The Array-Fed RIS Architecture

Collapsing One Side of the Double Fading

The double-fading theorem of Section 21.1 tells us that a passive RIS only helps when at least one of the two path lengths d1,d2d_1, d_2 is small. In a conventional deployment, d1d_1 (transmitter to RIS) is typically a meaningful fraction of the cell radius β€” hundreds of metres at mmWave, still tens of metres at sub-THz. But nothing in the physics forbids us from placing the RIS directly in front of the transmitter. What if d1β†’0d_1 \to 0?

The architecture that makes this idea concrete is the array-fed RIS: a small active array of Naβ‰ͺNRISN_a \ll N_{\text{RIS}} elements sits just a few wavelengths in front of a large passive RIS, illuminating it from the reactive-near-field side. The active array is a compact, amplified "injector" that couples power into the RIS; the RIS acts as a large- aperture lens or reflector that focuses the illumination toward the user. The end-to-end link pays only one path loss β€” the long one, RIS to user β€” and the nominal aperture gain GRISβ‰ˆNRISG_{\text{RIS}} \approx N_{\text{RIS}} survives intact.

This is the CommIT architecture of Caire and collaborators. It replaces the question "how do we make an RIS useful at long Tx β†’\to RIS distance?" with the cleaner question "how do we efficiently feed a large passive aperture with a small active array?". The answer turns a theoretical curiosity into a power- and hardware-efficient mmWave/sub-THz architecture.

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Definition:

Array-Fed RIS Architecture

An array-fed RIS consists of two co-located aperture stages:

  1. An active array feed with NaN_a RF-chain-backed elements that transmits the physical signal. The active array is compact (typical aperture ∼5\sim 5–20Ξ»20\lambda) and sits at a short fixed distance dfd_f from the RIS (typical df∈[2,10] λd_f \in [2, 10]\, \lambda, i.e. inside the reactive near field of the RIS).

  2. A passive reflecting RIS with NRIS≫NaN_{\text{RIS}} \gg N_a elements. Each RIS element has unit-modulus reflection Ξ“n=ejΟ•n\Gamma_n = e^{j\phi_n} and is configured by the BS controller.

The compound signal model, in the narrowband single-user setting, is

y=HRIS-RxH Φ Gf v⏟heff(Ο•,v) s+w,y = \underbrace{\mathbf{H}_{\text{RIS-Rx}}^H\, \boldsymbol{\Phi}\, \mathbf{G}_f\, \mathbf{v}}_{h_{\text{eff}}(\boldsymbol{\phi}, \mathbf{v})} \, s + \mathbf{w},

where Gf∈CNRISΓ—Na\mathbf{G}_f \in \mathbb{C}^{N_{\text{RIS}} \times N_a} is the short-range (reactive/near-field) coupling matrix from the active feed to the RIS, Ξ¦\boldsymbol{\Phi} is the diagonal RIS reflection, and HRIS-RxH∈C1Γ—NRIS\mathbf{H}_{\text{RIS-Rx}}^H \in \mathbb{C}^{1 \times N_{\text{RIS}}} is the long-range reflected channel to the user. The Tx-side precoding v∈CNa\mathbf{v} \in \mathbb{C}^{N_a} lives on the NaN_a-dimensional active feed; the RIS phase profile Ο•\boldsymbol{\phi} adds a further NRISN_{\text{RIS}} scalar degrees of freedom.

The key physical insight is that Gf\mathbf{G}_f is well-conditioned β€” essentially a lossless reactive-field transformer between the two apertures β€” so the effective single-hop path loss is set entirely by βˆ₯HRIS-Rxβˆ₯2\|\mathbf{H}_{\text{RIS-Rx}}\|^2, not by a product.

The architecture is often called a lens array in the antenna community: the passive surface acts as an RF lens focusing the active feed's pattern into a much larger effective aperture. The terminology "array-fed RIS" reflects its system-level framing β€” a standard hybrid architecture in which the analog stage happens to be a metasurface rather than a phase- shifter network.

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πŸŽ“CommIT Contribution(2022)

Power- and Hardware-Efficient Multiuser Multibeam Array-Fed RIS

G. Caire β€” CommIT group, technical report / IEEE Trans. Wireless Communications (preprint)

The array-fed RIS architecture developed by Caire and collaborators at the CommIT group reframes the RIS as an analog aperture stage of a hybrid architecture rather than as a stand-alone repeater. The central technical contributions, each of which is used somewhere in this chapter, are:

  1. Co-located feed + RIS geometry. Place an NaN_a-element active array at df∼5Ξ»d_f \sim 5\lambda from an NRISN_{\text{RIS}}-element passive RIS so that the forward link Gf\mathbf{G}_f is in the reactive near field. This eliminates the first path-loss factor and preserves the NRISN_{\text{RIS}} aperture gain of the reflected link. The result is an effective transmit aperture of NRISN_{\text{RIS}} elements with only NaN_a RF chains β€” a cost reduction of roughly NRIS/NaN_{\text{RIS}}/N_a compared with a fully digital array of equal size.

  2. Multiuser joint precoder design. The joint optimization of the active-array precoder W∈CNaΓ—K\mathbf{W} \in \mathbb{C}^{N_a \times K} and the RIS phase profile Ο•\boldsymbol{\phi} is non-convex, but admits a computationally tractable alternating solution that we derive in Section 21.4. Unlike fully hybrid architectures, the RIS stage can synthesize KK simultaneous beams even when Na<KN_a < K, provided NRISN_{\text{RIS}} is large.

  3. Eigenmode analysis of the cascaded channel. The effective channel Heff\mathbf{H}_{\text{eff}} has rank at most min⁑(Nr,Na)\min(N_r, N_a) regardless of NRISN_{\text{RIS}}, but its dominant singular values scale with NRISN_{\text{RIS}}, so the array gain is concentrated on a small number of high-quality eigenmodes. We derive this in Section 21.3.

  4. Power and rate comparison with fully digital arrays. Caire and collaborators quantified the rate–power tradeoff: the array-fed RIS architecture typically achieves 75–85% of the sum rate of a fully digital array of equal physical aperture at 1/5 to 1/10 of the DC power β€” a factor set essentially by the Na/NRISN_a/N_{\text{RIS}} ratio. Section 21.5 reproduces this comparison.

The architecture is particularly attractive for mmWave and sub-THz deployments, where even a modest RIS aperture (0.30.3–11 m) holds thousands of elements and where active-chain DC power dominates the equipment budget. In these bands, the array-fed RIS is plausibly the most power-efficient way to scale the transmit aperture.

rismmwavehybrid-beamformingmultiuserarray-fed

Array-fed RIS

A reflective transmitter architecture in which a small active array of NaN_a RF-chain-backed elements illuminates a large passive RIS of NRIS≫NaN_{\text{RIS}} \gg N_a elements at near-zero distance (within a few wavelengths). The active feed delivers transmit power locally; the RIS provides aperture gain. The architecture eliminates the double-fading loss of stand-alone passive RIS while keeping the RF-chain count proportional to the user count rather than the aperture size. Synonym: metasurface-fed antenna, lens-array antenna.

Related: Array-Fed RIS Architecture, Hybrid Analog-Digital Beamforming, Double-Fading Path Loss

Double fading

The compounded path loss of a reflective link, in which a signal travels through two free-space hops d1d_1 (Tx β†’\to RIS) and d2d_2 (RIS β†’\to Rx). The total received power decays as 1/(d1d2)21/(d_1 d_2)^2 rather than the single-hop 1/ddirect21/d_{\text{direct}}^2, which dominates when both hops are non-trivial. The phenomenon is the central obstacle to passive-RIS deployments and the motivation for the array-fed architecture.

Related: Array-Fed RIS Architecture, Array-Fed RIS Architecture, Path Loss

Array-Fed RIS Block Diagram

Array-Fed RIS Block Diagram
Block diagram of an array-fed RIS transmitter. Digital precoding W\mathbf{W} maps KK user streams onto NaN_a RF chains; the active array illuminates the passive RIS through a short-range near-field coupling Gf\mathbf{G}_f; the RIS phase profile Ο•\boldsymbol{\phi} reshapes the illumination into KK simultaneous beams steered toward the users. The double-fading path loss is avoided because the Tx-to-RIS distance dfd_f is only a few wavelengths.

Passive RIS vs Array-Fed RIS vs Fully Digital Array

PropertyPassive RISArray-Fed RISFully Digital Array
RF chains needed0NaN_a (small)NRISN_{\text{RIS}} (large)
Transmit power sourceExternal Tx at d1d_1Local feed NaN_aLocal feed NRISN_{\text{RIS}}
Path-loss factors1/(d1d2)21/(d_1 d_2)^21/d221/d_2^21/d221/d_2^2
Effective apertureβ‰ˆNRIS\approx N_{\text{RIS}}β‰ˆNRIS\approx N_{\text{RIS}}β‰ˆNRIS\approx N_{\text{RIS}}
DC power budget∼\sim mW (control only)Naβ‹…PcRFN_a\cdot P_c^{\text{RF}}NRISβ‹…PcRFN_{\text{RIS}}\cdot P_c^{\text{RF}}
Multiuser flexibilitySingle-beam (joint with Tx)min⁑(Na,NRIS)\min(N_a, N_{\text{RIS}}) beamsUp to NRISN_{\text{RIS}} beams
Per-user CSI neededCascaded Heff\mathbf{H}_{\text{eff}}Cascaded Heff\mathbf{H}_{\text{eff}}Direct H\mathbf{H}
Phase resolution mattersYes (critical)Less (dominated by W\mathbf{W})N/A
Best forBlocked-direct coverage holesLarge-aperture mmWave accessSub-6 GHz massive MIMO

Example: A 1024-Element Array-Fed RIS vs 256-Element Digital Array

We want to deploy a mmWave base station at f0=28f_0 = 28 GHz with a 0.3Γ—0.30.3 \times 0.3 m aperture (NRIS=1024N_{\text{RIS}} = 1024 at half-wavelength spacing). Option A is a fully digital 1024-element array. Option B is an array-fed RIS with Na=32N_a = 32 active elements feeding the 1024-element passive surface. Each active RF chain costs PcRF=250P_c^{\text{RF}} = 250 mW. Compare the DC power of the two options (ignore baseband, cooling).

Reflected Beam Pattern as the RIS Phase Profile Varies

Fix the active feed in a co-located array-fed RIS configuration and steer the outgoing beam by changing only the RIS phase profile. The angular pattern is computed analytically from the array manifold of a ULA RIS illuminated by a single-mode feed. Adjust the steering angle and the element count to see how beamwidth scales as 1/NRIS1/N_{\text{RIS}}.

Parameters
256
20
8

Array-Fed RIS Forward Signal Synthesis

Complexity: O(NRIS Na+K NRIS)\mathcal{O}(N_{\text{RIS}}\, N_a + K\, N_{\text{RIS}})
Input: Active precoder W∈CNaΓ—K\mathbf{W} \in \mathbb{C}^{N_a \times K},
RIS phase profile Ο•βˆˆ[0,2Ο€)NRIS\boldsymbol{\phi} \in [0,2\pi)^{N_{\text{RIS}}},
user symbols s∈CK\mathbf{s} \in \mathbb{C}^{K}, feed–RIS coupling
Gf\mathbf{G}_f
Output: Transmitted field pattern at the RIS, and per-user received signal
1. xa←W s\mathbf{x}_a \leftarrow \mathbf{W}\, \mathbf{s} // baseband signal on the active array
2. u←Gf xa\mathbf{u} \leftarrow \mathbf{G}_f\, \mathbf{x}_a // captured by the RIS
3. Φ←diag(ejΟ•1,…,ejΟ•NRIS)\boldsymbol{\Phi} \leftarrow \text{diag}(e^{j\phi_1}, \ldots, e^{j\phi_{N_{\text{RIS}}}})
4. z←Φ u\mathbf{z} \leftarrow \boldsymbol{\Phi}\, \mathbf{u} // reflected field on the RIS
5. for user k=1,…,Kk = 1, \ldots, K do
6. yk←HRIS-Rx,kH z+wk\quad y_k \leftarrow \mathbf{H}_{\text{RIS-Rx},k}^H\, \mathbf{z} + w_k
7. end for

The cost of the forward pass is dominated by the NRIS NaN_{\text{RIS}}\, N_a matrix-vector product Gfxa\mathbf{G}_f \mathbf{x}_a β€” feasible in real-time because NaN_a is small by construction.

Common Mistake: Counting the Array Gain Twice

Mistake:

A natural but wrong reading of the array-fed RIS link budget is that the user enjoys the product Naβ‹…NRISN_a \cdot N_{\text{RIS}} of the two stages' array gains. Students then conclude that a 3232-element feed and a 10241024-element RIS deliver NaNRIS=32,768N_a N_{\text{RIS}} = 32{,}768 of effective aperture gain.

Correction:

The reactive-near-field coupler Gf\mathbf{G}_f is an aperture-matching transformation, not a propagation stage. Nearly all of the active power flows into the RIS regardless of NaN_a, so the active-feed directivity GaG_a only sets how the power is distributed across modes on the RIS, not how much power is captured. The effective transmit array gain is therefore approximately GRISβ‰ˆNRISG_{\text{RIS}} \approx N_{\text{RIS}} alone, with the small correction from GaG_a reflecting mode coupling efficiency. The 32,76832{,}768 figure overcounts by a factor of NaN_a.