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International Conference on Computer and Communications Management (ICCCM)

Parameter-Efficient QCNN-Based Signal Detector for GEO Satellite SISO Communications

Ki-Chang Tong, Yeong-Gyun Jung, MinHyeok Choi, Dong-Woo Seo, Young-Hwan Youn, Hyoung‐Kyu Song

Published Jul 24, 2026• 0 citations
Publisher

Abstract

Signal detection in Geostationary Earth Orbit (GEO) satellite links can be degraded by Rician fading, receiver noise and imperfect channel state information (CSI). This paper investigates a parameter-count-efficient hybrid quantum-classical detector for GEO satellite Single-Input Single-Output (SISO) BPSK links. The objective is to evaluate whether a compact Quantum Convolutional Neural Network (QCNN) feature-processing block can provide CNN-comparable uncoded bit-detection reliability under a controlled imperfect-CSI software-simulation setup, while keeping the trainable model size small. The channel and SNR normalizations are explicitly stated, and the conventional random Line-of-Sight (LOS) phase in the Rician model is addressed through a phase-invariance argument for the proposed channel-compensated features. Four physics-based diagnostic features are extracted from a channel-compensated observation and encoded into a 4-qubit QCNN. The QCNN contains 2,289 trainable parameters, including 48 quantum-circuit parameters and 2,241 classical post-processing parameters, whereas the same-input CNN baseline contains 12,609 trainable parameters. Simulations from − 10 dB to 20 dB show that the QCNN achieves 89.39% average accuracy, compared with 89.74% for the CNN. As a complementary reliability-oriented metric, a capacity-weighted effective-throughput indicator is also evaluated, where the QCNN achieves an average effective throughput of 2.376 bps/Hz, compared with 2.406 bps/Hz for the CNN. These results suggest that the proposed QCNN can provide a favorable balance between detection reliability, effective-throughput behavior and trainable parameter count. This balance is particularly relevant to isolated GEO satellite receiver environments, where onboard memory, model-update opportunities and processing resources are limited after deployment.

DOI
10.1145/3841323.3841329

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Accurate channel estimation is a fundamental requirement for high-performance wireless communication systems, where conventional deep learning approaches often suffer from excessive trainable parameters and high memory cost as antenna and subcarrier dimensions scale up. This paper proposes a quantum machine learning (QML)-based channel estimation framework that addresses this scalability challenge through a compact hybrid quantum-classical architecture. An 8-qubit quantum neural network (QNN) based on a parameterized quantum circuit (PQC) encodes received pilot-domain features using both Cartesian and polar components through Hadamard initialization and rotation-based quantum encoding, and learns channel representations using trainable variational rotations and controlled-Z (CZ) entanglement. The Pauli-Z measurement outputs are then processed by a lightweight classical dense head to produce the final channel estimate. The proposed QNN is compared with a classical deep neural network (DNN) and a QNN without hidden dense layers over a 2 × 1 Rayleigh fading multiple-input single-output (MISO) channel across an SNR range of 10 dB to 30 dB. Simulation results show that the proposed hybrid QNN achieves the lowest normalized mean square error (NMSE) across the entire evaluated SNR range while using only 1,012 trainable parameters, compared with 3,356 for the DNN. At 30 dB SNR, the proposed QNN achieves the lowest NMSE of approximately − 20.24 dB, compared with approximately − 17.54 dB for the DNN baseline. An ablation study further confirms that the dense post-processing head is essential for accurate regression from raw quantum measurement outputs. These results suggest that compact hybrid quantum-classical estimators offer a promising direction for accurate and parameter-efficient channel estimation in next-generation wireless communication systems.
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Recent advances in quantum computing are opening new possibilities for Earth Observation (EO) data analysis. Quantum machine learning (QML) approaches offer novel ways to process information by exploiting quantum phenomena such as superposition and entanglement. These capabilities have motivated the exploration of whether quantum-enhanced models can address long-standing challenges in satellite remote sensing, where complex spectral and spatial signals often require sophisticated feature extraction. Among various fields of application, EO data allow the global monitoring of volcanic clouds and are crucial for aviation safety, hazard assessment, real-time eruption response, and evaluation of volcanic impacts on climate. Yet accurate detection of volcanic clouds remains difficult due to their similarity with meteorological clouds, the variability of eruption signatures, and the coarse spectral sampling of geostationary sensors. In this work, the potential of hybrid quantum convolutional neural networks (QCNNs) for the classification of satellite images containing volcanic clouds was investigated. These architectures integrate quantum computational layers into a classical convolutional framework. Two QCNN variants (with 2 and 4 qubits) have been considered to evaluate their ability to classify a dataset of SEVIRI images, including scenes with volcanic clouds (composed of ash, SO2SO_2SO2​, or mixed components) as well as non-volcanic backgrounds. Finally, the performance of the hybrid QCNN models was compared with that of purely classical architectures.
This study evaluates the use of Quantum Convolutional Neural Networks (QCNNs) for identifying signals resembling Gamma-Ray Bursts (GRBs) within simulated astrophysical datasets in the form of light curves. The task addressed here focuses on distinguishing GRB-like signals from background noise in simulated Cherenkov Telescope Array Observatory (CTAO) data, the next-generation astrophysical observatory for very high-energy gamma-ray science. QCNNs, a quantum counterpart of classical Convolutional Neural Networks (CNNs), leverage quantum principles to process and analyze high-dimensional data efficiently. We implemented a hybrid quantum-classical machine learning technique using the Qiskit framework, with the QCNNs trained on a quantum simulator. Several QCNN architectures were tested, employing different encoding methods such as Data Reuploading and Amplitude encoding. Key findings include that QCNNs achieved accuracy comparable to classical CNNs, often surpassing 90%, while using fewer parameters, potentially leading to more efficient models in terms of computational resources. A benchmark study further examined how hyperparameters like the number of qubits and encoding methods affected performance, with more qubits and advanced encoding methods generally enhancing accuracy but increasing complexity. QCNNs showed robust performance on time-series datasets, successfully detecting GRB signals with high precision. The research is a pioneering effort in applying QCNNs to astrophysics, offering insights into their potential and limitations. This work sets the stage for future investigations to fully realize the advantages of QCNNs in astrophysical data analysis.
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