The siphonic energy transfer between hot solar wind and cold martian ionosphere through open magnetic flux rope  

作　　者：Xiaojun Xu Lou-Chuang Lee Qi Xu Qing Chang Jing Wang Ming Wang Shaosui Xu Christian Mosti Charles J.Farrugia Xing Wang Yudong Ye Zilu Zhou Lei Luo Peishan He Shaoguan Cheng 

机构地区：[1]State Key Laboratory of Lunar and Planetary Sciences,Macao University of Science and Technology,Macao 999078,China [2]CNSA Macao Center for Space Exploration and Science,Macao 999078,China [3]Institute of Earth Science,Academia Sinica,Taipei 115029,China [4]Institute of Space Science and Applied Technology,Harbin Institute of Technology,Shenzhen 518000,China [5]Planetary Environmental and Astrobiological Research Laboratory(PEARL),School of Atmospheric Sciences,Sun Yat-sen University,Zhuhai 519000,China [6]Nanjing University of Information Science and Technology,Nanjing 210000,China [7]Space ScienceLaboratory,Universityof California,BerkeleyCA94320,USA [8]Space Research Institute,Austrian Academy of Sciences,Graz 8010,Austria [9]University of New Hampshire,NH 03824,USA

出　　处：《Fundamental Research》2024年第4期882-889,共8页自然科学基础研究（英文版）

基　　金：National Natural Science Foundation of China(42122061);the Science and Technology Development Fund of Macao SAR(0002/2019/A1);Macao Foundation,and the pre-research project on Civil Aerospace Technologies No.D020308 and D020104 funded by China National Space Administration.C.M.thanks the Austrian Science Fund(FWF):P31521-N27.C.J.F.thanks NASA grant:80NSSC19K1293.A basic version of the Grad-Shafranov reconstruction method in Matlab is available at https://github.com/cmoestl/interplanetarygrad-shafranov.We acknowledge the MAVEN contract for support.All MAVEN data are available on the Planetary Data System(https://pds.nasa.gov).

摘　　要：A mechanism for energy transfer from the solar wind to the Martian ionosphere through open magnetic flux rope is proposed based on the observations by Mars Atmosphere and Volatile EvolutioN(MAVEN).The satellite was located in the dayside magnetosheath at an altitude of about 70o km above the northern hemisphere.Collisions between the hot solar wind protons and the cold heavy ions/neutrals in the subsolar region can cool the protons and heat the heavy ions.As a result,the magnetosheath protons are siphoned into the ionosphere due to the thermal pressure gradient of protons and the heated heavy ions escape along the open magnetic field lines.Although direct collisions in the lower-altitude region were not detected,this physical process is demonstrated by MAVEN measurements of enhanced proton density,decreased proton temperature and oppositely directed motions of hot and cool protons within the flux rope,which are very different from the observational features of the flux transfer events near the Earth's magnetopause.This mechanism could universally exist in many contexts where a collisionless plasma region is connected to a collisional plasma region.By reconstructing the magnetic geometry and the cross-section of the flux rope using the Grad-Shafranov technique,the ion loss rates are quantitatively estimated to be on the order of 1023 s-l,which is much higher than previously estimated.

关 键 词：MARS Flux rope Solarwind IONOSPHERE Ion loss 

分 类 号：O57[理学—粒子物理与原子核物理]