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太阳爆发与空间天气研究进展OA

Solar Eruption and Space Weather

中文摘要英文摘要

太阳爆发活动(主要包括耀斑与日冕物质抛射)是太阳系内规模最大的瞬态能量释放过程,也是驱动灾害性空间天气的物理源头.以"太阳源区触发-行星际传输演化-近地空间响应"这一完整的因果链条为主线,系统评述该领域的研究现状与范式演进.在源区触发阶段,重点综述磁重联作为终极引擎的确立过程,以及磁通量绳从理论争议到多波段成像确证的跨越,并剖析理想磁流体不稳定性与非理想磁重联在灾变起始中的动力学博弈.在行星际传输阶段,阐述日冕物质抛射与动态、磁化太阳风环境的复杂相互作用,分析背景太阳风的动力学阻曳效应以及最新发现的磁场折返等微观结构对行星际媒介认知的重塑,并详述激波驱动的高能粒子加速机制与扩散路径模型.在近地响应阶段,系统论述爆发能量在地球磁层、热层及电离层中的层级耗散与耦合机制,解析南向磁场触发的能量注入路径,以及由此引发的热层径向膨胀、电离层不均匀体闪烁和地磁感应电流等物理过程.结合近年典型灾害空间天气案例,揭示现代技术文明在空间环境演变面前的系统性脆弱.针对预报瓶颈,梳理从经验统计到物理驱动数值模型,再到人工智能全链条数字孪生的范式更迭,并展望通过立体探测网构建日地全景数字孪生预报体系的科学蓝图.

Solar eruptive activities,primarily manifested as solar flares and coronal mass ejections,represent the transient energy release processes on the largest scale in the solar system and serve as the physical sources of hazardous space weather.Guided by the integral causal chain of"solar source triggering interplanetary transport and evolution-near Earth geospace response",this paper systematically reviews the current research status and the paradigmatic evolution in this field.In the solar source triggering stage,we focus on the establishment of magnetic reconnection as the ultimate engine and the transition of magnetic flux ropes from theoretical controversy to multi-wavelength imaging confirmation,while analyzing the dynamical interplay between ideal magnetohydrodynamic instabilities and non-ideal magnetic reconnection in the onset of eruptions.Regarding interplanetary transport,the paper elucidates the complex interactions between CMEs and the dynamic,magnetized solar wind environment.It analyzes the aerodynamic drag effects of the background solar wind and how recent discoveries of microstructures,such as magnetic switchbacks,have reshaped our under-standing of the structured interplanetary medium.Furthermore,the physical mechanisms of shock-driven energetic particle accelera-tion and diffusion path models are detailed.In the near-Earth response stage,the paper systematically discusses the hierarchical dissi-pation and coupling mechanisms of eruptive energy within the Earth's magnetosphere,thermosphere,and ionosphere.It resolves the energy injection pathways triggered by southward magnetic fields and the subsequent physical processes,including radial thermo-spheric expansion,ionospheric scintillation caused by plasma inhomogeneities,and the generation of geomagnetically induced cur-rents.By integrating typical hazardous space weather cases from recent years,the review reveals the systemic vulnerability of modern technological civilization to space environment variations.Addressing forecasting bottlenecks,the review outlines the paradigmatic shift from empirical statistics to physics-driven numerical models and then to AI-based full-chain digital twins,while envisioning a sci-entific blueprint for constructing a Sun-Earth panoramic digital twin forecasting system leveraging stereoscopic observation networks.

申远灯;谭宋;欧雨迪

哈尔滨工业大学(深圳)空天科技学院 太阳活动与空间天气全国重点实验室,广东 深圳 518055波茨坦莱布尼茨天体物理研究所,德国 波茨坦 14482哈尔滨工业大学(深圳)空天科技学院 太阳活动与空间天气全国重点实验室,广东 深圳 518055

天文与地球科学

太阳爆发空间天气日冕物质抛射磁重联数字孪生

solar eruptionspace weathercoronal mass ejectionmagnetic reconnectiondigital twin

《四川师范大学学报(自然科学版)》 2026 (3)

388-412,25

国家自然科学基金(12573059和12173083)

10.3969/j.issn.1001-8395.2026.03.009

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