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6GRIS3GPPMetasurfaceFR3 / mmWave

Reconfigurable Intelligent Surfaces (RIS) for 6G — The Complete Engineering Guide

A programmable wall that bends radio on command. This is the deep, standards-grounded version: the metasurface physics, the cascade channel and its brutal multiplicative path loss, RIS versus the Release‑18 Network‑Controlled Repeater, where 3GPP, ETSI and ITU actually stand, and the engineering problems still in the way.

A RIS turns a dead spot into a covered one — by steering, not amplifying gNB blockage direct path blocked RIS user covered no power amplifier — the surface only re-shapes and reflects the wave it receives

For a century we have treated the radio channel as a fixed, hostile thing we design around. Reconfigurable Intelligent Surfaces (RIS) flip that assumption: they make a slice of the propagation environment itself programmable. A thin panel of hundreds or thousands of tiny tunable elements, bolted to a wall, can take an incoming radio wave and re-aim it — filling a coverage hole, dodging a blockage, or sharpening a beam — using almost no power and no transmit chain. It is one of the defining "smart radio environment" ideas heading into 6G. This guide goes well past the metaphor into the physics, the math, the 3GPP/ETSI/ITU reality, and the problems that still stand between RIS and a real deployment.

What's inside
  1. The smart radio environment
  2. What a RIS actually is
  3. The physics: phase gradients
  4. The cascade channel & double path loss
  5. Near field & beamfocusing
  6. The RIS family (STAR, active, BD)
  7. RIS vs relay vs NCR
  8. 3GPP / ETSI / ITU status
  9. Control architecture
  10. Use cases & deployment
  11. The open challenges
  12. Glossary
  13. FAQ
~0 WRF power radiated by a passive RIS
10²–10⁴tunable elements per panel
1–2 bittypical per-element phase resolution
Rel-21earliest 6G normative window

1 · From a hostile channel to a smart radio environment

Every link budget you have ever built starts from a number you do not control: path loss. The transmitter beams power out, the environment scatters and attenuates it, and the receiver makes do with whatever survives. Beamforming, MIMO and massive MIMO all improved the two endpoints of the link — but the medium in between stayed a given.

The "smart radio environment" thesis is that the medium need not be a given. If we coat selected surfaces — façades, indoor walls, lamp posts — with electronically controllable reflectors, the network gains a third actor it can configure: the channel itself. A RIS is the canonical realisation of that idea. It does not generate a new signal; it edits the one already in the air.

The one-line definition. A RIS is a (near-)passive, software-controlled metasurface that imposes a chosen per-element phase (and sometimes amplitude) shift on an incident radio wave, so the surface as a whole reflects or refracts the wave toward a desired direction — a programmable mirror for radio.

2 · What a RIS actually is

Physically, a RIS is a planar array of unit cells, each much smaller than a wavelength (sub-wavelength spacing, often around λ/2 to λ/5). Each cell is a small patch antenna or resonator backed by a tunable load — a PIN diode, a varactor, or in some designs liquid crystal or MEMS. Changing the bias on that load changes the cell's reflection coefficient, specifically its phase. Do that across the whole grid and you have programmed a phase profile onto the surface.

Crucially, most RIS designs are passive or nearly passive: there is no power amplifier, no mixer, no ADC/DAC, no conventional RF chain on the signal path. The only power the surface draws is the trickle needed to bias the diodes and run a small controller. That is what separates a RIS from every relay and repeater that came before it — and it is also the root of its hardest problem (see §4).

Anatomy: a grid of phase-tunable unit cells incident wave controller sets each cell's phase steered reflection
Each unit cell tunes its reflection phase; collectively they re-aim the reflected wavefront.

3 · The physics — phase gradients and the generalized Snell's law

A flat metal mirror obeys the ordinary law of reflection: angle out equals angle in. A RIS breaks that rule on purpose. By imposing a linear phase gradient across the surface — cell n gets a little more phase delay than cell n−1 — the surface re-radiates a wavefront whose constructive-interference direction is tilted away from the mirror angle. This is the generalized (anomalous) law of reflection: the reflected angle now depends on the phase gradient you program.

// Generalized law of reflection — a phase gradient steers the beam
sin(θr) − sin(θi) = (λ / 2π) · (dΦ/dx)
// θi = incident angle, θr = reflected angle, dΦ/dx = phase gradient across the surface

Because each element's phase is set digitally — and cheap hardware only offers a few states — practical surfaces use quantized phases: a 1-bit cell picks between 0 and π; a 2-bit cell between 0, π/2, π, 3π/2. Coarser quantisation is cheaper and lower-power but loses a few dB of beamforming gain and raises side lobes. The art of RIS control is choosing the discrete phase per element so the reflected beam peaks exactly at the served user.

Plain mirror RIS (phase gradient) θr = θi θr steerable Program the gradient → choose the reflection angle.
Anomalous reflection: the RIS sends energy where you want it, not just where geometry dictates.
Interactive

Steer the beam yourself

Drag the slider to set the target angle. The strip under the surface shows the per-element phase the controller programs (the phase gradient); the beam re-aims live.

incident surface normal θr = +25° per-element phase (0→2π):
+25°
2-bit

Phase quantization — the price of cheap hardware

Real cells cannot take any phase; they pick from a few discrete states. Coarser quantisation is cheaper and lower-power but costs beamforming gain and lifts side lobes. The classic figures:

ResolutionStatesApprox. gain loss vs idealTypical use
1-bit0, π≈ 3.9 dBCheapest panels, coverage fill
2-bit0, π/2, π, 3π/2≈ 0.9 dBThe common sweet spot
3-bit8 phases≈ 0.2 dBHigh-performance / sensing
Continuous0 dB (ideal)Lab reference only

4 · The cascade channel and the multiplicative path-loss problem

Here is the equation that governs every honest RIS link budget. With a direct path hd (often blocked), a transmitter→RIS channel g, a RIS→receiver channel h, and the RIS response as a diagonal matrix Θ = diag(β₁ejφ₁, …, βNeN), the received signal is:

y = ( h Θ g  +  hd ) · x  +  n
// the RIS term is a CASCADE: Tx → RIS → Rx, tuned by Θ

The catch is in that cascade. A passive surface only re-radiates the power that lands on it. So the end-to-end path loss is the product of the two hop losses, not the sum. In the far field it scales roughly as:

PLRIS  ∝  (d₁ · d₂)² / N²    vs. a direct link PL ∝ (d₁+d₂)²

That squared product is the famous multiplicative (or "double") path loss, and it is why early lab demos that looked spectacular at 1–2 m disappoint at tens of metres. The two ways out are visible in the formula: make N (the element count) very large — hundreds to thousands of elements give an array gain that claws back the loss — or place the RIS close to one end of the link (small d₁ or small d₂), which is why RIS panels are best mounted near the gNB or near the served hotspot, not floating in the middle.

Engineer's reality check. A RIS is not a free relay. Because of multiplicative path loss, a mid-span passive RIS often underperforms a much smaller active repeater. RIS wins where it is large, near one endpoint, and replacing a path that would otherwise be fully blocked — not as a general-purpose "signal booster".
Cascade channel: loss multiplies, it doesn't add Tx RIS (N elements) Rx d₁ d₂ end-to-end loss ∝ (d₁·d₂)² / N² → big N, or small d₁ or d₂
The product-distance law is the single most important fact in RIS link design.
Interactive · link budget

Feel the multiplicative path loss

Move the sliders and watch why placement and element count decide everything. Simplified free-space model — directional, not for planning.

1024
20
40
7.0
RIS path loss
penalty vs LoS
N to break even

5 · Near field and beamfocusing

Make a surface big enough to beat path loss and you create a second subtlety. The boundary between "far field" (plane waves, steer by angle) and "near field" (spherical waves, focus on a point) is the Rayleigh distance, 2D²/λ, where D is the aperture size. A multi-metre RIS at mmWave or FR3 can push that boundary tens or hundreds of metres out — so many users sit in the surface's radiative near field.

That is not just a nuisance; it is an opportunity. In the near field a RIS can do beamfocusing — concentrating energy at a specific 3-D location (range and angle), not merely a direction. That sharpens spatial multiplexing and, as we will see, underpins RIS-aided positioning and sensing. It also complicates channel modelling, which is exactly why the 3GPP Release-19 channel-model work (below) matters.

Worked example — when is a user in the near field? Rayleigh distance is dR = 2D²/λ. A 0.5 m surface (D = 0.5 m) at 7 GHz (λ ≈ 4.3 cm) gives dR ≈ 2·0.25/0.043 ≈ 11.6 m; the same panel at 28 GHz (λ ≈ 1.07 cm) gives ≈ 47 m. So at mmWave, most served users sit inside the surface's radiative near field — and beamfocusing, not just beam-steering, is the right mental model.
Live physics · Huygens superposition

Watch the beam form from the elements

Each element re-radiates a wavelet; with the right per-element phases they interfere constructively toward the target. Toggle between steering (far field) and focusing (near field).

Focus
40%

6 · The RIS family — it is not just one device

"RIS" is now an umbrella. The variants differ in what physical quantity each element controls and on which side of the panel energy goes.

VariantWhat it doesTrade-off
Reflective RIS (the classic IRS)Phase-only reflection; users on the same side as the sourceSimplest, fully passive; 180° coverage only
Transmissive / refracting RISPasses & bends the wave through the surface (a programmable lens)Serves the far side; harder to build efficiently
STAR-RIS / IOS (simultaneous transmit & reflect)Splits energy to both sides at once → full 360° servicePer-element amplitude split adds control complexity
Active RISAdds a small per-element amplifier to fight multiplicative lossNeeds power; re-introduces noise & cost (a middle ground to NCR)
Beyond-Diagonal RIS (BD-RIS)Interconnects elements so Θ is no longer diagonal → richer controlHigher gain & flexibility, more wiring & control overhead
Why the diagonal matters. In a classic RIS each element acts alone, so Θ is a diagonal matrix — every element only scales its own incident signal. BD-RIS lets elements exchange energy (off-diagonal terms), trading hardware complexity for noticeably higher beamforming gain and wider steering range.

7 · RIS vs relay vs Network-Controlled Repeater (NCR)

This is the comparison that decides real deployments, because the network-controlled repeater is the option 3GPP has already standardised — and it is RIS's nearest competitor.

Decode-&-forward relayNCR (Rel-18)Passive RIS
Signal treatmentDecodes, regenerates, retransmitsAmplify-and-forward, beam-steeredReflects/re-shapes only
Power / RF chainsHigh; full transceiverModerate; PA + control linkVery low; no PA, no RF chain
Adds noise?No (regenerated)Yes (amplifies noise too)Essentially no
Path-loss behaviourAdditive (two healthy hops)AdditiveMultiplicative (the catch)
Latency addedProcessing delay~Negligible (analog)None (instantaneous)
3GPP statusRel-10 (LTE) onwardStandardised, Rel-18Study candidate (6G)

The Network-Controlled Repeater deserves attention because it is the pragmatic stepping-stone. 3GPP studied it in TR 38.867 and specified it in Release 18. An NCR has two parts: the NCR-MT (mobile-termination), which maintains a control link (the "C-link") to the gNB, and the NCR-Fwd (forwarding) function, which does the amplify-and-forward. Over the C-link the gNB sends side control information — beamforming weights, on/off timing, and TDD uplink/downlink switching — so the repeater is no longer the dumb, always-on booster of the 4G era but a beam-aware node the network actually orchestrates. RF requirements live alongside the NR repeater specifications (TS 38.106 family). In effect, NCR delivers much of the "smart coverage" promise today, with mature hardware, while RIS matures for 6G.

RIS — passive reflect NCR — active forward (Rel-18) reflect · ~0 W · no noise AMP C-link (control) amplify · powered · gNB-steered
The NCR is the standardised "smart repeater" today; the RIS is the (nearly) passive 6G candidate.

8 · Where standardization actually stands

This is where a lot of marketing gets ahead of reality, so let us be precise. As of mid-2026:

Bottom line. RIS today is pre-standard in 3GPP. The honest status is: standardised precursor = NCR (Rel-18); channel-model groundwork = Rel-19 (TR 38.901); first RIS study opportunity = Rel-20; earliest normative 6G = Rel-21. ETSI ISG RIS is where the detailed RIS specs are being written in the meantime.
The road to a standardised RIS Rel-18NCR Rel-19FR3/ISAC ch. model Rel-206G study (RIS?) Rel-21first 6G normative In parallel: ETSI ISG RIS specs · ITU-R IMT-2030 (M.2160) framework
Standardised precursor today (NCR); RIS's first 3GPP window is the Rel-20 6G study.

9 · Control architecture — who tells the surface what to do

A RIS only earns the "intelligent" in its name through control. Each panel has a small RIS controller (an MCU/FPGA) that drives the bias lines that set element phases. Above it sits a control path to the network. Three questions dominate the architecture debate:

The reason 3GPP standardisation is non-trivial is precisely this control plane: the surface needs synchronised, low-latency configuration tied to the gNB's scheduling and beam decisions — and that interface, its signalling, and its timing all have to be specified before multi-vendor RIS becomes real.

A codebook beam-management loop (the pragmatic design)

Rather than estimate the full cascade channel, most realistic proposals mirror NR's P1/P2/P3 beam management with a RIS codebook:

  1. Sweep — the gNB cycles the RIS through a small codebook of pre-stored phase patterns (each a candidate reflected beam), while the UE measures reference signals.
  2. Report & select — the UE reports the best beam (RSRP/SINR); the gNB picks the winning RIS configuration — exactly like CSI-RS/SSB beam reporting.
  3. Refine & track — a finer local codebook hones the beam, and the loop re-runs as blockage or the UE moves, with hysteresis to avoid thrashing.

Codebook control keeps signalling bounded and avoids the impossible task of a passive surface sounding its own channel — at the cost of some optimality versus full channel-state-based optimisation.

10 · Use cases and deployment scenarios

RIS is not a general booster; it is a precision tool. The scenarios where it genuinely shines:

Placement rule of thumb. Mount the surface where one hop is short — on the gNB mast (small d₁) or right at the served hotspot (small d₂) — and size it for the band. That single decision dominates whether a RIS deployment beats its link budget or quietly fails it.

11 · The open challenges — what is really in the way

Stripping away the hype, these are the problems engineers and standards bodies are actually fighting:

The five problems RIS must beat Path loss×, not + Channel est.passive blind Controllatency Deploymentwho owns it Standardsinterfaces
Solve these and RIS graduates from demo to deployment.

The honest takeaway

RIS is one of the most intellectually beautiful ideas in 6G: make the channel programmable and a whole new design dimension opens up — coverage, capacity, sensing, positioning and security all from a passive sheet on a wall. But beauty meets the product-distance law. The near-term truth is that the Network-Controlled Repeater already delivers network-steered coverage today, while RIS earns its place by being large, near an endpoint, and replacing genuinely blocked paths — and by maturing through the Rel-20 6G study, ETSI ISG RIS, and ITU's IMT-2030 framework toward possible normative status in Rel-21. Watch the channel models and the control interface: those, more than any lab gain figure, will decide whether the smart radio environment becomes real.

Quick glossary

RIS / IRS — Reconfigurable Intelligent Surface / Intelligent Reflecting Surface: the (near-)passive programmable metasurface.
Unit cell — one sub-wavelength tunable element; a PIN diode or varactor sets its reflection phase.
Θ (theta) matrix — diagonal matrix of per-element reflection coefficients β·e^{jφ} that defines the surface's response.
Cascade channel — the two-hop Tx→RIS→Rx path; source of multiplicative path loss.
Multiplicative path loss — end-to-end loss scaling as (d₁·d₂)², the central RIS limitation.
NCR — Network-Controlled Repeater; the active, gNB-steered amplify-and-forward node standardised in 3GPP Rel-18.
STAR-RIS / IOS — surface that simultaneously transmits and reflects for full 360° coverage.
BD-RIS — Beyond-Diagonal RIS; interconnected elements give a non-diagonal Θ and higher gain.
Beamfocusing — near-field focusing of energy to a 3-D point (range + angle), not just a direction.
TR 38.901 / 38.867 — 3GPP channel-model report; and the Rel-18 Network-Controlled Repeater study.

Frequently asked questions

What is a reconfigurable intelligent surface (RIS)?

A planar metasurface of many sub-wavelength unit cells whose electromagnetic response is electronically tunable. By setting a per-element phase shift it reshapes an incident radio wave and reflects (or refracts) it toward a chosen direction — with little or no amplification and no conventional RF chains. It is, in effect, a software-controlled mirror for radio.

How is RIS different from a Network-Controlled Repeater (NCR)?

An NCR (3GPP Release 18, study in TR 38.867) is an active amplify-and-forward node whose beams and on/off/TDD behaviour the gNB steers over a control link. A RIS is (nearly) passive — no PA, no RF chain — and only re-shapes the wave it receives. NCR adds gain but also noise and follows additive path loss; RIS adds almost no noise but suffers multiplicative (product-distance) path loss.

Is RIS standardized in 3GPP yet?

Not as normative 5G specs. It was not adopted into Release 19. The first realistic window is the Release 20 6G study phase (2025–2027, non-normative), with normative 6G work expected from Release 21. ETSI ISG RIS is producing RIS specifications today, and Rel-19 added ISAC and 7–24 GHz channel modelling to TR 38.901 that RIS work can reuse.

Why does RIS suffer "double" path loss?

A passive surface only re-radiates the power that lands on it, so the end-to-end loss scales with the product of the two hop distances (≈ (d₁·d₂)² in far field), not their sum. The fixes are a large element count N (for ~N² array gain) or mounting the RIS close to one endpoint.

What is the generalized Snell's law and why does it matter?

It states that a phase gradient across a surface bends the reflected wave away from the ordinary mirror angle. A RIS implements that gradient digitally (often 1-bit or 2-bit per element), so it can perform anomalous reflection and steer energy to a chosen user.

What are STAR-RIS, active RIS and beyond-diagonal RIS?

STAR-RIS (IOS) transmits and reflects at once for full 360° coverage. Active RIS adds small per-element amplifiers to fight multiplicative loss (at the cost of power and noise). Beyond-diagonal RIS interconnects elements so the reflection matrix is no longer purely diagonal, giving richer wave control and higher gain.

Where would an operator actually deploy a RIS?

Where one hop is short and the served path is otherwise blocked: on the gNB mast, on a façade beside a coverage hole, or inside a venue. Placement and panel size — not raw element count alone — decide whether the deployment beats its link budget.

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