Skip to main content

mmWave Adaptive Channel Estimation


Algorithm Description

The proposed adaptive beam-training procedure enables the Base Station (BS) and Mobile Station (MS) to jointly identify the optimal transmit–receive beam pair from predefined codebooks. The algorithm operates over multiple stages, where each stage progressively narrows the search space. This hierarchical refinement significantly reduces training overhead compared to exhaustive beam scanning.

1. Initialization

Both BS and MS are assumed to know the total number of angular directions N, the hierarchical resolution parameter K, and the codebooks F (for BS beams) and W (for MS beams).

The initial codebook subset indices are:

k1BS = 1,    k1MS = 1.

The total number of adaptive stages is:

S = logK(N)

ensuring that the search space is reduced by a factor of K in each stage.

2. Stage-wise Beam Training

For each stage s = 1,…,S, both BS and MS test K beam candidates.

2.1 BS Transmission

For each BS beam index mBS = 1,…,K, the BS transmits using the beam:

F(s, ksBS)[:, mBS].

2.2 MS Reception

For each BS beam, the MS cycles through its own beam candidates mMS = 1,…,K, applying:

W(s, ksMS)[:, mMS].

2.3 Measurement Collection

The MS records the received signal corresponding to each transmit–receive beam pair:

ymBS = √Ps · WH · H · F + nmBS.

The MS stores all measurements in:

Y(s) = [y₁, y₂, …, yK].

3. Beam Pair Selection

The strongest beam pair is identified by maximizing the magnitude of the collected measurements:

(m*BS, m*MS) = arg maxmBS, mMS |Y(s) ⊙ Y(s)*|.

This pair represents the best-performing combination in the current stage.

4. Subset Update

The indices of the selected beam subsets for the next stage are updated using:

ks+1BS = K(m*BS − 1) + 1,
ks+1MS = K(m*MS − 1) + 1.

This selects the sub-region of the angular domain containing the strongest path.

5. Final Parameter Estimation

After completing all stages, the estimated angle parameters are:

φ̂ = φ̄kS+1BS,    θ̂ = θ̄kS+1MS.

The corresponding path gain is estimated as:

α̂ = √(ρ/Ps) · G(S)[Y(s)]mMS*, mBS*.


MATLAB Code

% Example Usage:

N = 64;           % Total angles
K = 4;            % Beams per stage
S = log(N)/log(K);

% Build dummy hierarchical codebooks:
for s = 1:S
    for k = 1:N
        F{s, k} = exp(1j * 2*pi*(0:15)' * rand(1,K)); 
        W{s, k} = exp(1j * 2*pi*(0:15)' * rand(1,K));
    end
end

% Example channel
H = randn(16,16) + 1j*randn(16,16);

% Example power allocation
P = ones(S,1);

% Angle grids
phi_grid = linspace(-pi/2, pi/2, N);
theta_grid = linspace(-pi/2, pi/2, N);

% Run algorithm
[phi_hat, theta_hat, alpha_hat] = adaptive_beam_training(F, W, H, N, K, P, phi_grid, theta_grid);

function [phi_hat, theta_hat, alpha_hat] = adaptive_beam_training(F, W, H, N, K, P, phi_grid, theta_grid)

% -----------------------------------------------------------
% Adaptive Beam Training Algorithm
% -----------------------------------------------------------
% Inputs:
%  F          : BS codebook (cell array or 3-D matrix)
%  W          : MS codebook (cell array or 3-D matrix)
%  H          : Channel matrix
%  N          : Total number of angular bins
%  K          : Number of beams per stage
%  P          : Transmit power at each stage
%  phi_grid   : BS angle grid (vector)
%  theta_grid : MS angle grid (vector)
%
% Outputs:
%  phi_hat    : Estimated BS angle
%  theta_hat  : Estimated MS angle
%  alpha_hat  : Estimated path gain
%
% -----------------------------------------------------------

% ---------- Initialization ----------
k_bs = 1;     % BS codebook subset index
k_ms = 1;     % MS codebook subset index
S = log(N) / log(K);   % Number of adaptive stages

% ---------- Adaptive Stages ----------
for s = 1:S
    
    Y = zeros(K, K);  % Storage for received measurements
    
    % Sweep through all K × K beam combinations
    for mBS = 1:K
        
        f_bs = F{s, k_bs}(:, mBS);     % BS beam for stage s
        
        for mMS = 1:K
            
            w_ms = W{s, k_ms}(:, mMS); % MS beam for stage s
            
            % Measurement at MS:
            y = sqrt(P(s)) * (w_ms' * H * f_bs) + (randn + 1j*randn) * 0.01;
            
            Y(mMS, mBS) = abs(y);      % Magnitude for detection
            
        end
    end
    
    % ----- Select strongest beam pair -----
    [~, idx] = max(Y(:));
    [mMS_star, mBS_star] = ind2sub(size(Y), idx);
    
    % ----- Update subset indices -----
    k_bs = K*(mBS_star - 1) + 1;
    k_ms = K*(mMS_star - 1) + 1;

end

% ---------- Final Estimates ----------
phi_hat   = phi_grid(k_bs);
theta_hat = theta_grid(k_ms);

% Estimate gain using last measurement
alpha_hat = Y(mMS_star, mBS_star) / sqrt(P(end));

end


Hierarchical Beam Training Logic

Suppose:

  • N = 64 → total finest-resolution beams
  • K = 4 → number of beams tested per stage

Stage 1 (coarse search)

  • You divide the 64 total beams into 64 / 4 = 16 blocks, each block contains 4 beams.
  • You only test 1 beam per block, so at stage 1 you test K = 4 beams (one from each candidate block).
  • Goal: pick the block containing the strongest beam.

Stage 2 (intermediate search)

  • You now focus on the block selected in stage 1.
  • That block has 4 beams, divide it again into 4 sub-blocks, pick 1 beam per sub-block.
  • You test K = 4 beams in this stage again.
  • Goal: narrow down further.

Stage 3 (fine search)

  • The selected sub-block now contains the final 4 beams.
  • Test these 4 beams, pick the best one.

Key Points

  • At each stage, you only test K beams, not all N beams.
  • The algorithm zooms in progressively.
  • After S = log₄(64) = 3 stages, you have identified 1 beam out of 64.

Stage Summary

Stage Beams tested (K) Candidate beams in block Notes
1 4 64 Coarse search
2 4 16 Focused search
3 4 4 Fine search

At stage 1, you test 4 beams to choose one block of 16 beams.
At stage 2, you test 4 beams to choose one block of 4 beams.
At stage 3, you test 4 beams to pick the final beam.

If desired, a diagram can be drawn to show the 64 → 16 → 4 → 1 zoom-in process visually.


Summary

The algorithm carries out a multi-stage hierarchical search over the BS and MS codebooks. In every stage, it evaluates K × K beam pairs, selects the best combination, and restricts the next stage to a narrower sub-region. After S = logK(N) stages, the optimal beam pair is identified with dramatically reduced training overhead.


Further Reading


People are good at skipping over material they already know!

View Related Topics to







Contact Us

Name

Email *

Message *

Popular Posts

Online Simulator for ASK, FSK, and PSK

Try our new Digital Signal Processing Simulator!   Start Simulator for binary ASK Modulation Message Bits (e.g. 1,0,1,0) Carrier Frequency (Hz) Sampling Frequency (Hz) Run Simulation Simulator for binary FSK Modulation Input Bits (e.g. 1,0,1,0) Freq for '1' (Hz) Freq for '0' (Hz) Sampling Rate (Hz) Visualize FSK Signal Simulator for BPSK Modulation ...

Constellation Diagrams of ASK, PSK, and FSK

📘 Overview of Energy per Bit (Eb / N0) 🧮 Online Simulator for constellation diagrams of ASK, FSK, and PSK 🧮 Theory behind Constellation Diagrams of ASK, FSK, and PSK 🧮 MATLAB Codes for Constellation Diagrams of ASK, FSK, and PSK 📚 Further Reading 📂 Other Topics on Constellation Diagrams of ASK, PSK, and FSK ... 🧮 Simulator for constellation diagrams of m-ary PSK 🧮 Simulator for constellation diagrams of m-ary QAM BASK (Binary ASK) Modulation: Transmits one of two signals: 0 or -√Eb, where Eb​ is the energy per bit. These signals represent binary 0 and 1.    BFSK (Binary FSK) Modulation: Transmits one of two signals: +√Eb​ ( On the y-axis, the phase shift of 90 degrees with respect to the x-axis, which is also termed phase offset ) or √Eb (on x-axis), where Eb​ is the energy per bit. These signals represent binary 0 and 1.  BPSK (Binary PSK) Modulation: Transmits one of two signals...

Power Spectral Density Calculation Using FFT in MATLAB

📘 Overview 🧮 Steps to calculate the PSD of a signal 🧮 MATLAB Codes 📚 Further Reading Power spectral density (PSD) tells us how the power of a signal is distributed across different frequency components, whereas Fourier Magnitude gives you the amplitude (or strength) of each frequency component in the signal. Steps to calculate the PSD of a signal Firstly, calculate the first Fourier transform (FFT) of a signal Then, calculate the Fourier magnitude of the signal The power spectrum is the square of the Fourier magnitude To calculate power spectrum density (PSD), divide the power spectrum by the total number of samples and the frequency resolution. {Frequency resolution = (sampling frequency / total number of samples)} Sampling frequency (fs): The rate at which the continuous-time signal is sampled (in Hz). ...

FFT Magnitude and Phase Spectrum using MATLAB

📘 Overview & Theory 🧮 MATLAB Code 1 🧮 MATLAB Code 2 📚 Further Reading   MATLAB Code  % Developed by SalimWireless.Com clc; clear; close all; % Configuration parameters fs = 10000; % Sampling rate (Hz) t = 0:1/fs:1-1/fs; % Time vector creation % Signal definition x = sin(2 * pi * 100 * t) + cos(2 * pi * 1000 * t); % Calculate the Fourier Transform y = fft(x); z = fftshift(y); % Create frequency vector ly = length(y); f = (-ly/2:ly/2-1) / ly * fs; % Calculate phase while avoiding numerical precision issues tol = 1e-6; % Tolerance threshold for zeroing small values z(abs(z) < tol) = 0; phase = angle(z); % Plot the original Signal figure; subplot(3, 1, 1); plot(t, x, 'b'); xlabel('Time (s)'); ylabel('|y|'); title('Original Messge Signal'); grid on; % Plot the magnitude of the Fourier Transform subplot(3, 1, 2); stem(f, abs(z), 'b'); xlabel('Frequency (Hz)'); ylabel('|y|'); title('Magnitude o...

BER vs SNR for M-ary QAM, M-ary PSK, QPSK, BPSK, ...

📘 Overview of BER and SNR 🧮 Online Simulator for BER calculation of m-ary QAM and m-ary PSK 🧮 MATLAB Code for BER calculation of M-ary QAM, M-ary PSK, QPSK, BPSK, ... 📚 Further Reading 📂 View Other Topics on M-ary QAM, M-ary PSK, QPSK ... 🧮 Online Simulator for Constellation Diagram of m-ary QAM 🧮 Online Simulator for Constellation Diagram of m-ary PSK 🧮 MATLAB Code for BER calculation of ASK, FSK, and PSK 🧮 MATLAB Code for BER calculation of Alamouti Scheme 🧮 Different approaches to calculate BER vs SNR What is Bit Error Rate (BER)? The abbreviation BER stands for Bit Error Rate, which indicates how many corrupted bits are received (after the demodulation process) compared to the total number of bits sent in a communication process. BER = (number of bits received in error) / (total number of tran...

Comparisons among ASK, PSK, and FSK | And the definitions of each

📘 Comparisons among ASK, FSK, and PSK 🧮 Online Simulator for calculating Bandwidth of ASK, FSK, and PSK 🧮 MATLAB Code for BER vs. SNR Analysis of ASK, FSK, and PSK 📚 Further Reading 📂 View Other Topics on Comparisons among ASK, PSK, and FSK ... 🧮 Comparisons of Noise Sensitivity, Bandwidth, Complexity, etc. 🧮 MATLAB Code for Constellation Diagrams of ASK, FSK, and PSK 🧮 Online Simulator for ASK, FSK, and PSK Generation 🧮 Online Simulator for ASK, FSK, and PSK Constellation 🧮 Some Questions and Answers Modulation ASK, FSK & PSK Constellation MATLAB Simulink MATLAB Code Comparisons among ASK, PSK, and FSK    Comparisons among ASK, PSK, and FSK Comparison among ASK, FSK, and PSK Parameters ASK FSK PSK Variable Characteristics Amplitude Frequency ...

Theoretical BER vs SNR for binary ASK, FSK, and PSK

📘 Overview & Theory 🧮 MATLAB Codes 📚 Further Reading Theoretical BER vs SNR for Amplitude Shift Keying (ASK) The theoretical Bit Error Rate (BER) for binary ASK depends on how binary bits are mapped to signal amplitudes. For typical cases: If bits are mapped to 1 and -1, the BER is: BER = Q(√(2 × SNR)) If bits are mapped to 0 and 1, the BER becomes: BER = Q(√(SNR / 2)) Where: Q(x) is the Q-function: Q(x) = 0.5 × erfc(x / √2) SNR : Signal-to-Noise Ratio N₀ : Noise Power Spectral Density Understanding the Q-Function and BER for ASK Bit '0' transmits noise only Bit '1' transmits signal (1 + noise) Receiver decision threshold is 0.5 BER is given by: P b = Q(0.5 / σ) , where σ = √(N₀ / 2) Using SNR = (0.5)² / N₀, we get: BER = Q(√(SNR / 2)) Theoretical BER vs ...

MATLAB Code for Rms Delay Spread

RMS delay spread is crucial when you need to know how much the signal is dispersed in time due to multipath propagation, the spread (variance) around the average. In high-data-rate systems like LTE, 5G, or Wi-Fi, even small time dispersions can cause ISI. RMS delay spread is directly related to the amount of ISI in such systems. RMS Delay Spread [↗] Delay Spread Calculator Enter delays (ns) separated by commas: Enter powers (dB) separated by commas: Calculate   The above calculator Converts Power to Linear Scale: It correctly converts the power values from decibels (dB) to a linear scale. Calculates Mean Delay: It accurately computes the mean excess delay, which is the first moment of the power delay profile. Calculates RMS Delay Spread: It correctly calculates the RMS delay spread, defined as the square root of the second central moment of the power delay profile.   MATLAB Code  clc...