首页 > 最新文献

Advances in Space Research最新文献

英文 中文
VOH-Net: vision-optimized hybrid network for deep learning-based phase unwrapping VOH-Net:基于深度学习的相位展开的视觉优化混合网络
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.11.077
Saoussen Djeddi , Tarek Bentahar , Riad Saidi , Yacine Belhocine
Phase unwrapping remains a critical and inherently challenging task in interferometric synthetic aperture radar (InSAR) data processing, particularly for applications such as ground deformation monitoring, terrain mapping, and infrastructure stability assessment. Traditional and heuristic-based methods often exhibit limitations in the presence of high noise levels, phase discontinuities, and complex surface topographies, leading to compromised accuracy and reliability. In this study, we introduce VOH-Net (Vision-Optimized Hybrid Network), a novel deep learning architecture that synergistically combines convolutional neural networks (CNNs) with enhanced long short-term memory (E-LSTM) models within a unified encoder-decoder framework. The encoder extracts multi-scale spatial representations from wrapped phase maps, while the E-LSTM modules model contextual dependencies across spatial domains to facilitate more coherent phase reconstruction in the decoder. A hybrid loss function, comprising total variation, variance of error, and mean squared error, is employed to enforce smoothness, structural consistency, and pixel-wise precision. Comprehensive experiments conducted on both synthetic and real InSAR interferograms demonstrate that VOH-Net consistently outperforms conventional and state-of-the-art deep learning-based methods. Specifically, VOH-Net achieves a 21.3 % reduction in RMSE, an 18.7 % improvement in phase continuity index, and an overall unwrapping accuracy exceeding 94.6 % on challenging terrain scenarios. Moreover, it shows robust generalization capabilities across varying noise levels and interferometric conditions. These quantitative gains underscore the effectiveness of the proposed architecture in handling discontinuities and noise-corrupted inputs. VOH-Net thus offers a powerful, scalable solution for next generation InSAR applications, paving the way for more reliable and automated satellite-based geophysical monitoring.
相位展开在干涉合成孔径雷达(InSAR)数据处理中仍然是一项关键且具有挑战性的任务,特别是在地面变形监测、地形测绘和基础设施稳定性评估等应用中。传统的和基于启发式的方法在存在高噪声水平、相位不连续和复杂的表面地形时往往表现出局限性,导致准确性和可靠性受损。在本研究中,我们介绍了VOH-Net(视觉优化混合网络),这是一种新颖的深度学习架构,它在统一的编码器-解码器框架内协同结合了卷积神经网络(cnn)和增强型长短期记忆(E-LSTM)模型。编码器从包装相位图中提取多尺度空间表示,而E-LSTM模块跨空间域建模上下文依赖关系,以促进解码器中更连贯的相位重建。混合损失函数,包括总变异、误差方差和均方误差,用于增强平滑性、结构一致性和像素精度。在合成和真实InSAR干涉图上进行的综合实验表明,VOH-Net始终优于传统和最先进的基于深度学习的方法。具体来说,VOH-Net的RMSE降低了21.3%,相位连续性指数提高了18.7%,在具有挑战性的地形情况下,整体展开精度超过了94.6%。此外,它在不同的噪声水平和干涉条件下显示出强大的泛化能力。这些定量增益强调了所提出的结构在处理不连续和噪声损坏输入方面的有效性。因此,VOH-Net为下一代InSAR应用提供了强大的、可扩展的解决方案,为更可靠和自动化的卫星地球物理监测铺平了道路。
{"title":"VOH-Net: vision-optimized hybrid network for deep learning-based phase unwrapping","authors":"Saoussen Djeddi ,&nbsp;Tarek Bentahar ,&nbsp;Riad Saidi ,&nbsp;Yacine Belhocine","doi":"10.1016/j.asr.2025.11.077","DOIUrl":"10.1016/j.asr.2025.11.077","url":null,"abstract":"<div><div>Phase unwrapping remains a critical and inherently challenging task in interferometric synthetic aperture radar (InSAR) data processing, particularly for applications such as ground deformation monitoring, terrain mapping, and infrastructure stability assessment. Traditional and heuristic-based methods often exhibit limitations in the presence of high noise levels, phase discontinuities, and complex surface topographies, leading to compromised accuracy and reliability. In this study, we introduce VOH-Net (Vision-Optimized Hybrid Network), a novel deep learning architecture that synergistically combines convolutional neural networks (CNNs) with enhanced long short-term memory (E-LSTM) models within a unified encoder-decoder framework. The encoder extracts multi-scale spatial representations from wrapped phase maps, while the E-LSTM modules model contextual dependencies across spatial domains to facilitate more coherent phase reconstruction in the decoder. A hybrid loss function, comprising total variation, variance of error, and mean squared error, is employed to enforce smoothness, structural consistency, and pixel-wise precision. Comprehensive experiments conducted on both synthetic and real InSAR interferograms demonstrate that VOH-Net consistently outperforms conventional and state-of-the-art deep learning-based methods. Specifically, VOH-Net achieves a 21.3 % reduction in RMSE, an 18.7 % improvement in phase continuity index, and an overall unwrapping accuracy exceeding 94.6 % on challenging terrain scenarios. Moreover, it shows robust generalization capabilities across varying noise levels and interferometric conditions. These quantitative gains underscore the effectiveness of the proposed architecture in handling discontinuities and noise-corrupted inputs. VOH-Net thus offers a powerful, scalable solution for next generation InSAR applications, paving the way for more reliable and automated satellite-based geophysical monitoring.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3220-3238"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081809","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Determination of reference point for Sheshan SLR telescope using self-driven prism system 利用自驱动棱镜系统确定佘山单反望远镜参考点
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.12.015
Zhikang Wang , Zhibin Zhang , Bin Wang , Shuzhen Yuan , Zhipeng Mei , Xiaohui Ma , Liangquan Jia , Yong Liu , Haifeng Zhang , Si Qin , Li Zhang , Chengli Huang , Zhaoxiang Qi
High-precision geodetic datums are crucial for studying Earth’s motion and deformation, positioning, and deep space exploration. The reference point coordinates of instruments from different geodetic techniques (i.e., local tie vector) constitute fundamental elements in the construction of high-precision geodetic data set. Constrained by physical limitations, the reference point coordinates of SLR telescopes cannot be obtained through direct observation. Traditional reference point determination measurements are time-consuming and prone to systematic errors. To address these challenges, we designed and implemented a self-driven prism system that enables automatic monitoring of target points moving with the telescope. Applying this system to the Sheshan SLR telescope, the experimental results demonstrate that a few hours monitoring can achieve a submillimeter error in the reference point coordinates, with the consistency of the coordinate components of ITRF2020 within 5 mm. The self-driven prism system enables more optimal target scatter observation with improved dispersion, which in turn reduces the correlations among the solved reference point horizontal coordinates, the tilt of the azimuth axis and other parameters. Moreover, this system is highly beneficial for the high spatio-temporal resolution monitoring of reference points and local tie vectors, as well as for the construction of multi-technology geodetic reference frames.
高精度大地测量基准是研究地球运动和变形、定位和深空探测的关键。不同大地测量技术仪器的参考点坐标(即局部联系向量)是构建高精度大地测量数据集的基本要素。受物理条件的限制,单反望远镜的参考点坐标无法通过直接观测得到。传统的参考点测定测量既耗时又容易产生系统误差。为了应对这些挑战,我们设计并实现了一个自驱动棱镜系统,可以自动监测随着望远镜移动的目标点。将该系统应用于佘山单反望远镜,实验结果表明,几个小时的监测可以实现参考点坐标的亚毫米误差,ITRF2020的坐标分量一致性在5毫米以内。自驱动棱镜系统使目标散射观测更加优化,色散得到改善,从而降低了解算参考点水平坐标、方位轴倾角等参数之间的相关性。此外,该系统对参考点和局部联系向量的高时空分辨率监测以及多技术大地测量参考框架的构建非常有利。
{"title":"Determination of reference point for Sheshan SLR telescope using self-driven prism system","authors":"Zhikang Wang ,&nbsp;Zhibin Zhang ,&nbsp;Bin Wang ,&nbsp;Shuzhen Yuan ,&nbsp;Zhipeng Mei ,&nbsp;Xiaohui Ma ,&nbsp;Liangquan Jia ,&nbsp;Yong Liu ,&nbsp;Haifeng Zhang ,&nbsp;Si Qin ,&nbsp;Li Zhang ,&nbsp;Chengli Huang ,&nbsp;Zhaoxiang Qi","doi":"10.1016/j.asr.2025.12.015","DOIUrl":"10.1016/j.asr.2025.12.015","url":null,"abstract":"<div><div>High-precision geodetic datums are crucial for studying Earth’s motion and deformation, positioning, and deep space exploration. The reference point coordinates of instruments from different geodetic techniques (i.e., local tie vector) constitute fundamental elements in the construction of high-precision geodetic data set. Constrained by physical limitations, the reference point coordinates of SLR telescopes cannot be obtained through direct observation. Traditional reference point determination measurements are time-consuming and prone to systematic errors. To address these challenges, we designed and implemented a self-driven prism system that enables automatic monitoring of target points moving with the telescope. Applying this system to the Sheshan SLR telescope, the experimental results demonstrate that a few hours monitoring can achieve a submillimeter error in the reference point coordinates, with the consistency of the coordinate components of ITRF2020 within 5 mm. The self-driven prism system enables more optimal target scatter observation with improved dispersion, which in turn reduces the correlations among the solved reference point horizontal coordinates, the tilt of the azimuth axis and other parameters. Moreover, this system is highly beneficial for the high spatio-temporal resolution monitoring of reference points and local tie vectors, as well as for the construction of multi-technology geodetic reference frames.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3628-3639"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081338","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Experimental assessment of wood as a lightweight proton-radiation shield for spacecraft structures 木材作为航天器结构轻型质子辐射屏蔽材料的实验评估
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.12.021
Woo-Min Cho , Hyun-Ung Oh
Wooden satellites are currently under development owing to their lighter weight, better processability, and lower manufacturing costs compared with conventional metallic constructs. Additionally, wooden satellites are inherently capable of autogenous deorbit burn-up after completing the mission. Therefore, wooden satellites are proposed to mitigate orbital waste. However, there is a general lack of research and knowledge on the space radiation shielding characteristics of wood, compared with conventional materials used in satellite structural manufacturing. Space radiation is an essential factor to consider in satellite system design, and energetic ions can markedly impair or destroy onboard electronics. To evaluate the radiation shielding properties of wood, 10 species underwent proton beam irradiation. The experimental results demonstrated that the two species effectively attenuated ionizing particles. Furthermore, the radiation energy degradation rate was quantified for wood and aluminum shielding to demonstrate suitability for space applications.
与传统金属结构相比,木制卫星的重量更轻,可加工性更好,制造成本更低,因此目前正在开发中。此外,木制卫星在完成任务后具有自燃脱轨的能力。因此,建议使用木制卫星来减少轨道浪费。然而,与卫星结构制造中使用的传统材料相比,普遍缺乏关于木材空间辐射屏蔽特性的研究和知识。空间辐射是卫星系统设计中必须考虑的一个重要因素,高能离子会对卫星上的电子设备造成明显的损伤或破坏。为了评价木材的辐射屏蔽性能,对10种木材进行了质子束辐照。实验结果表明,这两种物质能有效地衰减电离粒子。此外,还量化了木材和铝屏蔽的辐射能量降解率,以证明其适合空间应用。
{"title":"Experimental assessment of wood as a lightweight proton-radiation shield for spacecraft structures","authors":"Woo-Min Cho ,&nbsp;Hyun-Ung Oh","doi":"10.1016/j.asr.2025.12.021","DOIUrl":"10.1016/j.asr.2025.12.021","url":null,"abstract":"<div><div>Wooden satellites are currently under development owing to their lighter weight, better processability, and lower manufacturing costs compared with conventional metallic constructs. Additionally, wooden satellites are inherently capable of autogenous deorbit burn-up after completing the mission. Therefore, wooden satellites are proposed to mitigate orbital waste. However, there is a general lack of research and knowledge on the space radiation shielding characteristics of wood, compared with conventional materials used in satellite structural manufacturing. Space radiation is an essential factor to consider in satellite system design, and energetic ions can markedly impair or destroy onboard electronics. To evaluate the radiation shielding properties of wood, 10 species underwent proton beam irradiation. The experimental results demonstrated that the two species effectively attenuated ionizing particles. Furthermore, the radiation energy degradation rate was quantified for wood and aluminum shielding to demonstrate suitability for space applications.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3640-3653"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081341","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Channels near 22.235 GHz band improve the accuracy of water vapor profile measurements by microwave sounders 22.235 GHz附近通道提高了微波测深仪测量水汽廓线的精度
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.11.075
E.V. Pashinov , V.V. Sterlyadkin
It is known that passive microwave measurements of the atmospheric humidity profile from space at a typical frequency set of 165.5–183.31 GHz are weakly sensitive to changes in tropospheric humidity below 4 km, where most of the water vapor is concentrated. The calculations showed that additional use of radiometric channels near 22.235 GHz absorption line (18–27 GHz) allows obtaining differential weighting functions with altitude selectivity in the range of 0–3.5 km and the required sensitivity. The information content of additional channels was assessed. It turned out that the degrees of freedom increase by 1.2 or 35–63 %. Modeling of various humidity profiles showed that adding channels near 22.235 GHz band reduces measurement errors at altitudes of 1–4.0 km by 10–40 % and allows to retrieve water vapor profile inversions. The method of humidity profile retrieving using low-frequency channels was applied to real radiometric data obtained by the MTVZA-GYa device installed on the Meteor-M №2 satellite. It turned out that the additional use of 18.7 GHz (V); 23.8 GHz (V) and 31.5 GHz (V) channels in solving the problem of water vapor profile retrieving allowed us to reduce retrieving errors by 10–30 % at altitudes of 1–3 km, which confirmed theoretical and model calculations.
众所周知,在165.5-183.31 GHz的典型频率组上,从太空对大气湿度剖面的被动微波测量对4公里以下对流层湿度变化的敏感性较弱,而4公里以下是大部分水蒸气集中的地方。计算表明,在22.235 GHz吸收线(18-27 GHz)附近额外使用辐射通道,可以获得0-3.5 km范围内具有高度选择性和所需灵敏度的微分加权函数。评估了其他渠道的信息内容。结果表明,自由度增加了1.2%,即35 - 63%。各种湿度廓线的模拟表明,在22.235 GHz波段附近增加通道可使1-4.0 km高度的测量误差降低10 - 40%,并可恢复水汽廓线的逆温。将低频通道湿度廓线反演方法应用于气象二号卫星上安装的MTVZA-GYa装置获得的实际辐射数据。事实证明,额外使用18.7 GHz (V);23.8 GHz (V)和31.5 GHz (V)通道解决了水汽剖面反演问题,使反演误差在1 ~ 3 km高度降低了10 ~ 30%,验证了理论和模式计算。
{"title":"Channels near 22.235 GHz band improve the accuracy of water vapor profile measurements by microwave sounders","authors":"E.V. Pashinov ,&nbsp;V.V. Sterlyadkin","doi":"10.1016/j.asr.2025.11.075","DOIUrl":"10.1016/j.asr.2025.11.075","url":null,"abstract":"<div><div>It is known that passive microwave measurements of the atmospheric humidity profile from space at a typical frequency set of 165.5–183.31 GHz are weakly sensitive to changes in tropospheric humidity below 4 km, where most of the water vapor is concentrated. The calculations showed that additional use of radiometric channels near 22.235 GHz absorption line (18–27 GHz) allows obtaining differential weighting functions with altitude selectivity in the range of 0–3.5 km and the required sensitivity. The information content of additional channels was assessed. It turned out that the degrees of freedom increase by 1.2 or 35–63 %. Modeling of various humidity profiles showed that adding channels near 22.235 GHz band reduces measurement errors at altitudes of 1–4.0 km by 10–40 % and allows to retrieve water vapor profile inversions. The method of humidity profile retrieving using low-frequency channels was applied to real radiometric data obtained by the MTVZA-GYa device installed on the Meteor-M №2 satellite. It turned out that the additional use of 18.7 GHz (V); 23.8 GHz (V) and 31.5 GHz (V) channels in solving the problem of water vapor profile retrieving allowed us to reduce retrieving errors by 10–30 % at altitudes of 1–3 km, which confirmed theoretical and model calculations.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3190-3200"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081344","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Neuroadaptive predefined-time 6-DOF integrated tracking control for spacecraft proximity operations with pose constraints 具有位姿约束的航天器接近操作神经自适应预定义时间六自由度综合跟踪控制
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.11.061
Yu Wang , Kang Liu , Yuquan Chen
This paper investigates the predefined-time relative position and attitude tracking control problem with pose constraints for spacecraft proximity operations. First, a modified practically predefined time stable (PPTS) system is established as theoretical basis of subsequent control design. Compared to previous PPTS-based studies, this article emphasises system response speed. Furthermore, by incorporating the quadratic-fraction type barrier Lyapunov function and neural networks into the predefined-time command filtered backstepping procedure, the pose constraints are not violated and the unknown dynamic terms are compensated, simultaneously. It is verified that the closed-loop system is PPTS, and the boundedness of system states can be guaranteed and the tracking errors can adjusted within predefined time. Finally, comparative simulations are implemented to substantiate the performance of the proposed method.
研究了航天器接近操作中具有姿态约束的预定时间相对位置和姿态跟踪控制问题。首先,建立了一个改进的实际预定义时间稳定系统,作为后续控制设计的理论基础。与以往基于ppts的研究相比,本文强调系统响应速度。此外,将二次分数型障碍Lyapunov函数和神经网络结合到预定义时间命令滤波的反演过程中,既不违反位姿约束,同时又补偿了未知动态项。验证了闭环系统是pts,能够保证系统状态的有界性,并能在预定时间内调整跟踪误差。最后,通过对比仿真验证了该方法的有效性。
{"title":"Neuroadaptive predefined-time 6-DOF integrated tracking control for spacecraft proximity operations with pose constraints","authors":"Yu Wang ,&nbsp;Kang Liu ,&nbsp;Yuquan Chen","doi":"10.1016/j.asr.2025.11.061","DOIUrl":"10.1016/j.asr.2025.11.061","url":null,"abstract":"<div><div>This paper investigates the predefined-time relative position and attitude tracking control problem with pose constraints for spacecraft proximity operations. First, a modified practically predefined time stable (PPTS) system is established as theoretical basis of subsequent control design. Compared to previous PPTS-based studies, this article emphasises system response speed. Furthermore, by incorporating the quadratic-fraction type barrier Lyapunov function and neural networks into the predefined-time command filtered backstepping procedure, the pose constraints are not violated and the unknown dynamic terms are compensated, simultaneously. It is verified that the closed-loop system is PPTS, and the boundedness of system states can be guaranteed and the tracking errors can adjusted within predefined time. Finally, comparative simulations are implemented to substantiate the performance of the proposed method.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3906-3921"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081630","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
The IRIS reflectance IR database for space missions 用于空间任务的IRIS反射率红外数据库
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.12.048
I. Weber, M.P. Reitze, T. Heyer, A. Morlok, T. Grund, H. Hiesinger
Infrared (IR) spectroscopy is widely used in the analysis of a broad range of different materials. The technique is sensitive, well approved, non-destructive and can be used in-situ, making it ideal for remote applications. In relation to space missions, IR remote sensing has been shown to provide essential information about the compositions of planetary surfaces being studied. Because of its proven ability, IR spectroscopy has been a cornerstone of space missions for decades, playing a key role in identifying ices, minerals, and organic compounds on planets, moons, and asteroids.
For the correct interpretation of remote sensing IR data, laboratory spectra of suitable analogue material are required, ideally in a dedicated database. Thus, the IRIS (InfraRed and Raman for Interplanetary Spectroscopy) laboratory in Münster generates spectra from analogue material similar to the materials expected to occur on planetary surfaces, especially Mercury, but also on other Solar System bodies without atmosphere, such as the Moon or asteroids.
In this article, we present a continuously expanding database of infrared reflection spectra from laboratory measurements. The measured analogue materials were and are selected on the basis of previously published remote sensing observations and our own investigations (e.g., of the Moon and meteorites) or were produced internally. In addition, we present not only reflectance spectra, but also chemical and microscopic analyses, as well as Raman spectra. The database is online, free of charge, accessible without registration, and constantly being expanded (http://IRIS.uni-muenster.de/).
The database is particularly suitable for interpreting the upcoming data from the MERTIS instrument (MErcury Radiometer and Thermal Infrared Spectrometer) on the BepiColombo mission to Mercury, which will reach the final orbit around the planet in 2026.
红外(IR)光谱学广泛应用于各种不同材料的分析。该技术灵敏、可靠、无损,可在现场使用,是远程应用的理想选择。在空间任务方面,已证明红外遥感可以提供关于所研究的行星表面组成的基本资料。由于其经过验证的能力,红外光谱学几十年来一直是太空任务的基石,在识别行星、卫星和小行星上的冰、矿物和有机化合物方面发挥着关键作用。为了正确解释遥感红外数据,需要适当的模拟物质的实验室光谱,理想情况下是在专门的数据库中。因此,nster的IRIS(红外和拉曼行星际光谱)实验室从类似于行星表面(尤其是水星)以及其他没有大气层的太阳系天体(如月球或小行星)上预计会出现的物质的模拟物质中产生光谱。在本文中,我们提出了一个不断扩大的数据库的红外反射光谱从实验室测量。测量的模拟材料是根据以前发表的遥感观测和我们自己的调查(例如对月球和陨石的调查)选择的,或者是内部生产的。此外,我们不仅提供了反射光谱,还提供了化学和微观分析以及拉曼光谱。该数据库是在线的,免费的,无需注册即可访问,并不断扩展(http://IRIS.uni-muenster.de/).The数据库特别适合解释BepiColombo水星任务中MERTIS仪器(水星辐射计和热红外光谱仪)即将获得的数据,该仪器将于2026年到达绕水星的最终轨道。
{"title":"The IRIS reflectance IR database for space missions","authors":"I. Weber,&nbsp;M.P. Reitze,&nbsp;T. Heyer,&nbsp;A. Morlok,&nbsp;T. Grund,&nbsp;H. Hiesinger","doi":"10.1016/j.asr.2025.12.048","DOIUrl":"10.1016/j.asr.2025.12.048","url":null,"abstract":"<div><div>Infrared (IR) spectroscopy is widely used in the analysis of a broad range of different materials. The technique is sensitive, well approved, non-destructive and can be used in-situ, making it ideal for remote applications. In relation to space missions, IR remote sensing has been shown to provide essential information about the compositions of planetary surfaces being studied. Because of its proven ability, IR spectroscopy has been a cornerstone of space missions for decades, playing a key role in identifying ices, minerals, and organic compounds on planets, moons, and asteroids.</div><div>For the correct interpretation of remote sensing IR data, laboratory spectra of suitable analogue material are required, ideally in a dedicated database. Thus, the IRIS (InfraRed and Raman for Interplanetary Spectroscopy) laboratory in Münster generates spectra from analogue material similar to the materials expected to occur on planetary surfaces, especially Mercury, but also on other Solar System bodies without atmosphere, such as the Moon or asteroids.</div><div>In this article, we present a continuously expanding database of infrared reflection spectra from laboratory measurements. The measured analogue materials were and are selected on the basis of previously published remote sensing observations and our own investigations (e.g., of the Moon and meteorites) or were produced internally. In addition, we present not only reflectance spectra, but also chemical and microscopic analyses, as well as Raman spectra. The database is online, free of charge, accessible without registration, and constantly being expanded (<span><span>http://IRIS.uni-muenster.de/</span><svg><path></path></svg></span>).</div><div>The database is particularly suitable for interpreting the upcoming data from the MERTIS instrument (MErcury Radiometer and Thermal Infrared Spectrometer) on the BepiColombo mission to Mercury, which will reach the final orbit around the planet in 2026.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3934-3946"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081627","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Theoretical bounds on the altimetry bias due to Earth’s curvature in ground-based GNSS reflectometry 地面GNSS反射测量中由于地球曲率引起的测高偏差的理论界限
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.11.090
Vitor Hugo de Almeida Junior , Felipe Geremia-Nievinski
Ground-based GNSS Reflectometry (GNSS-R) is a promising alternative for coastal sea level measurements. GNSS-R is a geodetic remote sensing technique based on radio waves continuously emitted by navigation satellites. In addition to the direct or line-of-sight reception, these radio waves are reflected on Earth’s surface. The interferometric delay, defined as the difference in propagation delay between reflected and direct wave paths, is the main quantity used in sea level altimetry. It may be observed indirectly, in terms of multipath power or carrier-to-noise density measurements (interference patterns). For ground-based GNSS-R, the geometrical modeling of interferometric delay normally involves a planar and horizontal reflecting surface. However, such an assumption may be not valid for reflection points far from the receiving antenna, due to the Earth’s curvature. An osculating sphere, normal to Earth’s spheroid, is a more appropriate representation of the sea surface. In the present work, we quantify the theoretical bounds on altimetry bias due to Earth’s curvature in ground-based GNSS-R. Firstly, we modeled the interferometric delay for each plane and sphere; then, we calculated the discrepancy between the two. We simulated scenarios for varying transmitting satellite elevation angle (from zenith down to the spherical horizon) and varying receiving antenna height (from zero to 500 m). Secondly, we derived an altimetry correction, based on the typical altimetry retrieval algorithm, half of the rate of change of the interferometric delay with respect to the sine of elevation angle. Considering a 1-cm altimetry error threshold for sea-level measurements, we observed that altimetry correction is needed at 10°, 20°, and 30° satellite elevation, for an antenna altitude of 60 m, 120 m, and 160 m, respectively; above 200 m antenna height, the correction is needed for any satellite elevation angle, even at zenith. We compared the rigorous altimetry correction with two approximate altimetry corrections. They differ from the rigorous one by 1 cm at antenna heights above 200 m and differences increase significantly at elevation angles close to the planar horizon.
地面GNSS反射测量(GNSS- r)是一种很有前途的沿海海平面测量替代方案。GNSS-R是一种基于导航卫星连续发射无线电波的大地测量遥感技术。除了直接或视线接收外,这些无线电波还会反射到地球表面。干涉时延定义为反射波路径和直接波路径之间传播时延的差异,是海平面测高中使用的主要量。它可以通过多径功率或载波噪声密度测量(干涉模式)间接观察到。对于地面GNSS-R,干涉延迟的几何建模通常包括平面反射面和水平反射面。然而,由于地球的曲率,这种假设可能对远离接收天线的反射点无效。一个与地球球体垂直的密切球,是海洋表面更合适的表示。在目前的工作中,我们量化了地面GNSS-R中由于地球曲率引起的测高偏差的理论界限。首先,对各平面和球面的干涉延迟进行建模;然后,我们计算两者之间的差异。我们模拟了不同发射卫星仰角(从天顶向下到球面地平线)和不同接收天线高度(从0到500米)的场景。其次,基于典型的测高检索算法,推导了干涉时延相对于仰角正弦变化率的一半的测高修正量。考虑海平面测量的测高误差阈值为1 cm,我们观察到天线高度分别为60 m、120 m和160 m时,需要在卫星高度10°、20°和30°处进行测高校正;在200米以上的天线高度,任何卫星仰角都需要校正,即使在天顶也是如此。我们比较了严格的测高校正与两种近似的测高校正。当天线高度在200米以上时,它们与严格值相差1厘米,当仰角接近平面水平时,差异显著增加。
{"title":"Theoretical bounds on the altimetry bias due to Earth’s curvature in ground-based GNSS reflectometry","authors":"Vitor Hugo de Almeida Junior ,&nbsp;Felipe Geremia-Nievinski","doi":"10.1016/j.asr.2025.11.090","DOIUrl":"10.1016/j.asr.2025.11.090","url":null,"abstract":"<div><div>Ground-based GNSS Reflectometry (GNSS-R) is a promising alternative for coastal sea level measurements. GNSS-R is a geodetic remote sensing technique based on radio waves continuously emitted by navigation satellites. In addition to the direct or line-of-sight reception, these radio waves are reflected on Earth’s surface. The interferometric delay, defined as the difference in propagation delay between reflected and direct wave paths, is the main quantity used in sea level altimetry. It may be observed indirectly, in terms of multipath power or carrier-to-noise density measurements (interference patterns). For ground-based GNSS-R, the geometrical modeling of interferometric delay normally involves a planar and horizontal reflecting surface. However, such an assumption may be not valid for reflection points far from the receiving antenna, due to the Earth’s curvature. An osculating sphere, normal to Earth’s spheroid, is a more appropriate representation of the sea surface. In the present work, we quantify the theoretical bounds on altimetry bias due to Earth’s curvature in ground-based GNSS-R. Firstly, we modeled the interferometric delay for each plane and sphere; then, we calculated the discrepancy between the two. We simulated scenarios for varying transmitting satellite elevation angle (from zenith down to the spherical horizon) and varying receiving antenna height (from zero to 500 m). Secondly, we derived an altimetry correction, based on the typical altimetry retrieval algorithm, half of the rate of change of the interferometric delay with respect to the sine of elevation angle. Considering a 1-cm altimetry error threshold for sea-level measurements, we observed that altimetry correction is needed at 10°, 20°, and 30° satellite elevation, for an antenna altitude of 60 m, 120 m, and 160 m, respectively; above 200 m antenna height, the correction is needed for any satellite elevation angle, even at zenith. We compared the rigorous altimetry correction with two approximate altimetry corrections. They differ from the rigorous one by 1 cm at antenna heights above 200 m and differences increase significantly at elevation angles close to the planar horizon.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3300-3310"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081955","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Seismo-ionospheric anomalies associated with the 2025 Mw 7.7 Myanmar earthquake: a case study 与2025 Mw 7.7缅甸地震相关的地震-电离层异常:个案研究
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.11.015
Siva Sai Kumar Rajana , Sambit Prasanajit Naik , Sampad Kumar Panda , Chiranjeevi G. Vivek , Sridevi Jade
Myanmar, located at the convergence of the Indian and Sunda plates, is one of the most seismically active and tectonically complex regions in Southeast Asia. Despite the high seismic hazard, limited ionospheric research has been conducted to understand earthquake-related atmospheric and ionospheric disturbances in this region. The Mw 7.7 Myanmar earthquake that occurred near Mandalay on 28 March 2025 has been considered in this work to examine seismo-ionospheric coupling along the active Sagaing Fault. Using GNSS-derived Total Electron Content (TEC) data, this study identifies both co-seismic and pre-seismic ionospheric anomalies. Multiple Receiver-Satellite (R-S) pairs reveal coherent, temporally correlated perturbations peaking around 0635 UT, indicative of upward-propagating seismic-induced Acoustic Gravity Waves (AGWs). The disturbance amplitudes decreased with distance from the epicenter, with dominant frequencies (3–5 mHz) consistent with seismically induced Traveling Ionospheric Disturbances (TIDs). Horizontal propagation speed of 1.19 km/s confirm the acoustic wave origin of these TEC perturbations. Prominent ionospheric anomalies are detected in the western side of the epicenter, corresponding to the fault rupture zone. These localized, directional perturbations indicate the clear coupling between the strike-slip fault dynamics and ionospheric disturbances. A significant regional TEC reduction detected three days prior to the event under geomagnetically quiet conditions suggests Lithosphere-Atmosphere-Ionosphere (LAI) coupling, likely linked to stress-induced radon emissions or electric field changes. The timing and characteristics of these anomalies reinforce the potential of TEC monitoring as an effective earthquake precursor. The findings not only demonstrate the sensitivity of TEC data to both pre- and post-seismic disturbances but also highlight the potential of TEC-based monitoring as a viable early warning tool, particularly in inter-plate settings where conventional seismic networks may be sparse or underdeveloped. Such ionospheric precursor detection can play a crucial role in enhancing seismic hazard forecasting and preparedness in geologically complex and high-risk regions like Myanmar.
缅甸位于印度板块和巽他板块的交汇处,是东南亚地震最活跃、构造最复杂的地区之一。尽管该地区地震危险性高,但在了解该地区与地震有关的大气和电离层扰动方面进行了有限的电离层研究。本文考虑了发生在2025年3月28日曼德勒附近的缅甸7.7级地震,以研究沿实皆断层活动的地震-电离层耦合。利用gnss衍生的总电子含量(TEC)数据,本研究确定了同震和震前电离层异常。多个接收机-卫星(R-S)对显示出相干的、时间相关的扰动在0635 UT左右达到峰值,表明是向上传播的地震诱发声重力波(agw)。扰动振幅随距离震中的远近而减小,主导频率(3 ~ 5 mHz)与地震诱发的电离层行扰动(TIDs)一致。1.19 km/s的水平传播速度证实了这些TEC扰动的声波起源。在震中的西侧检测到明显的电离层异常,对应于断层破裂带。这些局部的定向扰动表明走滑断层动力学和电离层扰动之间存在明显的耦合。在地磁安静的条件下,在事件发生三天前检测到明显的区域TEC减少,这表明岩石圈-大气-电离层(LAI)耦合,可能与应力诱导的氡排放或电场变化有关。这些异常的时间和特征加强了TEC监测作为有效地震前兆的潜力。这些发现不仅证明了TEC数据对地震前和地震后扰动的敏感性,而且还强调了基于TEC的监测作为一种可行的早期预警工具的潜力,特别是在传统地震台网可能稀疏或不发达的板块间环境中。这种电离层前兆探测可以在加强缅甸等地质复杂和高风险地区的地震灾害预报和防备方面发挥关键作用。
{"title":"Seismo-ionospheric anomalies associated with the 2025 Mw 7.7 Myanmar earthquake: a case study","authors":"Siva Sai Kumar Rajana ,&nbsp;Sambit Prasanajit Naik ,&nbsp;Sampad Kumar Panda ,&nbsp;Chiranjeevi G. Vivek ,&nbsp;Sridevi Jade","doi":"10.1016/j.asr.2025.11.015","DOIUrl":"10.1016/j.asr.2025.11.015","url":null,"abstract":"<div><div>Myanmar, located at the convergence of the Indian and Sunda plates, is one of the most seismically active and tectonically complex regions in Southeast Asia. Despite the high seismic hazard, limited ionospheric research has been conducted to understand earthquake-related atmospheric and ionospheric disturbances in this region. The Mw 7.7 Myanmar earthquake that occurred near Mandalay on 28 March 2025 has been considered in this work to examine seismo-ionospheric coupling along the active Sagaing Fault. Using GNSS-derived Total Electron Content (TEC) data, this study identifies both co-seismic and pre-seismic ionospheric anomalies. Multiple Receiver-Satellite (R-S) pairs reveal coherent, temporally correlated perturbations peaking around 0635 UT, indicative of upward-propagating seismic-induced Acoustic Gravity Waves (AGWs). The disturbance amplitudes decreased with distance from the epicenter, with dominant frequencies (3–5 mHz) consistent with seismically induced Traveling Ionospheric Disturbances (TIDs). Horizontal propagation speed of 1.19 km/s confirm the acoustic wave origin of these TEC perturbations. Prominent ionospheric anomalies are detected in the western side of the epicenter, corresponding to the fault rupture zone. These localized, directional perturbations indicate the clear coupling between the strike-slip fault dynamics and ionospheric disturbances. A significant regional TEC reduction detected three days prior to the event under geomagnetically quiet conditions suggests Lithosphere-Atmosphere-Ionosphere (LAI) coupling, likely linked to stress-induced radon emissions or electric field changes. The timing and characteristics of these anomalies reinforce the potential of TEC monitoring as an effective earthquake precursor. The findings not only demonstrate the sensitivity of TEC data to both pre- and post-seismic disturbances but also highlight the potential of TEC-based monitoring as a viable early warning tool, particularly in inter-plate settings where conventional seismic networks may be sparse or underdeveloped. Such ionospheric precursor detection can play a crucial role in enhancing seismic hazard forecasting and preparedness in geologically complex and high-risk regions like Myanmar.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3367-3385"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081920","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
FVMD-HTLD: Prediction of TEC based on Signal decomposition and integrated models FVMD-HTLD:基于信号分解和集成模型的TEC预测
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-02-01 DOI: 10.1016/j.asr.2025.11.033
Jumin Zhao , Qimei Wang , Fanming Wu , Hairong Jiang , Dengao Li
As a key parameter for characterizing the state of the ionosphere, the variation of total electron content (TEC) is significantly influenced by space weather events such as solar wind and solar flares, and it plays a crucial role in indicating the signal propagation of the Global Navigation Satellite System (GNSS). However, the nonlinear and non-stationary characteristics of TEC time-series data pose significant challenges to accurate prediction. In this study, an innovative prediction method for ionospheric TEC based on variational mode decomposition (VMD) and an integrated model (FVMD-HTLD) is proposed. The optimal mode number K of VMD is adaptively determined through Fast Fourier Transform (FFT) analysis. The original TEC sequence is decomposed into K Intrinsic Mode Functions (IMFs), which effectively separate the different frequency components in the signal and mine the deep features of the data. Subsequently, BiLSTM, BiTCN, vand DBN are selected as the base models, and a secondary prediction correction is achieved by establishing a nonlinear weight distribution among the prediction results of the base models. This method not only fully utilizes the advantages of different models but also further enhances prediction accuracy through a meta-learner. The input of the model consists of TEC data observed by six evenly distributed GPS reference stations in China, and it is combined with space environment parameters such as the solar activity index (F10.7) and geomagnetic indices (Dst, Kp). The experimental results show that the coefficient of determination (R2) of the integrated model on the test set reaches 0.998, with an RMSE of 0.231, which validates the effectiveness of the proposed method in ionospheric TEC prediction.
总电子含量(TEC)的变化是表征电离层状态的关键参数,受到太阳风、太阳耀斑等空间天气事件的显著影响,对全球卫星导航系统(GNSS)信号传播具有重要指示作用。然而,TEC时间序列数据的非线性和非平稳特征给准确预测带来了重大挑战。本文提出了一种基于变分模态分解(VMD)和集成模型(FVMD-HTLD)的电离层TEC预测方法。通过快速傅里叶变换(FFT)分析,自适应确定了VMD的最优模态数K。将原始TEC序列分解为K个本征模态函数(IMFs),有效分离信号中的不同频率分量,挖掘数据的深层特征。随后,选取BiLSTM、BiTCN、vand DBN作为基模型,通过建立基模型预测结果之间的非线性权重分布,实现二次预测校正。该方法不仅充分利用了不同模型的优点,而且通过元学习器进一步提高了预测精度。模型输入由中国分布均匀的6个GPS参考站观测到的TEC数据组成,并结合太阳活动指数(F10.7)和地磁指数(Dst, Kp)等空间环境参数。实验结果表明,综合模型在测试集上的决定系数(R2)达到0.998,RMSE为0.231,验证了该方法在电离层TEC预测中的有效性。
{"title":"FVMD-HTLD: Prediction of TEC based on Signal decomposition and integrated models","authors":"Jumin Zhao ,&nbsp;Qimei Wang ,&nbsp;Fanming Wu ,&nbsp;Hairong Jiang ,&nbsp;Dengao Li","doi":"10.1016/j.asr.2025.11.033","DOIUrl":"10.1016/j.asr.2025.11.033","url":null,"abstract":"<div><div>As a key parameter for characterizing the state of the ionosphere, the variation of total electron content (TEC) is significantly influenced by space weather events such as solar wind and solar flares, and it plays a crucial role in indicating the signal propagation of the Global Navigation Satellite System (GNSS). However, the nonlinear and non-stationary characteristics of TEC time-series data pose significant challenges to accurate prediction. In this study, an innovative prediction method for ionospheric TEC based on variational mode decomposition (VMD) and an integrated model (FVMD-HTLD) is proposed. The optimal mode number K of VMD is adaptively determined through Fast Fourier Transform (FFT) analysis. The original TEC sequence is decomposed into K Intrinsic Mode Functions (IMFs), which effectively separate the different frequency components in the signal and mine the deep features of the data. Subsequently, BiLSTM, BiTCN, vand DBN are selected as the base models, and a secondary prediction correction is achieved by establishing a nonlinear weight distribution among the prediction results of the base models. This method not only fully utilizes the advantages of different models but also further enhances prediction accuracy through a meta-learner. The input of the model consists of TEC data observed by six evenly distributed GPS reference stations in China, and it is combined with space environment parameters such as the solar activity index (F10.7) and geomagnetic indices (Dst, Kp). The experimental results show that the coefficient of determination (R<sup>2</sup>) of the integrated model on the test set reaches 0.998, with an RMSE of 0.231, which validates the effectiveness of the proposed method in ionospheric TEC prediction.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 3","pages":"Pages 3404-3417"},"PeriodicalIF":2.8,"publicationDate":"2026-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081921","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Revisiting the Midori-II satellite anomaly: evidence of electrostatic discharge from SPENVIS simulations 重新审视Midori-II卫星异常:来自SPENVIS模拟的静电放电证据
IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-30 DOI: 10.1016/j.asr.2025.12.023
Nizam Ahmad , Darsono , Isdandy Rezki Febrianto , Neflia , Ery Fitrianingsih , Eriko Nasemudin Nasser , Alka Budi Wahidin , Futikhatun Rohmah , Poki Agung Budiantoro , Dede Suhendar
Most damage to satellites in space originates from interactions between space radiation and satellites. Midori-II failure in October 2023, which led to its total loss, was one of such cases believed to be related to charging effects during geomagnetic storms. We studied the effect of charging on the Midori-II satellite structure, modeled as a probe, by performing simulations using SPENVIS tools, focusing on surface charging with EQUIPOT and internal dielectric charging with DICTAT. We simplified the structure of the probe into two main structures, i.e., the first structure coated by multi-layer insulation (MLI) and the second structure shielded by aluminum. Simulation results showed that the first structure experienced high-voltage charging of approximately −1.8 kV, while the second structure suffered less charging on the order of −0.5 kV. The electric field inside the dielectric surpassed the breakdown threshold of 1 × 107 V/m, suggesting a high probability of electrostatic discharge (ESD) initiation. The more significant potential drop on both structures explains the effects of charging on the probe that can be the cause of failure of the Midori-II satellite.
对空间卫星的大多数损害是由于空间辐射与卫星之间的相互作用造成的。2023年10月,Midori-II号的失败导致其全部损失,这是被认为与地磁风暴期间的充电效应有关的案例之一。通过使用SPENVIS工具进行模拟,研究了充电对Midori-II卫星结构的影响,将其建模为探针,重点研究了EQUIPOT的表面充电和DICTAT的内部介电充电。我们将探针的结构简化为两种主要结构,即第一种结构采用多层绝缘涂层(MLI),第二种结构采用铝屏蔽。仿真结果表明,第一种结构的充电电压约为−1.8 kV,而第二种结构的充电电压较小,约为−0.5 kV。电介质内部的电场超过1 × 107 V/m的击穿阈值,表明静电放电(ESD)发生的可能性很大。这两种结构上更显著的电位下降解释了充电对探测器的影响,这可能是导致Midori-II卫星失败的原因。
{"title":"Revisiting the Midori-II satellite anomaly: evidence of electrostatic discharge from SPENVIS simulations","authors":"Nizam Ahmad ,&nbsp;Darsono ,&nbsp;Isdandy Rezki Febrianto ,&nbsp;Neflia ,&nbsp;Ery Fitrianingsih ,&nbsp;Eriko Nasemudin Nasser ,&nbsp;Alka Budi Wahidin ,&nbsp;Futikhatun Rohmah ,&nbsp;Poki Agung Budiantoro ,&nbsp;Dede Suhendar","doi":"10.1016/j.asr.2025.12.023","DOIUrl":"10.1016/j.asr.2025.12.023","url":null,"abstract":"<div><div>Most damage to satellites in space originates from interactions between space radiation and satellites. Midori-II failure in October 2023, which led to its total loss, was one of such cases believed to be related to charging effects during geomagnetic storms. We studied the effect of charging on the Midori-II satellite structure, modeled as a probe, by performing simulations using SPENVIS tools, focusing on surface charging with EQUIPOT and internal dielectric charging with DICTAT. We simplified the structure of the probe into two main structures, i.e., the first structure coated by multi-layer insulation (MLI) and the second structure shielded by aluminum. Simulation results showed that the first structure experienced high-voltage charging of approximately −1.8 kV, while the second structure suffered less charging on the order of −0.5 kV. The electric field inside the dielectric surpassed the breakdown threshold of 1 × 10<sup>7</sup> V/m, suggesting a high probability of electrostatic discharge (ESD) initiation. The more significant potential drop on both structures explains the effects of charging on the probe that can be the cause of failure of the Midori-II satellite.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"77 4","pages":"Pages 5354-5363"},"PeriodicalIF":2.8,"publicationDate":"2026-01-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146081657","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
期刊
Advances in Space Research
全部 Acc. Chem. Res. ACS Applied Bio Materials ACS Appl. Electron. Mater. ACS Appl. Energy Mater. ACS Appl. Mater. Interfaces ACS Appl. Nano Mater. ACS Appl. Polym. Mater. ACS BIOMATER-SCI ENG ACS Catal. ACS Cent. Sci. ACS Chem. Biol. ACS Chemical Health & Safety ACS Chem. Neurosci. ACS Comb. Sci. ACS Earth Space Chem. ACS Energy Lett. ACS Infect. Dis. ACS Macro Lett. ACS Mater. Lett. ACS Med. Chem. Lett. ACS Nano ACS Omega ACS Photonics ACS Sens. ACS Sustainable Chem. Eng. ACS Synth. Biol. Anal. Chem. BIOCHEMISTRY-US Bioconjugate Chem. BIOMACROMOLECULES Chem. Res. Toxicol. Chem. Rev. Chem. Mater. CRYST GROWTH DES ENERG FUEL Environ. Sci. Technol. Environ. Sci. Technol. Lett. Eur. J. Inorg. Chem. IND ENG CHEM RES Inorg. Chem. J. Agric. Food. Chem. J. Chem. Eng. Data J. Chem. Educ. J. Chem. Inf. Model. J. Chem. Theory Comput. J. Med. Chem. J. Nat. Prod. J PROTEOME RES J. Am. Chem. Soc. LANGMUIR MACROMOLECULES Mol. Pharmaceutics Nano Lett. Org. Lett. ORG PROCESS RES DEV ORGANOMETALLICS J. Org. Chem. J. Phys. Chem. J. Phys. Chem. A J. Phys. Chem. B J. Phys. Chem. C J. Phys. Chem. Lett. Analyst Anal. Methods Biomater. Sci. Catal. Sci. Technol. Chem. Commun. Chem. Soc. Rev. CHEM EDUC RES PRACT CRYSTENGCOMM Dalton Trans. Energy Environ. Sci. ENVIRON SCI-NANO ENVIRON SCI-PROC IMP ENVIRON SCI-WAT RES Faraday Discuss. Food Funct. Green Chem. Inorg. Chem. Front. Integr. Biol. J. Anal. At. Spectrom. J. Mater. Chem. A J. Mater. Chem. B J. Mater. Chem. C Lab Chip Mater. Chem. Front. Mater. Horiz. MEDCHEMCOMM Metallomics Mol. Biosyst. Mol. Syst. Des. Eng. Nanoscale Nanoscale Horiz. Nat. Prod. Rep. New J. Chem. Org. Biomol. Chem. Org. Chem. Front. PHOTOCH PHOTOBIO SCI PCCP Polym. Chem.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1