地球与行星物理论评（中英文）2025，Vol.56Issue(4)：407-420,14.DOI:10.19975/j.dqyxx.2024-048
火星与金星弓激波和磁堆积边界研究进展
Review of boundary model studies in the Venusian and Martian induced magnetosphere
摘要
Abstract
Although Venus and Mars do not have a global magnetic field but have atmospheres and iono-spheres.During their coupling with the solar wind,the induced magnetospheres are created,as well as the bounda-ries of the bow shock and the magnetic pileup boundary.These boundaries not only reflect the upstream solar wind conditions but also reveal the state of the planetary space environment.Hence,on the one hand,the modeling of these boundaries can help to understand the basic process of solar wind-planet space interaction.On the other hand,these boundary models can also provide more accurate data on the location of the boundaries for planetary explora-tion and lay a theoretical foundation for China's"Tianwen-1"program and the corresponding deep space explora-tions.In addition,these boundary model studies also give important insights into the evolution and development of Earth-like planets.It is shown that the dynamic pressure of the solar wind,the interplanetary magnetic field,the crustal magnetic field,and the solar extreme ultraviolet radiation are all key factors affecting the location of the Martian magnetic pileup boundary,and thus they also affect the shape and size of the Martian bow shock.In addi-tion,the effect of magnetosonic Mach number on the Martian bow shock cannot be neglected.As for the Venusian bow shock,the magnetosonic Mach number is the main controlling factor.Based on the results of the influence of the above parameters,scientists have established relevant boundary models.In this paper,we review the research progress on the Venusian and Martian bow shock and magnetic pileup boundary models,providing reference for planetary science research and deep space exploration.关键词
火星/金星/感应磁层/弓激波/磁堆积边界Key words
Mars/Venus/induced magnetosphere/bow shock/magnetic pileup boundary分类
地球科学引用本文复制引用
张佳琪,王明,眭昊旸,管子健,李劲羽,杜可涵,吕建永..火星与金星弓激波和磁堆积边界研究进展[J].地球与行星物理论评（中英文）,2025,56(4):407-420,14.基金项目
国家自然科学基金资助项目(42441824,42074195) Supported by the National Natural Science Foundation of China(Grant Nos.42441824,42074195) （42441824,42074195）
