The Array-Fed RIS Architecture

Why mmWave Demands Array-Fed RIS

Conventional RIS deployments at mmWave face a hard trilemma: (1) the product path loss d12d22d_1^2 d_2^2 is brutal at 2828-140140 GHz, (2) active BS arrays need to be huge (Nt64N_t \geq 64) to close the link budget, and (3) digital beamforming at large NtN_t over GHz of bandwidth is prohibitive in power and cost. The conventional answer is hybrid analog-digital beamforming (MIMO Ch. 20–21) — but even that requires tight coordination between many RF chains.

The array-fed RIS takes a radically different approach: use a small active array (Nt8N_t \sim 8-3232) that is very close to a large passive RIS (N256N \sim 256-40964096). The active array provides the baseband complexity (few RF chains, conventional digital precoding); the RIS provides the aperture gain (large physical area, passive). They combine to deliver massive-MIMO-like performance at 1010-20%20\% of the hardware cost. This is the CommIT Group's (Caire et al.) flagship architecture for 6G mmWave.

The golden thread: the RIS programs the propagation, but now its programmability is jointly designed with an active precoder that the RIS sees in the near field.

Array-Fed RIS

An architecture combining a small active antenna array with a large passive RIS panel placed in the array's near field. The active array provides digital baseband flexibility via few RF chains; the RIS provides aperture gain. The near-field BS-RIS channel is full-rank, enabling multi-user multiplexing through one passive surface.

Related: Near Field, Eigenmode Decomposition of H1\mathbf{H}_1

RIS Eigenmode

A singular-vector pair (uk,vk)(\mathbf{u}_k, \mathbf{v}_k) of the BS-RIS channel H1\mathbf{H}_1. The active array excites the kk-th eigenmode via vk\mathbf{v}_k; the RIS then receives an excitation uk\mathbf{u}_k that can be focused toward user kk. Independent eigenmodes enable multi-user multiplexing in array-fed RIS.

Related: Array-Fed RIS Architecture, Svd

Definition:

Array-Fed RIS Architecture

An array-fed RIS consists of:

  • A small active array of NtN_t antennas at the BS.
  • A large passive RIS of NNtN \gg N_t elements.
  • A short array-RIS distance dARd_{\text{AR}} such that the RIS is in the near-field of the array (i.e., dAR<dFAR=2DA2/λd_{\text{AR}} < d_F^{\text{AR}} = 2 D_A^2 / \lambda, where DAD_A is the active-array aperture).

The BS-to-RIS channel H1CN×Nt\mathbf{H}_1 \in \mathbb{C}^{N \times N_t} is a near-field channel, with rank governed by the near-field eigenmodes (not just the angular spread). Then H2CNr×N\mathbf{H}_2 \in \mathbb{C}^{N_r \times N} is the (typically far-field) RIS-to-UE channel.

The system model is identical to Chapter 3's cascaded channel: y=(Hd+H2ΦH1)Ws+w\mathbf{y} = (\mathbf{H}_d + \mathbf{H}_2 \boldsymbol{\Phi} \mathbf{H}_1)\mathbf{W}\mathbf{s} + \mathbf{w}, but the near-field structure of H1\mathbf{H}_1 is the new engineering variable.

,

Theorem: Near-Field Eigenmode Rank of H1\mathbf{H}_1

For an array-fed configuration with active-array aperture DAD_A, RIS aperture DRD_R, array-RIS distance dARd_{\text{AR}}, and wavelength λ\lambda:

  • Far-field regime (dARdFAR=2max(DA,DR)2/λd_{\text{AR}} \gg d_F^{\text{AR}} = 2\,\max(D_A, D_R)^2 / \lambda): rank(H1)L\text{rank}(\mathbf{H}_1) \sim L where LL is the number of scattering paths (typically 1-3 in mmWave LoS).
  • Near-field regime (dARdFARd_{\text{AR}} \ll d_F^{\text{AR}}): rank(H1)min(Nt,Neff)\text{rank}(\mathbf{H}_1) \approx \min(N_t, N_{\text{eff}}), where Neff(DADR)/(dARλ)N_{\text{eff}} \sim (D_A \cdot D_R) / (d_{\text{AR}} \lambda) is the near-field "number of degrees of freedom."

In the array-fed RIS, we deliberately place the array in the near-field of the RIS: dARd_{\text{AR}} \sim a few λ\lambda. The rank becomes approximately min(Nt,N)\min(N_t, N) — full rank in NtN_t.

In the far-field, a BS antenna "sees" the RIS as a single direction: H1\mathbf{H}_1 has rank 1\sim 1 per LoS path. In the near-field, each active-array element has a slightly different path length and angle to each RIS element, giving a full-rank H1\mathbf{H}_1 of rank min(Nt,N)\min(N_t, N) under sufficient aperture geometry. Near-field gives us many eigenmodes; far-field gives us few.

Array-Fed RIS Architecture Diagram

Array-Fed RIS Architecture Diagram
A small active array of Nt=8N_t = 8 antennas mounted a few λ\lambda in front of a large passive RIS with N=512N = 512 elements. The array illuminates the RIS with near-field beams; the RIS reflects toward distant UEs with far-field coherent gain. Result: Nt\sim N_t independent streams, each with N\sim N aperture gain — hybrid-beamforming-like performance at a fraction of the cost.

Array-Fed RIS vs. Conventional Alternatives

Three architectural alternatives at mmWave:

  1. Large fully-digital array (Nt=256N_t = 256, NRF=256N_{\text{RF}} = 256): best performance, prohibitive cost (256\sim 256 high-power ADCs at >20> 20 GHz).
  2. Hybrid analog-digital (Nt=256N_t = 256, NRF=8N_{\text{RF}} = 8): trades performance for cost. 3\sim 3-55 dB below fully-digital.
  3. Array-fed RIS (Nt=8N_t = 8 active + N=512N = 512 passive): trades both for hardware simplicity. Active array is conventional digital; RIS is near-field passive. Close to hybrid performance.

The array-fed RIS is the cost-effective third option. Its advantage grows as frequency increases (mmWave → sub-THz): active arrays become exponentially expensive, while passive RIS stays cheap per element.

Array-Fed RIS vs. Massive MIMO vs. Hybrid BF

Compare the sum-rate achievable by three architectures at matched cost: large fully-digital, hybrid analog-digital, and array-fed RIS. Vary the BS-UE distance; see how array-fed RIS dominates at mmWave/sub-THz where path loss is severe.

Parameters
8
512
28
100

Key Takeaway

Array-fed RIS: small active, large passive, near-field coupling. The active array provides digital-processing flexibility and multi-stream capability; the passive RIS provides aperture gain and physical coverage. They combine to approach massive-MIMO performance at 1010-20%20\% of the hardware cost — the key architectural argument for mmWave / sub-THz 6G.

⚠️Engineering Note

Array-Fed RIS Deployment

Practical array-fed RIS deployment:

  1. Physical form: active array and passive RIS mounted on the same or adjacent structures, with dARd_{\text{AR}} \sim few λ\lambda (e.g., 55-3030 cm at 28 GHz, 22-1010 cm at 140 GHz).
  2. Array-RIS alignment: the array must be near-field-centered on the RIS; off-axis alignment degrades the eigenmode structure.
  3. Integration: active array typically mounts on a rooftop; RIS panel on an adjacent wall or building facade; they are connected via a known-phase backhaul.
  4. Control latency: active array uses conventional BBU processing (ns latency). RIS controller uses a few-microsecond latency for phase reconfiguration.
  5. Calibration: the near-field BS-RIS link requires one-time high-accuracy calibration at deployment; subsequent drift is slow (months).
Practical Constraints
  • Typical dARd_{\text{AR}} at 28 GHz: 1010-3030 cm.

  • Total BS + RIS power: active array 10\sim 10-5050 W; RIS 1\sim 1-55 W (passive).

  • RIS panel size: 0.50.5-22 m² at mmWave, smaller at sub-THz.

  • System cost: 5×\sim 5\times less than an equivalent fully-digital array.

Common Mistake: Don't Place the Array in the Far-Field of the RIS

Mistake:

"Put the array far from the RIS for convenience; the geometry doesn't matter too much."

Correction:

Array-fed RIS only works in the near-field configuration. If dAR>dFARd_{\text{AR}} > d_F^{\text{AR}}, the array-RIS channel becomes rank-1 (far-field), and the RIS sees the array as a single effective source — no eigenmode multiplexing. The architecture collapses to a conventional "weak BS + passive RIS" setup, losing all the multi-user multiplexing benefit. Always design dAR<dFAR/5d_{\text{AR}} < d_F^{\text{AR}} / 5 as a rule of thumb, with a safety margin.