inference latency and scan overhead.
  • Non-orthogonal multiple access (NOMA): users share resources with power allocation and successive interference cancellation. Account for decoding errors and user pairing.
  • Near-field focusing: use spherical-wave distances when plane-wave assumptions fail. Report the physical aperture and target distance, not only element count.

The phase-focusing lab in the preceding note shows how to inspect a simplified spherical-wave sum before making a system-level claim.

References for this section3

Experimental Evidence

Yasmeen, Kundu and Ram report an around-the-corner RIS experiment at 5.5 GHz capturing walking micro-Doppler signatures under NLoS conditions. It is a concrete example of a particular geometry and hardware setup, not a universal coverage guarantee.

For a prototype, record surface response, calibration procedure, target trajectory, clutter, bandwidth and an equal-resource baseline. A simulation supports a model; an experiment tests how that model survives a specific environment.

References for this section3

Takeaway

Choose an architecture by its energy, noise and measurement budget. Next, include control overhead and mobility before calling the design deployable.

References for this section3

Check your understanding

0 of 4 answered

  1. A passive STAR surface has total usable power efficiency 0.8 and splits that equally. What are T and R?

  2. If T = 0.4 on each of two transmissions through the same surface, what factor remains before other losses?

  3. If an amplifier boosts both a signal and its dominant input noise by 10 dB, with no added noise, what happens to their SNR?

  4. At fixed surface efficiency η = 0.8, transmission takes 75% of usable power. What is reflected incident-power fraction?

Complete references and further reading