Meteor burst channels (MBC) exhibit significant randomness and non-stationarity, limiting the effectiveness of traditional fixed-rate transmission strategies. This paper proposes an adaptive coding and modulation (ACM) scheme based on real-time channel state perception using enhanced Turbo codes. By leveraging the interleaving structure of Turbo codes to mitigate channel fading and incorporating multi-rate adaptation, the scheme dynamically adjusts symbol rate, modulation, and coding methods to improve spectral efficiency. Meanwhile, a joint evaluation mechanism integrating physical-layer signal to noise ratio (SNR) estimation and media access control (MAC)-layer frame error rate (FER) statistics is introduced to achieve dynamic optimization of switching thresholds in multipath channels. Simulation and experimental results demonstrate that the proposed scheme significantly enhances system adaptability to MBC, and increases data transmission success rates, offering a more efficient and reliable solution for MBC systems.
Meteor radars are widely used to study the dynamics of the mesosphere and lower thermosphere, where the accuracy of atmospheric observations depends critically on the quality of meteor echo signals. This study focuses on improving echo signal quality, as meteor trail echoes are transient, low-SNR, and highly susceptible to interference. Four filtering algorithms-wavelet denoising-bilateral filtering (WD-BF), wavelet denoising-guided filtering (WD-GF), extended Kalman-guided filtering (EK-GF), and an improved convolutional neural network (ICNN)-based method are examined through theoretical analysis and numerical simulations. The optimal algorithm is further integrated into the digital acquisition and processing unit of a meteor radar system. The WD-GF method shows superior denoising performance and robustness, yielding an average SNR improvement of 9.3 dB relative to the raw signal. Long-term field observations verify its effectiveness, demonstrating a 15.26 % increase in detected meteors. The proposed WD-GF filtering algorithm significantly improves meteor radar detection capability and measurement accuracy, providing a practical and efficient solution for high-precision, real-time atmospheric observations.
Meteor burst channel demonstrates special fading characteristics, in which the statistics of channel envelope along the time domain explicitly violate the traditional iid (independent and identically distributed) assumption. Because this kind of channel will rapidly disappear after its occurrence. In order to adapt to this particular characteristic of meteor burst channel, a non-iid assumption based Gaussian approximation (GA) algorithm is employed to rebuild the state-of-the-art polarization adjusted convolutional (PAC) code. Then, the polarization effect under non-iid condition is analyzed and an interleaving method is employed to enhance the polarization efficiency. Compared with the widely used low density parity check (LDPC) codes and turbo product codes (TPC), our interleaved PAC codes are capable of decreasing the BLER level by one order of magnitude.
Meteor burst communications (MBC) offers a resilient method for long-range data transfer, whose performance could be enhanced during meteor showers. However, the potential improvements in channel parameters attributable to meteor showers have not been systematically evaluated. This study presents a detailed analysis of key MBC metrics including the spatial distribution, decay time, and interval time of usable meteor trails in the case of Geminids meteor shower in 2024, leveraging the University of Science and Technology of China (USTC) multi-static meteor radar network. By synergistically combining forward-scatter (FS) and backscatter (BS) observations, we overcome the limitations of single-technique studies and can compare the different echoes simultaneously detected in this network. The spatial distribution of usable trails is mapped, showing significant regional variability related to the shower radiant. Compared with sporadic background conditions, the Geminids (GEM) shower increases the mean and median trail decay time ($\tau$) by up to 20% and decreases the mean and median interval (waiting) time by up to 70% (maximum relative changes across the investigated links). This work translates raw meteor observations into practical communications insights, providing a predictive framework for optimizing MBC system scheduling, data throughput, and receiver design during shower periods.
Meteor-burst communication provides low probability of interception and strong resilience to jamming, making it attractive for maritime and terrestrial emergency links. In practice, however, short and rapidly decaying trails prevent conventional modulation and coding schemes (MCS) from exploiting high-SNR opportunities. To address this, we propose a joint adaptation strategy that adjusts transmit power, symbol rate, modulation, and coding within each burst. The threshold-tracking power control and the geometrically quantized symbol rate ladder stabilize the symbol SNR. On top of this, bit-interleaved coded modulation, with adaptive modulation and code-family selection (LDPC for longer trails and Polar for shorter ones), enables higher-order constellations while satisfying block error rate (BLER) targets. Incremental redundancy (IR) coding and IR hybrid automatic repeat request (HARQ) further improve reliability. The joint configuration covers the symbol rate, modulation order, and IR coding, enabling efficient utilization of the channel. The numerical results show consistent gains in average throughput and success probability over baselines, with robustness against fading and short trails.
The meteor burst communication (MBC) system exploits short-lived ionized meteor trails to establish long-distance but intermittent radio links. However, the feasibility of such data transmission strongly depends on meteor trail properties. We utilize observation data from the University of Science and Technology of China (USTC) multistatic meteor radar network to statistically analyze the key parameters of meteor trail echoes. The decay times, waiting time, and signal-to-noise ratio (SNR) are investigated in detail. Results show that most trails are only suitable for instantaneous data transmission, and longer-lived trails occur at lower altitudes. More distant forward-scatter links detect shorter decay times, leading to longer waiting times and higher latency. The SNR statistics further reveal diurnal, seasonal, and spatial patterns consistent with meteor occurrence. These findings offer quantitative guidance for the design and optimization of MBC systems, informing decisions on packet sizing, probing intervals, and rate adaptation based on link geometry.