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Knowledge Hubris assisted isac system2. Echo Through an RIS: The Four-Hop Budget

ris assisted isac system learning note

2. Echo Through an RIS: The Four-Hop Budget

Derive a reciprocal aperture budget, separate one-way signal gain from echo gain, and test distance and panel-size penalties.

At a glance

  • Two distances, each traversed twiceIn the stated far-field model, echo power scales as d₁⁻⁴d₂⁻⁴.
  • Aperture helps on both passesFor the same reciprocal subarray, echo power scales as A⁴; power efficiency appears twice.
  • Check the domain firstAperture scaling assumes far-field legs, coherent steering and fixed antenna gains; it cannot be extended without limit.

Why Count Every Leg?

A communication receiver needs the outward BS–RIS–user path. A monostatic sensing receiver, located at the transmitter, also needs the target echo to return. Here we isolate BS–RIS–target–RIS–BS. Mixed direct/reflected paths require different budgets.

Let PtP_t denote transmitted power in watts, GtG_t and GrG_r dimensionless BS transmit and receive gains, λ\lambda wavelength, AA panel area, and η\eta power efficiency per reflection. Target radar cross section σ\sigma, in square metres, describes backscattered power in the observed direction. It is not simply the target’s physical area. Distances d1d_1 and d2d_2 are the two outward legs.

References for this section1

Derive the Budget in Four Steps

For an ideal broadside aperture, the incident power density at the RIS is S1=PtGt/(4πd12)S_1=P_tG_t/(4\pi d_1^2). Approximate the panel’s capture area by AA and its reradiation directivity by 4πA/λ24\pi A/\lambda^2.

  1. Illuminate the target: ST=S1ηA2/(λ2d22)S_T=S_1\eta A^2/(\lambda^2d_2^2).
  2. Scatter back to the panel: SR=STσ/(4πd22)S_R=S_T\sigma/(4\pi d_2^2).
  3. Redirect toward the BS: SB=SRηA2/(λ2d12)S_B=S_R\eta A^2/(\lambda^2d_1^2).
  4. Collect at the receiver: Pr=SBGrλ2/(4π)P_r=S_BG_r\lambda^2/(4\pi).

Each density SS is in W/m². Multiplying these steps gives this teaching model:

Pr=PtGtGrση2A4(4π)3λ2d14d24.P_r=\frac{P_tG_tG_r\sigma\eta^2A^4}{(4\pi)^3\lambda^2d_1^4d_2^4}.

This is an ideal aperture specialization, not a replacement for measured element patterns or the more detailed NLoS radar models in the references.

References for this section1

A Budget You Can Calculate

The lab fixes Pt=1P_t=1 W, Gt=Gr=100G_t=G_r=100 (20 dBi each) and frequency at 3 GHz. At the default distances 50 m and 30 m, panel area 0.64 m², efficiency 0.7 and cross section 1 m², the echo is approximately −80.9 dBm.

For bandwidth B=20B=20 MHz and receiver noise figure FdB=6F_{\rm dB}=6 dB, the room-temperature noise approximation is:

NdBm=−174+10log⁡10(B/1 Hz)+FdB≈−95.0 dBm.N_{\rm dBm}=-174+10\log_{10}(B/1\,\mathrm{Hz})+F_{\rm dB}\approx-95.0\ \mathrm{dBm}.

SNR, the signal-to-noise ratio, is Pr,dBm−NdBmP_{r,\rm dBm}-N_{\rm dBm}, approximately 14.1 dB here. Detection also depends on clutter, integration, a detection threshold and acceptable false alarms.

Can a four-hop echo reach the receiver?

1. Formula and symbols
Pr=PtGtGrση2A4(4π)3λ2d14d24P_r=\frac{P_tG_tG_r\sigma\eta^2A^4}{(4\pi)^3\lambda^2d_1^4d_2^4}
  • PtP_t: Transmitted power in watts
  • PrP_r: Received echo power in watts
  • GtG_t: Linear transmit gain at the BS
  • GrG_r: Linear receive gain at the BS
  • σ\sigma: target cross section
  • η\eta: aperture efficiency
  • AA: panel area
  • λ\lambda: wavelength
  • d1d_{1}: Distance between the BS and RIS
  • d2d_{2}: Distance between the RIS and target

This is the stated broadside far-field aperture model.

-120.0-90.0-60.0Received echo power (dBm); vertical scale adaptsRIS–target distance: 26 m (left) → 150 m (right)Receiver noise -95.0 dBm
2. Work with the current inputs
Pr=PtGtGrση2A4(4π)3λ2d14d24P_r=\frac{P_tG_tG_r\sigma\eta^2 A^4}{(4\pi)^3\lambda^2d_1^4d_2^4}
Pr=1×1002×1.0×0.702×0.644(4π)3(0.09993)2×504×304 W≈8.194×10−12 WP_r=\frac{1\times100^2\times1.0\times0.70^2\times0.64^4}{(4\pi)^3(0.09993)^2\times50^4\times30^4}\ \mathrm{W}\approx8.194\times10^{-12}\ \mathrm{W}
Pr,dBm=10log⁡10(1000Pr/1 W)=−80.9 dBmP_{r,\mathrm{dBm}}=10\log_{10}(1000P_r/1\,\mathrm{W})=-80.9\ \mathrm{dBm}
N=−174+10log⁡10(20×106)+6=−95.0 dBmN=-174+10\log_{10}(20\times10^6)+6=-95.0\ \mathrm{dBm}
3. Result
Echo power-80.9 dBm
Single-observation SNR14.1 dB
Far-field boundary25.6 m
Broadside reciprocal aperture model derived in this note, following the NLoS radar-equation approach of Aubry et al. (2021). Fixed 3 GHz, 1 W transmit power and 20 dBi transmit/receive gains. Each leg stays beyond 2D²/λ for a square panel. No clutter, fading, atmospheric loss or integration gain; SNR alone is not a detection probability.
References for this section1

Distance, Area and Efficiency Are Different Levers

  • Double either distance: echo falls by a factor of 16, approximately 12 dB.
  • Double both distances: echo falls by 256, approximately 24 dB.
  • Halve area at fixed wavelength: echo falls by 16 in this model.
  • Halve efficiency: echo falls by four because the same loss occurs twice.

These ratios hold with other quantities fixed. At fixed physical area, adding more simulation elements does not create an unlimited physical aperture gain.

References for this section1

Know Where the Formula Stops

For a square panel, conservatively use its diagonal D=2AD=\sqrt{2A} as the maximum aperture dimension. A conventional far-field check is d1,d2>2D2/λd_1,d_2>2D^2/\lambda. The lab keeps both distances beyond this boundary, increasing their minimum values when panel area grows. The model assumes calibrated coherent phases, broadside effective apertures and a reciprocal route. It omits clutter, blockage on the chosen legs, polarization mismatch and hardware saturation.

Near-field focusing requires spherical-wave modeling; changing frequency can also change antenna gain, efficiency and target cross section. Keep these dependencies explicit when comparing designs.

References for this section1

Takeaway

Write the route before writing a gain claim. Next, split the available surface between data and sensing and see the price of sharing it.

References for this section1

Check your understanding

0 of 4 answered

  1. If only the RIS–target distance doubles, what happens to echo power in this model?

  2. If both leg distances double while everything else stays fixed, what is the echo power ratio?

  3. If per-reflection power efficiency is 0.5, what efficiency factor enters the reciprocal echo budget?

  4. An echo is −90 dBm and receiver noise is −95 dBm. What is SNR before processing gain?

Complete references and further reading