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CGAAN: CFAR-Guided Architecture-Adaptive Network for SAR Target Detection

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06 May 2026

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07 May 2026

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Abstract
Improving robustness across diverse SAR scenes remains a key challenge in deep learning-based SAR target detection. To address this issue, we propose a CFAR-guided architecture-adaptive network (CGAAN), which adjusts its network structure according to dataset complexity. Specifically, dataset complexity is quantified under the CFAR principle by computing the proportion of pixels whose locally adaptive thresholds exceed a predefined global reference, thereby reflecting background clutter and detection difficulty. Based on this indicator, an architecture-adaptive YOLOv8 is constructed with three key components. First, a lightweight representation-enhanced backbone integrating ResNet18 and a dilated convolutional spatial pyramid (DCSP) module is adopted to improve contextual representation while maintaining low model complexity. Second, a structure-adaptive neck (SAN) is further developed to regulate multi-level feature fusion according to dataset complexity. Third, a Complete Intersection over Union (CIoU)-modulated head (CMH) is developed to enhance classification-regression alignment and suppress clutter-induced responses. Experiments on SAR-Aircraft-1.0 and HRSID datasets indicate that deeper feature fusion benefits high-complexity datasets, whereas shallower fusion is sufficient for low-complexity scenarios. Moreover, the proposed CGAAN achieves superior performance over representative detectors, demonstrating its effectiveness and stability on SAR datasets with different scene characteristics.
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1. Introduction

Synthetic aperture radar (SAR) is an active microwave sensor that provides all-day and all-weather imaging capability as well as strong penetration ability. These advantages have enabled its widespread applications in disaster assessment, land-use monitoring, maritime surveillance, and military reconnaissance. Among various SAR image interpretation tasks, target detection plays a fundamental role by automatically localizing and identifying objects of interest, such as aircraft, ships, and vehicles, in SAR imagery [1]. However, due to the coherent imaging mechanism of SAR, the acquired images are inherently affected by multiplicative speckle noise, complex scattering behavior, and heterogeneous background clutter, which significantly reduce the separability between targets and background clutter. These characteristics make SAR target detection still challenging.
Early SAR target-detection methods mainly relied on statistical modeling to characterize the differences between targets and backgrounds. Constant false alarm rate (CFAR) detectors were among the most widely used approaches [2]. CFAR estimated local background statistics and adaptively determined detection thresholds to maintain a constant false alarm probability. Owing to their low computational complexity and clear physical interpretability, CFAR-based methods have been extensively deployed in practical systems. Nevertheless, their performance was fundamentally constrained by assumptions on local clutter distribution. In complex environments such as near-shore, port, or urban areas, clutter heterogeneity and model mismatch degraded detection reliability, limiting the generalization capability of CFAR-based detectors.
In recent years, deep learning-based SAR target detection has gradually become the dominant paradigm. By learning hierarchical nonlinear feature representations end-to-end, deep SAR detectors significantly outperform traditional approaches based on handcrafted features in both representation capability and detection accuracy. From the perspective of detection pipelines, existing methods can be broadly categorized into two-stage detectors [3,4,5] and one-stage detectors [6,7,8,9,10,11]. From an architectural perspective, most high-performance SAR target detection methods are still constructed on convolutional neural networks (CNNs) [12,13,14,15,16,17], benefiting from their strong inductive biases and efficient local feature modeling. More recently, CNN-Transformer hybrid architectures are more commonly adopted, in which CNNs extract multi-scale local features, and Transformers capture long-range dependencies, thereby improving robustness in complex SAR scenes while maintaining computational efficiency [18,19,20].
Despite these advances, the performance of deep SAR detectors remains highly dependent on the compatibility between network architecture and dataset characteristics. In real cases, SAR datasets often exhibit substantial variations in scene complexity, target density, and clutter distribution. As illustrated in Figure 1(a), SAR-Aircraft-1.0 [21] is a fine-grained aircraft detection dataset characterized by complex backgrounds. In contrast, the HRSID dataset [22], shown in Figure 1(b), is dedicated to ship detection without fine-grained classification, and most of the images correspond to offshore scenes with relatively simple backgrounds. Such differences in target granularity and clutter intensity imply that a unified architecture is hard to achieve optimal performance across different datasets. The optimal feature extraction depth and fusion strategy should be varied across datasets with distinct levels of complexity.
To address model adaptability, existing approaches mainly follow two directions. The first seeks to improve cross-domain generalization through domain adaptation or domain generalization techniques [23,24,25,26], which attempt to align feature distributions across different datasets. The second relies on neural architecture search (NAS) to automatically explore optimal structures within predefined search spaces [27]. The first one aims to develop a general-purpose model, whereas the second one focuses on a specialized model. However, these methods exhibit some shortcomings. Domain adaptation typically requires target-domain data, domain generalization requires strict assumptions about category-space alignment, and NAS entails substantial computational overhead and lacks interpretability.
In this work, a data-driven compromise model between general and specialized models is proposed. Inspired by the cell-averaging CFAR (CA-CFAR) principle [28], we first evaluate dataset complexity by computing the proportion of pixels whose local adaptive thresholds exceed a predefined global reference threshold. Then, an architecture-adaptive detection network is constructed based on YOLOv8, which can be adjusted to align model capacity with the characteristics and complexity levels of SAR data. The proposed network keeps the overall framework unchanged across datasets, while the local structures for feature fusion are adaptively determined based on dataset complexity. The primary contributions are summarized as follows:
(1)
A CA-CFAR-based complexity metric is proposed to characterize dataset-level detection difficulty. For each dataset, local adaptive thresholds are estimated using the CA-CFAR detector, and the proportion of thresholds exceeding a predefined global reference threshold is used as a quantitative indicator of background clutter intensity. Based on this indicator, the complexity of different SAR datasets can be objectively compared.
(2)
A lightweight representation-enhanced backbone is designed by integrating ResNet18 and a dilated convolution spatial pyramid (DCSP) module. ResNet18 is adopted for its suitability to SAR datasets with limited training samples. By employing cascaded dilated convolutions with shared parameters, DCSP enlarges the receptive field and strengthens contextual feature modeling while keeping the parameter overhead low.
(3)
A structure-adaptive neck (SAN) is proposed to tailor multi-level feature fusion to dataset complexity. By adaptively adjusting the aggregation depth and cross-scale interactions, SAN facilitates more effective feature fusion across datasets with diverse background-clutter levels.
(4)
A CIoU-modulated head (CMH) is designed to improve classification-regression alignment by reweighting predictions according to localization reliability, thereby emphasizing reliable samples, suppressing clutter-affected unreliable ones, and enhancing prediction consistency.
Experiments on SAR-Aircraft-1.0 and HRSID show that adapting feature-fusion depth to dataset complexity enables CGAAN to achieve superior and stable detection performance under different SAR scene characteristics.

3. Method

3.1. Overall Framework

The overall framework of CGAAN is illustrated in Figure 2. It consists of two sequential stages: dataset complexity assessment and architecture-adaptive detection. In the first stage, a CA-CFAR-based statistical analysis is performed on the training dataset to quantify clutter intensity and detection difficulty. The resulting complexity indicator provides a training-free and interpretable measure of dataset-level background heterogeneity. In the second stage, an architecture-adaptive detection model is constructed upon YOLOv8. According to the estimated dataset complexity, a predefined structural configuration is activated to align model capacity with scene characteristics. The selected architecture comprises three major components: a lightweight representation-enhanced backbone for feature extraction, a SAN for complexity-aware multi-scale feature fusion, and a CMH for reliability-aware classification-regression alignment. The detailed descriptions are presented in the following subsections.

3.2. CA-CFAR-Based Dataset Complexity Assessment

To quantitatively characterize dataset-level detection difficulty, a CA-CFAR-based statistical framework is adopted. Following the classical CA-CFAR detection principle, local background statistics are estimated from reference cells surrounding the cell under test (CUT), and an adaptive threshold is computed to meet a predefined false-alarm probability. Unlike conventional CFAR detection, which performs a binary decision for target presence, the proposed framework further exploits the spatial distribution of adaptive thresholds to assess dataset complexity. By introducing a common global intensity benchmark, the proportion of pixels whose local adaptive thresholds exceed this benchmark is calculated as a dataset complexity indicator. A higher proportion implies stronger background heterogeneity and greater detection difficulty.
Suppose a SAR image has size W×H, where W and H denote the width and height, respectively. For a CUT located at position (w, h) ( 1 w W , 1 h H ), a two-dimensional sliding window is defined and divided into three regions: the CUT, guard cells, and reference cells. The CUT lies at the center of the window. Guard cells form a surrounding region adjacent to the CUT to prevent target leakage into background estimation. Reference cells are located outside the guard region and are assumed to contain pure background clutter.
If the total number of reference pixels is M, the local average clutter power Z is computed as,
Z w , h = 1 M m = 1 M X m
where X m denotes the amplitude value of the m-th (m=1, 2, …, M) reference cell.
Under a predefined false alarm probability P f a , the adaptive threshold for the CUT is calculated as,
T w , h = Z w , h γ
where the scaling factor γ is determined by,
γ = M P f a 1 / M 1 .
From (1)-(3), the adaptive threshold is statistically consistent with the assumed clutter distribution under the constant false alarm rate constraint.
To evaluate dataset complexity, a global reference threshold T g l o b a l is introduced as a unified intensity benchmark. The complexity indicator is defined as the ratio of the number of pixels with T T g l o b a l to the total number of pixels in the dataset. It can be written by,
R a t i o = i = 1 N D w = 1 W h = 1 H I T w , h T g l o b a l W × H × N D
where N D represents the number of images in the dataset, and I is the indicator function.
According to (4), a larger ratio indicates greater clutter intensity and higher background heterogeneity. Based on the estimated complexity indicator, two structural modes are predefined: Mode S (shallow fusion) for low-complexity datasets and Mode D (deep fusion) for high-complexity datasets. This method enables objective and training-free complexity estimation and provides a principled basis for subsequent architecture adaptation.

3.3. Lightweight Representation-Enhanced Backbone

A lightweight backbone integrating ResNet18 with a DCSP module is adopted for feature extraction. ResNet18 is selected for its moderate depth and stable optimization behavior, which are well-suited to SAR datasets with limited training samples. Compared with deeper architectures, it alleviates the risk of overfitting while preserving representation capacity. Besides, the DCSP module, derived from the original spatial pyramid pooling-fast (SPPF) module in YOLOv8, is integrated into the backbone to enhance contextual perception without introducing excessive parameters. Unlike SPPF, which enlarges the receptive field through fixed pooling operations, DCSP employs cascaded dilated convolutions with shared weights to achieve learnable receptive-field expansion.
The detailed structures of DCSP and SPPF are shown in Figure 3(a) and (b), respectively. The DCSP module applies a standard 1×1 convolution to reorganize channel information, followed by three cascaded 3×3 dilated convolution operations with different dilation rates. The intermediate feature maps can be expressed as,
Y 0 = C o n v 1 × 1 X Y 1 = C o n v 3 × 3 d = 1 Y 0 , W s h a r e Y 2 = C o n v 3 × 3 d = 3 Y 1 , W s h a r e Y 3 = C o n v 3 × 3 d = 5 Y 2 , W s h a r e
where X denotes the input feature maps, C o n v represents a convolution operation, d is the dilation rate, and W s h a r e denotes the shared convolution parameters across the cascaded layers.
The final output of DCSP can be expressed by,
Y f i n a l = C o n v 1 × 1 C o n c a t Y 0 , Y 1 , Y 2 , Y 3
where C o n c a t denotes channel-wise concatenation.
The DCSP design provides two primary advantages. First, progressive dilation enlarges the effective receptive field in a learnable, hierarchical manner, which is beneficial for modeling anisotropic scattering patterns and contextual dependencies in SAR imagery. Second, weight sharing across the dilated convolutions reduces parameter redundancy and introduces implicit regularization, encouraging scale-consistent feature learning while maintaining computational efficiency.

3.4. Structure-Adaptive Neck

To align feature aggregation depth with dataset complexity, SAN is designed for feature fusion. In the original YOLOv8, the feature pyramid network and path aggregation network (FPN-PAN) use fixed multi-scale fusion pathways, with feature interaction patterns remaining unchanged regardless of scene characteristics. However, in SAR imagery, the appropriate fusion depth is influenced by factors such as clutter intensity and target scale distribution. Datasets with strong clutter tend to benefit from deeper cross-scale contextual modeling, whereas simpler scenes may favor shallower feature fusion to preserve local discriminative details. This adaptive design helps mitigate over-smoothing.
Inspired by the information flow of bidirectional FPN (BiFPN), SAN introduces a complexity-aware cross-layer fusion mechanism. Instead of using linear weighted summation as in BiFPN, SAN integrates semantic and detail infusion (SDI) [40] and grouped shuffle convolution (GSC) [41] to enhance both feature expression and inter-channel information exchange. The structure of SDI-GSC is shown in Figure 4(a), and the simplified version is shown in Figure 4(b). Before fusion, feature maps from different scales are first transformed into a unified spatial resolution through up-sampling, identity mapping, or down-sampling operations. Suppose that the features to be fused originate from K branches, and the feature map of the k-th (k=1, 2, …, K) branch is denoted as X k . To unify all features to the spatial resolution of the r-th ( 1 r K ) branch, the transformed feature map can be expressed by,
Y k r = D X k k < r I X k k = r U X k k > r
where D represents a down-sampling operation; I represents an identity mapping operation; U represents an up-sampling operation.
After scale unification, GSC is employed to enhance inter-channel interaction, and the detailed structure is shown in Figure 4(c). It combines standard convolution and depth-wise convolution to generate both intrinsic and ghost features at low computational cost, followed by a channel shuffle operation to further enhance cross-channel information exchange. This design improves parameter efficiency while preserving strong representation capability.
Given the input Y k r , the output of GSC is,
F k r = S h u f f l e C o n c a t C o n v Y k r , D W C o n v C o n v Y k r
where C o n v represents standard convolution; D W C o n v represents depth-wise convolution; S h u f f l e represents the channel shuffling operation.
Through the joint operation of SDI and GSC, the fusion block achieves scale alignment across heterogeneous feature resolutions, semantic-detail complementarity between deep and shallow representations, and efficient channel interaction under lightweight constraints.
Finally, the enhanced feature maps of all S branches are fused by the Hadamard multiplication, and the final r-th scale output feature maps can be expressed by,
F r = F 1 r F 2 r F K r
where denotes the Hadamard product.
Compared with additive fusion, multiplicative interaction reinforces mutually consistent activations across scales while suppressing inconsistent responses, thereby mitigating clutter-induced false alarms in SAR imagery.
Despite sharing the same SDI-GSC fusion principle, the two structural modes (Mode S and Mode D) adopt different fusion pathways. Under Mode S, shallow feature interaction is emphasized to preserve fine-grained details and reduce over-smoothing. Under Mode D, deeper cross-scale aggregation paths are activated to enhance contextual reasoning and suppress clutter interference. The detailed structures of these two modes are shown in Figure 5(a) and (b). In Figure 5(a), Mode S adopts SDI-GSC1/2/3 configurations for relatively shallow fusion, while Mode D adopts SDI-GSC4/5/6 configurations for deeper and denser cross-scale interaction. The simplified structures of configurations are shown in Figure 5(c)-(h), respectively.

3.5. CIoU-Modulated Head

YOLOv8 adopts an anchor-free detection paradigm, in which each spatial prediction location on the feature map directly outputs classification scores and bounding box regression parameters. In its detection head, a task-aligned learning (TAL) mechanism is employed to couple classification confidence with localization accuracy. Specifically, an alignment metric—typically formulated as the product of classification probability and complete intersection over union (CIoU) —is used to jointly represent category confidence and regression quality. However, in SAR target detection, targets such as aircraft and ships are frequently embedded in strong and heterogeneous background clutter. This clutter seriously perturbs the CIoU calculation of predicted bounding boxes, leading to compressed CIoU distributions and reduced separability between high-quality and low-quality predictions. As a result, the alignment metric becomes less discriminative, weakening the reliability of positive sample selection.
To mitigate this issue, a CMH is proposed, as illustrated in Figure 2. The core idea is to reshape the CIoU distribution before task-aligned computation by amplifying reliable predictions and suppressing clutter-induced unreliable ones. By incorporating this CIoU modulation into the TAL module, the dynamic range of localization quality is enlarged, thereby improving the robustness of alignment-based sample assignment. Let the batch size be B, the number of ground-truth targets in each image be J, and the total number of prediction locations be N. For the n-th prediction location (n=1, 2, …, N) in the b-th (b=1, 2, …, B) image, the classification head outputs a raw score S b n r a w , and the regression head predicts location distributions D b n p r e d . After applying the sigmoid function, the classification probability is obtained as S b n p r o b . The regression outputs are decoded into predicted bounding boxes B b n p r e d .
For the j-th (j=1, 2, …, J) ground-truth box B b j g t in the b-th image, the CIoU between B b n p r e d and B b j g t is computed as,
I b j n = CIoU B b n P r e d , B b j g t
During the task alignment, the CIoU is nonlinearly modulated to expand the separability between reliable and unreliable predictions,
I b j n = I b j n 1 / P o w e r I b j n I 0 I b j n P o w e r 2 I b j n < I 0
where I 0 represents the threshold, and P o w e r = 2 .
This modulation increases the contrast between high-CIoU and low-CIoU samples. High-quality predictions receive amplified supervision signals, whereas clutter-induced low-overlap predictions are suppressed. From an optimization perspective, this reshaping redistributes gradient contributions toward reliable candidates.
The probability that the n-th prediction location belongs to the category of the j-th ground truth target is defined as,
S b j n = S b n L b j p r o b
where L b j represents the category label of the j-th ground-truth box in the b-th image.
The alignment metric is computed by jointly considering classification probability and modulated CIoU,
A b j n = S b j n α × I b j n β
where α = 1 and β = 6 .
For each ground-truth target, only prediction locations with high alignment scores are retained as candidate positive samples, thereby improving computational efficiency while restricting supervision to geometrically plausible locations. Specifically, for the j-th ground-truth target, select the top K predictions ranked by A b j n as candidate samples by using the mask M b j n t o p K . Additionally, spatial constraints are enforced so that only predictions located inside the ground-truth box are retained via mask M b j n i n .
The positive sample mask of the j-th ground-truth target is defined as,
M b j n p o s , i n i t i a l = M b j n t o p K × M b j n i n .
To avoid assigning multiple targets to the same prediction location, conflict resolution is performed. For the n-th prediction location, if it is assigned to multiple ground-truth targets, only the one with the maximum CIoU is retained,
M b j n p o s = 1 i f   j = argmax j J b n i n i t i a l I b j n 0 o t h e r w i s e
where J b n i n i t i a l = j M b j n p o s , i n i t i a l = 1 represents an index set of ground-truth targets assigned to the n-th prediction location in the b-th image.
The alignment metric is then filtered using the final mask M b j n p o s ,
A b j n f i l t e r e d = A b j n × M b j n p o s .
To stabilize training by preventing domination from extreme alignment values, the relative quality score of the n-th prediction location for the j-th ground-truth target is defined as,
Q b j n = A b j n f i l t e r e d × I b j max A b j max
where A b j max and I b j max can be calculated by,
A b j max = max n A b j n f i l t e r e d I b j max = max n I b j n × M b j n p o s .
For each prediction location n in the b-th image, the final quality weight is determined by taking the maximum relative quality score across all ground-truth targets assigned to the location,
W b n = max j Q b j n .

3.6. Loss Function

In the anchor-free YOLOv8 framework, each prediction location outputs classification scores and bounding box regression distributions. Therefore, ground-truth labels must be reformulated into target representations aligned with prediction locations.
For each prediction location n in the b-th image selected as positive samples after task-aligned selection, the corresponding target category label and bounding box are assigned as,
L b n t a r g e t = L b , J b n g t B b n t a r g e t = B b , J b n g t
where J b n = j M b j n p o s = 1 .
Classification Loss: Instead of using a hard binary label, the soft-weighting mechanism allows high-quality positive samples to contribute more to optimization. The soft category label is obtained by weighting the target category label with the final quality weight from task alignment, which can be expressed as,
L b n = L b n t a r g e t × W b n .
With this soft label, the classification loss is formulated using binary cross-entropy:
L c l s = b = 1 B n = 1 N L b n log S b n p r e d + 1 L b n log 1 S b n p r e d b = 1 B n = 1 N W b n .
Regression Loss: Let f g = b , n j   s . t .   M b j n p o s = 1 denote the set of prediction locations assigned to at least one ground-truth box. The regression loss can be written as,
L r e g = b , n f g W b n 1 CIoU B b n pred , B b n target b = 1 B n = 1 N W b n .
Distribution Focal Loss (DFL): YOLOv8 adopts DFL to model bounding box offsets as discrete probability distributions. For the l-th coordinate at prediction location n (where l l e f t , t o p , r i g h t , b o t t o m indexes the box edge), the predicted distribution d t b n l is converted to a probability distribution via softmax,
p t b n l = exp d t b n l t = 0 R e g m a x 1 exp d t b n l , t = 0 , 1 , ... , R e g m a x 1
where R e g m a x is the maximum regression bin index.
For the target distribution y b n l encoded from B b n t a r g e t , the left and right bin indices and the corresponding interpolation weights are defined as,
t l e f t = y b n l t r i g h t = t l e f t + 1 W l e f t = t r i g h t y b n l W r i g h t = 1 W l e f t
where represents the floor operation.
The DFL loss is computed as,
L d f l = b , n f g W b n l = 1 4 L d f l 0 p b n l , y b n l b = 1 B n = 1 N W b n
where
L d f l 0 p b n l , y b n l = W l e f t log p t l e f t + W r i g h t log p t r i g h t .
Finally, the total loss can be expressed by,
L t o t a l = λ c l s L c l s + λ r e g L r e g + λ d f l L d f l
where λ c l s , λ r e g , and λ d f l are balancing coefficients.
It is worth noting that the proposed CIoU modulation influences both sample assignment and quality weight, thereby implicitly affecting the optimization of classification, regression, and DFL losses, as reflected in (22), (23), and (26), respectively.

4. Experiments

4.1. Datasets

Experiments are conducted on two representative SAR datasets with distinct complexity characteristics, i.e, SAR-Aircraft-1.0 and HRSID.
SAR-AIRcraft-1.0 consists of 4,368 SAR images acquired by the GaoFen-3 satellite [21], containing 16,463 aircraft instances across seven fine-grained categories. There are Boeing 737, Boeing 787, A220, A320/321, A330, ARJ21, and other categories. This dataset is characterized by complex airport environments, dense target distribution, strong structural interference from airport facilities, multi-scale aircraft instances, and fine-grained classification requirements. Such characteristics result in strong background clutter and heterogeneous scattering patterns. The dataset is split into training, validation, and test sets with a 7:1:2 proportion.
HRSID contains 5,604 SAR images collected from three satellites, with 16,951 ship instances [22]. Unlike SAR-Aircraft-1.0, it includes only a single ship category without fine-grained subdivision. Ships are distributed in offshore and nearshore scenes, accounting for 81.6% and 18.4%, respectively. Since most targets are located in offshore areas with relatively homogeneous backgrounds, the overall dataset complexity is relatively low. The dataset is split into training, validation, and test sets with an 8:1:1 ratio.

4.2. Experimental Setup and Evaluation Metrics

All experiments are conducted on an NVIDIA GeForce RTX 4080 GPU with 16 GB of memory. The implementation is based on Python 3.10.14, PyTorch 2.2.2, and CUDA 12.1. During training, the batch sizes for SAR-AIRcraft-1.0 and HRSID are set to 8 and 32, respectively, and the initial learning rate is 0.01.
Model performance is evaluated from three perspectives: detection accuracy, model complexity, and computational efficiency [42]. Detection accuracy is assessed using precision (P), recall (R), and COCO-style metrics, including AP50, AP75, and AP50:95. Model complexity is assessed in terms of the number of parameters and floating-point operations (FLOPs). Computational efficiency is measured by the inference speed, reported in frames per second (FPS), measured on a single GPU.

4.3. Dataset Complexity Assessment

To quantitatively evaluate dataset-level complexity, the proposed CA-CFAR-based metric is applied to both SAR-Aircraft-1.0 and HRSID. A constant false alarm probability of 2% is adopted. For each pixel, the average background power Z and local adaptive threshold T are computed according to (1)-(3). A unified global reference threshold T g l o b a l = 6000 is used as an intensity benchmark. The empirical proportion of pixels whose adaptive thresholds exceed T g l o b a l is calculated using (4) and serves as the complexity indicator.
As shown in Figure 6(a) and (b), the complexity indicators for SAR-Aircraft-1.0 and HRSID are 22.3% and 8.2%, respectively. The larger proportion observed in SAR-Aircraft-1.0 indicates stronger background heterogeneity and higher spatial variability of local clutter statistics. In contrast, HRSID exhibits a more homogeneous background distribution at the dataset level. One representative image is randomly selected from each dataset. The pixels with T T g l o b a l are illustrated in Figure 7(a) and (b), respectively. It can be observed that the high-threshold regions in SAR-Aircraft-1.0 are more densely distributed, whereas those in HRSID are relatively sparse. As a result, the deeper Mode D is selected for the aircraft dataset, while the shallower Mode S is selected for the ship dataset.

4.4. Ablation Experiment

Ablation experiments are conducted on both SAR-Aircraft-1.0 and HRSID, with the original YOLOv8 serving as the baseline. To ensure fairness and mitigate the risk of overfitting due to limited SAR training data, ResNet18 is used as the backbone in the baseline, while the original FPN-PAN neck and detection head are retained. Based on this baseline, DCSP, SAN, and CMH are progressively incorporated to evaluate their respective effectiveness and complementary contributions.
Results on SAR-Aircraft-1.0 dataset: The ablation results are presented in Table 1. After introducing DCSP into the backbone, P, R, AP50, AP75, and AP50:95 are increased by 0.4%, 0.5%, 0.7%, 0.2%, and 0.4%, respectively. Meanwhile, the number of parameters shows a slight increase, while the inference speed exhibits a marginal decrease, indicating that DCSP enhances feature representation at a low additional cost. Replacing the original FPN-PAN with SAN improves P, R, AP50, AP75, and AP50:95 by 1.3%, 2%, 1.5%, 0.5%, and 0.3%, respectively. The notable gains in precision, recall, and AP50 suggest more efficient multi-scale feature aggregation and better prediction quality in complex airport scenes. In addition, SAN significantly reduces parameters and FLOPs. Although FPS decreases from 285 to 251, this is mainly due to the additional multi-branch fusion and feature alignment operations, which are less hardware-efficient despite their lower theoretical computational cost. Replacing the original detection head with CMH improves P, R, AP50, AP75, and AP50:95 by 2.9%, 2.1%, 2.6%, 0.8%, and 0.7%, respectively. The larger gains in precision, recall, and AP50 indicate that CMH mainly improves overall prediction quality by enhancing the alignment between classification confidence and localization reliability. Consequently, false alarms and missed detections are reduced, while parameters, FLOPs, and FPS remain nearly unchanged.
For the dual-module settings, DCSP+SAN further improves precision, recall, and AP50:95 over SAN alone, with only slight decreases in AP50 and AP75, indicating a trade-off between stronger feature representation and strict localization accuracy. SAN+CMH achieves clear gains in precision and AP50:95 over SAN alone, demonstrating effective complementarity between feature fusion and reliability-aware prediction modulation. DCSP+CMH yields the most notable gains in recall and AP50 compared with DCSP alone, suggesting improved target coverage and coarse-localization quality. The full model achieves the best performance, with P, R, AP50, AP75, and AP50:95 increased by 3.8%, 3.8%, 2.9%, 1%, and 1.4%, respectively, compared with the baseline. These results demonstrate that DCSP, SAN, and CMH can be effectively integrated to exploit complementary strengths and improve overall detection performance.
Heatmaps for the baseline and the progressively enhanced variants with DCSP, SAN, and CMH are presented in Figure 8(a)-(d), respectively, while the ground truth is given in Figure 8(e). As shown in Figure 8(a), the baseline fails to sufficiently highlight the targets’ weak-scattering components, resulting in incomplete activation across the target regions. After introducing DCSP into the backbone, as shown in Figure 8(b), the activations become more concentrated around the dominant scattering centers, and the response intensity over the true target regions is noticeably enhanced. This improvement can be attributed to the enlarged receptive field and stronger contextual aggregation capability of DCSP. Nevertheless, some parts of the targets still exhibit relatively weak responses. In Figure 8(c), after replacing the original FPN-PAN with SAN, the target regions are well activated, and the overall activation distribution becomes more spatially consistent due to enhanced cross-scale feature interaction and feature alignment. However, a few background regions show weak activations. After further replacing the original detection head with CMH, the heatmap in Figure 8(d) exhibits clearer target focus and sharper response boundaries. In particular, non-target strong scattering regions are significantly suppressed, and the activation responses are better aligned with the ground-truth bounding boxes in Figure 8(e). These observations indicate that the proposed reliability-aware classification-regression alignment effectively mitigates clutter-induced false alarms and improves localization consistency within true target regions.
Results on HRSID dataset: The ablation results are summarized in Table 2. After introducing DCSP into the backbone, the gains in precision and AP50:95 are more pronounced than those observed on the SAR-Aircraft-1.0 dataset. Although recall decreases slightly by 0.1%, this can be regarded as a normal fluctuation. These results suggest that DCSP primarily improves target discrimination rather than recall on this dataset, since ship targets are set against relatively clean backgrounds, making target coverage less challenging. Replacing the original FPN-PAN with SAN yields clear improvements in precision and AP50:95, while recall decreases noticeably. This indicates that SAN effectively suppresses false alarms but tends to produce fewer positive predictions, leading to a more precision-oriented behavior. Replacing the original detection head with CMH yields moderate overall improvements, while AP75 decreases slightly. This indicates that the benefit of CMH in relatively simple scenes is mainly reflected in overall prediction quality rather than further enhancement of high-IoU localization.
For the dual-module settings, DCSP+SAN further improves all evaluation metrics over DCSP alone, demonstrating complementary effects between stronger feature representation and adaptive feature fusion. SAN+CMH improves recall over SAN alone, indicating that CMH can effectively alleviate the conservative prediction tendency introduced by SAN. DCSP+CMH yields a notable improvement in AP75 compared with CMH alone, suggesting that the combination is particularly beneficial for high-quality localization. The complete model yields consistent performance improvements across all evaluation metrics, demonstrating that the three proposed modules effectively complement one another. In addition, after introducing one or more modules, the variation trends of parameters, FLOPs, and FPS remain generally consistent with those on the SAR-Aircraft-1.0 dataset.
Heatmaps for the baseline and for sequentially introducing DCSP, SAN, and CMH to the baseline are presented in Figure 9(a)-(d), respectively; the ground truth is given in Figure 9(e). In Figure 9(a), the phenomena where some target regions fail to be activated, and background clutter is activated, are observed in different image samples. In Figure 9(b), after introducing DCSP, the activation becomes more concentrated around the central target structure. However, some target regions still fail to be activated. In Figure 9(c), after replacing the original FPN-PAN with SAN, all target regions are correctly activated, while some background regions are weakly activated. In Figure 9(d), after further replacing the original detection head with CMH, the target regions are correctly activated, whereas the background clutter is not. Overall, Figure 9 verifies that each proposed component contributes progressively to improved target localization and clutter suppression.

4.5. Hyperparameter Experiment

The modulation threshold I0 in (11) determines the boundary between enhancement and suppression for CIoU values in CMH, and therefore plays an important role in reliability-aware task alignment. The detection results under different values of I0 on SAR-Aircraft-1.0 and HRSID datasets are shown in Table 3 and Table 4, respectively.
For the SAR-Aircraft-1.0 dataset with complex background clutter, the model achieves the best performance when I0 is set to 0.5. By contrast, for the HRSID dataset with relatively simple backgrounds, the optimal performance is obtained when I0 is set to 0.1. Except for minor fluctuations in AP75, the other metrics decrease as I0 increases. This difference in the threshold-parameter experimental results between the two datasets indicates that the optimal modulation threshold is data-dependent. A relatively higher threshold is more suitable for complex and cluttered scenes, where stronger suppression is required to filter unreliable background responses, while a lower threshold is preferable in cleaner scenes to avoid suppressing valid target predictions.

4.6. Comparative Experiment

The effectiveness of the proposed detector is evaluated by comparing it with several state-of-the-art detectors on the SAR-Aircraft-1.0 and HRSID datasets.
Results on the SAR-Aircraft-1.0 dataset: For a fair comparison, all detectors are evaluated using ResNet18 and ResNet50 as backbones, and the results are presented in Table 5. Across both backbone configurations, the proposed CGAAN consistently achieves the best performance among all compared detectors. When using ResNet18, CGAAN outperforms representative anchor-based and anchor-free detectors, including RetinaNet [43], GFL [44], AutoAssign [45], ATSS [46], and FCOS [47]. Compared with more recent advanced detectors, such as RTMDet [48] and YOLOv10 [49], CGAAN consistently improves all evaluation metrics, demonstrating comprehensive performance gains in false-alarm suppression, target coverage, and localization in complex airport scenes. When replacing the backbone with ResNet50, CGAAN still achieves higher recall, AP50, and AP75 than Faster R-CNN [50], Cascade R-CNN [51], RepPoints [52], SKG-Net [53], and SA-Net [21], demonstrating its robustness across different backbone configurations. However, compared with the ResNet18-based setting, the performance decreases. This indicates that a deeper backbone is not more suitable for small-sample SAR datasets.
The detection results of all models using ResNet18 as the backbone are visualized for comparison. Five randomly selected images are used for qualitative comparison, with the results of eight detectors presented in Figure 10(a)-(h). In these figures, green, red, and blue bounding boxes denote correctly detected targets, missed detections, and false alarms, respectively. As shown in Figure 9(a)-(e), early detectors such as RetinaNet, GFL, AutoAssign, ATSS, and FOCS suffer from false alarms and missed detections, and duplicate detections frequently occur. This observation indicates insufficient discrimination between targets and complex background clutter. In Figure 10(f)-(g), corresponding to RTMDet and YOLOv10, the number of missed detections is significantly reduced. However, false alarms remain relatively prominent, suggesting that although these methods improve target coverage, their ability to suppress clutter-induced responses is still limited. In Figure 10(h), the proposed CGAAN further reduces both false alarms and missed detections while alleviating duplicate detections. Moreover, the predicted bounding boxes exhibit better spatial consistency with the ground-truth targets, indicating improved localization accuracy. These observations are consistent with the metrics achieved by CGAAN in Table 5.
Results on the HRSID dataset: The comparison results under the ResNet18 backbone are presented in Table 6. The proposed CGAAN delivers the most favorable performance among all compared detectors. Compared with conventional detectors such as RetinaNet [43], GFL [44], AutoAssign [45], ATSS [46], FCOS [47], DDOD [54], and FoveaBox [55], CGAAN yields consistent improvements across all metrics. It also outperforms recent advanced methods, including RTMDet [48] and YOLOv10 [49], particularly in AP75, indicating better localization quality under stricter evaluation criteria. Although HRSID has a relatively simple background, clear performance differences among detectors still exist. These results suggest the effectiveness and stable performance of the proposed CGAAN in relatively less challenging SAR scenes.
The detection results of RetinaNet, GFL, AutoAssign, ATSS, FCOS, DDOD, FoveaBox, RTMDet, YOLOv10, and the proposed CGAAN, all using ResNet18 as the backbone, are visualized in Figure 11. Three offshore and two nearshore images are selected for comparison. From left to right, the 2nd and 5th columns correspond to offshore images, while the 1st, 3rd, and 4th columns correspond to nearshore images. The color definitions are consistent with Figure 10. As shown in Figure 11(a)-(g), most detectors suffer from false alarms and missed detections. In Figure 11(h)-(i), RTMDet and YOLOv10 significantly reduce missed detections, especially in offshore scenes, while suppressing false alarms to some extent. In Figure 11(j), CGAAN further reduces both missed detections and false alarms across offshore and nearshore scenes. The predicted bounding boxes exhibit better spatial correspondence with the true targets, confirming improved localization consistency. These visual observations are in good agreement with the quantitative results listed in Table 6.

5. Discussion

5.1. Effectiveness of the Adaptive Structure

Effectiveness of the structure-adaptive fusion mode: To further verify the effectiveness of adapting the fusion model structure to the complexity of the dataset, experiments are conducted with both matched and mismatched feature-fusion configurations. Specifically, the shallow fusion mode (Mode S) and the deep fusion mode (Mode D) are applied to both datasets. The results under all settings are summarized in Table 7. When the fusion strategy is consistent with the dataset complexity level, significant improvements are observed in P, R, AP50, AP75, and AP50:95. Therefore, the proposed complexity-driven architecture selection mechanism effectively enhances detection performance.
Effectiveness of each module: The ablation results on two datasets show that DCSP, SAN, and CMH all bring performance improvements to different degrees, and their combination further improves the overall detection performance. This demonstrates the complementarity among the three modules. Specifically, DCSP enhances contextual feature representation, SAN improves multi-scale feature fusion, and CMH strengthens the consistency between classification and localization. Meanwhile, the performance gains are achieved without a clear increase in model complexity. Compared with the baseline, the number of parameters and GFLOPs in the full mode is even reduced. Although FPS decreases to some extent, this is mainly caused by hardware-unfriendly operations, rather than an increase in theoretical computational cost.
Effectiveness of the overall detection framework: The comparison results show that the proposed CGAAN outperforms several representative detectors on both SAR-Aircraft-1.0 with complex airport backgrounds and HRSID with relatively simple ship scenes. This demonstrates the overall detection capability of CGAAN under different SAR scene characteristics. In addition, the visualization results show that CGAAN effectively reduces false alarms, missed detections, and duplicate detections, and produces more accurate bounding boxes, further verifying its practical detection effectiveness.

5.2. Stability of the Adaptive Structure

Stability of performance improvements across datasets: SAR-Aircraft-1.0 contains complex airport backgrounds and fine-grained aircraft targets, whereas HRSID mainly contains ships in relatively simple offshore scenes. Although the two datasets differ significantly in background complexity and scene characteristics, the ablation results show that CGAAN improves P, R, AP50, AP75, and AP50:95 over the baseline on both datasets. This indicates that the proposed detector is not limited to a single target category or scene type, but provides stable performance gains on different datasets.
Stability of complexity and efficiency trends: The number of parameters, GFLOPs, and FPS in the ablation results show generally consistent variation trends on the two datasets. Although the specific GFLOPs and FPS values differ because different fusion depths are adopted by SAN on different datasets, the overall trends remain consistent. This indicates that the proposed structural adaptation is controllable and stable.
Stability of comparison results with different detectors: The comparison results show that CGAAN outperforms representative detectors on both datasets, indicating that its performance advantage is stable rather than being observed only on a single dataset. For SAR-Aircraft-1.0, experiments with different backbone networks further show that CGAAN consistently outperforms other detectors, demonstrating its stability with respect to backbone variations.

6. Conclusions

CGAAN is proposed for SAR target detection across datasets with varying background complexities in this work. First, a CA-CFAR-based complexity metric is introduced to quantify the detection difficulty at the dataset level. Then, guided by the complexity metric, an improved YOLOv8 model is developed to enable adaptive target detection. For the backbone, it is constructed by integrating ResNet18 with a DCSP module, which effectively improves contextual feature modeling while maintaining low computational cost. For the neck, SAN is designed to adjust multi-level feature fusion according to dataset complexity. For the head, CMH is proposed to enhance classification-regression alignment by emphasizing reliable predictions and suppressing clutter-affected ones. Finally, experiments on the SAR-Aircraft-1.0 and HRSID datasets demonstrate the effectiveness and robustness of the proposed CGAAN. Significant improvements are observed on the SAR-Aircraft-1.0 dataset with complex backgrounds, particularly in recall and AP75, indicating enhanced target coverage and localization consistency. For HRSID, where most images exhibit relatively simple backgrounds, CGAAN still achieves stable gains and maintains the best overall performance. The visualization results further confirm that CGAAN can effectively suppress false alarms and missed detections under different scene conditions. These advantages primarily stem from its adaptive structural design. In future work, more flexible adaptive strategies can be explored to further improve generalization across diverse SAR imaging conditions and more challenging small-target detection tasks.

Author Contributions

Conceptualization, L.Y. and W.H.; methodology, X.X.; software, X.X. and X.J.; validation, M.L. and X.Y.; writing, L.Y. and X.X. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by the National Natural Science Foundation of China (no. 62261027, no. 62561003, no. 62566028, and no. 62266020), the Natural Science Foundation of Jiangxi Province (no. 20252BAC240198, no. 20224BAB202002, and no. 20224BAB212013), the Jiangxi Provincial Graduate Innovation Special Foundation under Grant YC2024-S571, the Jiangxi Provincial Key Laboratory of Multidimensional Intelligent Perception and Control of China (no. 2024SSY03161), and the Supercomputing Platform of Jiangxi University of Science and Technology.

Data Availability Statement

The SAR-Aircraft-1.0 dataset is available at https://aistudio.baidu.com/datasetdetail/312407, accessed on 28 March 2026. The HRSID dataset is available at https://github.com/chaozhong2010/HRSID, accessed on 28 March 2026.

Conflicts of Interest

The authors declare no conflicts of interest.

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Figure 1. Two datasets with different complexities. (a) SAR-AIRcraft-1.0 dataset. (b) HRSID dataset (onshore). (c) HRSID dataset (offshore).
Figure 1. Two datasets with different complexities. (a) SAR-AIRcraft-1.0 dataset. (b) HRSID dataset (onshore). (c) HRSID dataset (offshore).
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Figure 2. The overall framework of CGAAN. (a) CA-CFAR-based complexity assessment. (b) Backbone. (c) SAN. (d) CMH.
Figure 2. The overall framework of CGAAN. (a) CA-CFAR-based complexity assessment. (b) Backbone. (c) SAN. (d) CMH.
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Figure 3. The structures of DCSP and SPPF. (a) DCSP. (b) SPPF.
Figure 3. The structures of DCSP and SPPF. (a) DCSP. (b) SPPF.
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Figure 4. The structure of SDI-GSC. (a) SDI-GSC. (b) Simplified SDI-GSC. (c) GSConv.
Figure 4. The structure of SDI-GSC. (a) SDI-GSC. (b) Simplified SDI-GSC. (c) GSConv.
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Figure 5. The structures of SAN under Mode S and D. (a) Mode S. (b) Mode D. (c) SDI-GSC1. (d) SDI-GSC2. (e) SDI-GSC3. (f) SDI-GSC4. (g) SDI-GSC5. (h) SDI-GSC6.
Figure 5. The structures of SAN under Mode S and D. (a) Mode S. (b) Mode D. (c) SDI-GSC1. (d) SDI-GSC2. (e) SDI-GSC3. (f) SDI-GSC4. (g) SDI-GSC5. (h) SDI-GSC6.
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Figure 6. Distribution of local adaptive thresholds. (a) SAR-AIRcraft-1.0. (b) HRSID.
Figure 6. Distribution of local adaptive thresholds. (a) SAR-AIRcraft-1.0. (b) HRSID.
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Figure 7. Pixels in an image whose T values exceed Tglobal. (a) SAR-AIRcraft-1.0. (b) HRSID.
Figure 7. Pixels in an image whose T values exceed Tglobal. (a) SAR-AIRcraft-1.0. (b) HRSID.
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Figure 8. (a) Baseline. (b) Baseline+DCSP. (c) Baseline+DCSP+SAN. (d) Baseline+DCSP+SAN+CMH. (e) Ground truth.
Figure 8. (a) Baseline. (b) Baseline+DCSP. (c) Baseline+DCSP+SAN. (d) Baseline+DCSP+SAN+CMH. (e) Ground truth.
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Figure 9. (a) Baseline. (b) Baseline+DCSP. (c) Baseline+DCSP+SAN. (d) Baseline+DCSP+SAN+CMH. (e) Ground truth.
Figure 9. (a) Baseline. (b) Baseline+DCSP. (c) Baseline+DCSP+SAN. (d) Baseline+DCSP+SAN+CMH. (e) Ground truth.
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Figure 10. Comparison of detection results on the SAR-AIRcraft-1.0 dataset. (a) RetinaNet. (b) GFL. (c) AutoAssign. (d) ATSS. (e) FCOS. (f) RTMDet. (g) YOLOv10. (h) CGAAN (Ours). Green, red, and blue bounding boxes denote correctly detected targets, missed detections, and false alarms, respectively.
Figure 10. Comparison of detection results on the SAR-AIRcraft-1.0 dataset. (a) RetinaNet. (b) GFL. (c) AutoAssign. (d) ATSS. (e) FCOS. (f) RTMDet. (g) YOLOv10. (h) CGAAN (Ours). Green, red, and blue bounding boxes denote correctly detected targets, missed detections, and false alarms, respectively.
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Figure 11. Comparison of detection results on the HRSID dataset. (a) RetinaNet. (b) GFL. (c) AutoAssign. (d) ATSS. (e) FCOS. (f) DDOD. (g) FoveaBox. (h) RTMDet. (i) YOLOv10. (j) CGAAN (Ours). From left to right, the 2nd and 5th columns correspond to offshore SAR images, while the 1st, 3rd, and 4th columns correspond to nearshore SAR images.
Figure 11. Comparison of detection results on the HRSID dataset. (a) RetinaNet. (b) GFL. (c) AutoAssign. (d) ATSS. (e) FCOS. (f) DDOD. (g) FoveaBox. (h) RTMDet. (i) YOLOv10. (j) CGAAN (Ours). From left to right, the 2nd and 5th columns correspond to offshore SAR images, while the 1st, 3rd, and 4th columns correspond to nearshore SAR images.
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Table 1. Ablation Experiments on SAR-AIRcraft-1.0 Dataset.
Table 1. Ablation Experiments on SAR-AIRcraft-1.0 Dataset.
Baseline DCSP SAN CMH P(%) R(%) AP50(%) AP75(%) AP50:95(%) Parameters(M) FLOPs(G) FPS
85.5 90.5 93.8 80.5 70.6 17.9 46.3 285
85.9 91 94.5 80.7 71 18.5 46.3 278
86.8 92.5 95.3 81 70.9 14.3 35.8 251
88.4 92.6 96.4 81.3 71.3 17.9 46.3 286
87.6 93 95.1 80.9 71.4 14.9 35.8 250
89 92.5 95.8 81.4 71.9 14.3 35.8 253
87.3 94.1 96.6 80.8 71.5 18.5 46.3 279
89.3 94.3 96.7 81.5 72 14.9 35.8 253
Table 2. Ablation Experiments on HRSID Dataset.
Table 2. Ablation Experiments on HRSID Dataset.
Baseline DCSP SAN CMH P(%) R(%) AP50(%) AP75(%) AP50:95(%) Parameters(M) FLOPs(G) FPS
90.9 85.7 91.5 79.8 69.4 17.9 46.3 243
92.2 85.6 92.2 79.9 70.5 18.5 46.3 233
93.2 84.2 92.2 80 70.4 14.3 43.2 219
91.6 85.9 92.5 79.7 70.2 17.9 46.3 239
92.9 86.4 93.2 80.7 71.1 14.9 43.2 210
92.5 85.9 92.7 80.6 70.9 14.3 43.2 211
92.6 86.6 91.6 81 70 18.5 46.3 232
93.6 87.4 93.3 81.2 71.9 14.9 43.2 211
Table 3. Hyperparameter Experiments on SAR-AIRcraft-1.0 Dataset.
Table 3. Hyperparameter Experiments on SAR-AIRcraft-1.0 Dataset.
I0 P(%) R(%) AP50(%) AP75(%) AP50:95(%)
0.1 89.2 92.8 96.3 81.4 71.6
0.3 88.1 94.3 95.9 81.2 71.4
0.5 89.3 94.3 96.7 81.5 72
0.7 86.4 94 95.1 80.9 70.8
Table 4. Hyperparameter Experiments on HRSID Dataset.
Table 4. Hyperparameter Experiments on HRSID Dataset.
I0 P(%) R(%) AP50(%) AP75(%) AP50:95(%)
0.1 93.6 87.4 93.3 81.2 71.9
0.3 93.1 85.6 92.7 80.8 71.5
0.5 92.6 84.3 91.4 81 71.2
0.7 92.1 82.2 90.3 80.5 70.6
Table 5. Comparative Experiments on SAR-AIRcraft-1.0 Dataset.
Table 5. Comparative Experiments on SAR-AIRcraft-1.0 Dataset.
Methods Backbone P(%) R(%) AP50(%) AP75(%)
RetinaNet [43] ResNet18 76 71.9 79 56.4
GFL [44] ResNet18 80.9 79.2 83.9 59.1
AutoAssign [45] ResNet18 82.3 80 85.5 68.2
ATSS [46] ResNet18 75.2 74.9 80.3 59.1
FCOS [47] ResNet18 78.6 79.8 85.6 61
RTMDet [48] ResNet18 82.6 92.6 94.2 73.9
YOLOv10 [49] ResNet18 87.1 91.8 95.3 78.9
CGAAN (Ours) ResNet18 89.3 94.3 96.7 81.5
Faster R-CNN [21,50] ResNet50 77.6 78.1 71.6 53.6
Cascade R-CNN [21,51] ResNet50 89 79.5 77.8 59.1
RepPoints [21,52] ResNet50 62.7 88.7 80.3 52.9
SKG-Net [21,53] ResNet50 57.6 88.8 79.8 51
SA-Net [21] ResNet50 87.5 82.2 80.4 61.4
CGAAN (Ours) ResNet50 87 94.1 95.6 80.6
Table 6. Comparative Experiments on HRSID Dataset.
Table 6. Comparative Experiments on HRSID Dataset.
Methods Backbone P(%) R(%) AP50(%) AP75(%)
RetinaNet [43] ResNet18 83.9 69.2 78.8 59.8
GFL [44] ResNet18 91.1 71.6 82.8 62.1
AutoAssign [45] ResNet18 88.7 73.7 83 62.7
ATSS [46] ResNet18 87 71.7 81.8 61.8
FCOS [47] ResNet18 88.6 70.4 81 61.9
DDOD [54] ResNet18 83.3 59.7 70.3 57.6
FoveaBox [55] ResNet18 83.8 65.2 75.5 59
RTMDet [48] ResNet18 93 82.5 90.5 71.3
YOLOv10 [49] ResNet18 90.9 83.1 90 73.8
CGAAN (Ours) ResNet18 93.6 87.4 93.3 81.2
Table 7. Detection Results on SAR-AIRCRAFT-1.0 and HRSID Datasets under Two Fusion Modes.
Table 7. Detection Results on SAR-AIRCRAFT-1.0 and HRSID Datasets under Two Fusion Modes.
Dataset Fusion Mode P(%) R(%) AP50(%) AP75(%) AP50:95(%)
SAR-AIRcraft-1.0 D 89.3 94.3 96.7 81.5 72
S 85.5 92.2 94.4 79.8 68.2
HRSID D 89.8 73.2 84.2 73.8 64.2
S 93.6 87.4 93.3 81.2 71.9
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