Efficient infrared dim object detection has been challenged by low signal-to-noise ratios (SNRs). Traditional methods rely on the gradient difference and fixed-parameter model. These methods fail to adapt to sophisticated and variable situations in the real world. To tackle the issue, a deep learning method based on the spatio-temporal network is proposed in this paper. The model is established by the Convolutional Long Short-Term Memory cell (Conv-LSTM) and the 3D Convolution cell (3D-Conv). It is trained to learn the motion constraint of moving targets (spatio-temporal constraint module, called STM) and to fuse the multiscale local feature between the target and background (deep spatial features module, called DFM). In addition, a variable interval search module (state-aware module, called STAM) is added to the inference. The submodule decides to conduct a global search for images only if the target is lost due to fast motion, uncertain obstruction, and frame loss. Comprehensive experiments indicate that the proposed method achieves better performance over all baseline methods. On the mid-wave infrared datasets collected by the authors, the proposed method achieves a 95.87% detection rate. The SNR of the dataset is around 1–3 dB, and the background of the sequence includes sky, asphalt road, and buildings.

In response to problems such as large target scale variations, strong background noise, and blurred features leading by low contrast in infrared target detection in near space environments, this paper proposes an efficient detection model, YOLO-MARS, which is based on YOLOv8. The model introduces a Space-to-Depth (SPD) convolution module into the backbone section, which retains the detailed features of smaller targets by downsampling operations without information loss, alleviating the loss of the target feature caused by traditional downsampling. The Grouped Multi-Head Self-Attention (GMHSA) module is added after the backbone’s SPPF module to improve cross-scale global modeling capabilities for target area feature responses while suppressing complex thermal noise background interference. In addition, a Light Adaptive Spatial Feature Fusion (LASFF) detector head is designed to mitigate the scale sensitivity issue of infrared targets (especially smaller targets) in the feature pyramid. It uses a shared weighting mechanism to achieve adaptive fusion of multi-scale features, reducing computational complexity while improving target localization and classification accuracy. To address the extreme scarcity of near space data, we integrated 284 near space images with the HIT-UAV dataset through physical equivalence analysis (atmospheric transmittance, contrast, and signal-to-noise ratio) to construct the NS-HIT dataset. The experimental results show that ${mAP}_{@0.5}$ increases by 5.4% and the number of parameters only increase 10% using YOLO-MARS compared to YOLOv8. YOLO-MARS improves the accuracy of detection significantly while considering the requirements of model complexity, which provides an efficient and reliable solution for applications in near space infrared target detection.

Infrared small target detection is a critical task in remote sensing. However, it remains highly challenging due to low contrast, heavy background clutter, and large variations in target scale. Traditional convolutional networks are inadequate for joint modeling, as they cannot effectively capture both fine structural details and global contextual dependencies. To address these issues, we propose FSGPNet, a frequency–spatial domain jointly guided perceptual network that explicitly exploits complementary representations in both the frequency and spatial domains. Specifically, a Frequency–Spatial Enhancement Module (FSEM) is introduced to strengthen target details while suppressing background interference through high-frequency enhancement and Perona–Malik diffusion. To enhance global context modeling, we propose a Multi-Scale Global Perception (MSGP) module that integrates non-local attention with multi-scale dilated convolutions, enabling robust background modeling. Furthermore, a Gabor Transformer Attention Module (GTAM) is designed to achieve selective frequency–spatial feature aggregation via self-attention over multi-directional and multi-scale Gabor responses, effectively highlighting discriminative structures of various small targets. Extensive experiments are conducted on two benchmark datasets (IRSTD-1K and NUDT-SIRST) that cover typical remote sensing infrared scenarios. Quantitative and qualitative results demonstrate that FSGPNet consistently outperforms state-of-the-art methods across multiple evaluation metrics. These findings validate the effectiveness and robustness of the proposed FSGPNet for detecting small infrared targets in remote sensing applications.

啮齿动物是空间研究中常见的模型对象，已开展的空间生物实验中，小鼠表现出对飞行条件的有效适应.通过空间培养，研究者可对失重环境下小鼠的生理行为、骨骼和神经系统变化做进一步研究分析.本文对空间小鼠实验有效载荷的研究进展及其空间飞行实验进行了概述，为中国空间站上的小鼠培养箱设计提供参考.概述了地面小鼠培养技术和装置，为空间小鼠实验有效载荷设计提供地面对照；从实验研究内容和硬件系统设计两方面介绍了国际上已开展的空间小鼠实验，为中国空间生命科学研究和工程研制提供参考；对于中国发展空间小鼠实验有效载荷提出了建议.

Infrared small target detection is a critical task in remote sensing, where targets typically span only a few pixels and are easily submerged by complex background clutter. Traditional convolutional networks predominantly rely on data-driven feature learning or computationally expensive global attention mechanisms. In this paper, we propose the Anomaly-Driven Gated Fusion Network (ADGFNet), a lightweight end-to-end framework that explicitly embeds the statistical characteristics into the feature extraction and fusion pipeline. The core of ADGFNet comprises two synergistic modules: Local Anomaly Block (LAB), which decomposes anomaly perception into a Local Contrast Branch capturing multi-scale intensity saliency and a Gradient Prior Branch extracting boundary discontinuities via Sobel operators; and Anomaly-Guided Feature Pyramid Neck (AG-FPN), which reuses the spatial anomaly maps generated by the LAB as guidance gates to perform spatially selective cross-scale feature fusion without requiring additional learnable spatial-attention modules. Comprehensive evaluations on the NUDT-SIRST and IRSTD-1K benchmarks demonstrate that ADGFNet achieves a superior accuracy–efficiency trade-off, attaining the best nIoU and the lowest false alarm rates with only 0.58 M parameters. With TensorRT FP16 acceleration, ADGFNet and its ultra-lightweight variant, ADGFNet-Lite (0.12 M parameters), enable real-time inference without appreciable loss of detection accuracy on an NVIDIA Jetson AGX Xavier.

As a widely used display device, the effective display area of a digital micromirror device (DMD) is limited by its micromirror count and pitch, which cannot meet large-format target-plane display requirements. This paper proposes a large-format scene simulation system based on multi-DMD optical stitching, and uses an optical relay to overcome the inability to directly tile DMDs because of their package frames. By constructing a DMD display architecture comprising an illumination module, a relay module, a stitching module, and a projection module, the system quadruples the effective display area relative to a single DMD without sacrificing frame rate. Design results show that the system achieves an MTF greater than 0.5 at 50 lp/mm, with near-diffraction-limited performance; the RMS spot radius is less than 10 $\mathsf{\mu }$m. All key indicators meet application requirements.