Acceleration of solar wind particles due to inertial Alfvén waves

作     者：Kiran Batool Imran A Khan M Shamir Abdul Kabir S Ayaz Kiran Batool;Imran A Khan;M Shamir;Abdul Kabir;S Ayaz

作者机构：Theoretical Physics DepartmentNational Centre for PhysicsIslamabad 44000Pakistan Department of Space SciencesInstitute of Space TechnologyIslamabad 44000Pakistan Space and Astrophysics Research Lab(SARL)National Center of GIS and Space Applications(NCGSA)Islamabad 44000Pakistan Salam ChairDepartment of PhysicsGC University LahoreKatchery RoadLahorePunjab 54000Pakistan Department of Space Science and CSPARUniversity of Alabama in HuntsvilleHuntsvilleAL 35899United States of America 

出 版 物：《Communications in Theoretical Physics》 (理论物理通讯（英文版）)

年 卷 期：2024年第76卷第6期

页      面：137-141页

核心收录：

学科分类：070802[理学-空间物理学] 07[理学] 08[工学] 0708[理学-地球物理学] 0825[工学-航空宇航科学与技术] 

主　　题：solar wind inertial Alfven waves resonant particles 

摘      要：Gaining an understanding of the effects and dynamics of the solar wind is crucial for the study of space weather,Earth s magnetosphere,spacecraft protection,the dynamics of the Solar System,and various other *** show that Alfvén waves effectively transfer energy to resonant *** study demonstrates how inertial Alfvén waves deliver their energy to resonant plasma particles in different solar environments under certain *** analysis shows that inertial Alfvén waves experience more rapid damping with increasing parallel wavenumber,ambient magnetic field strength,and particle number density,coupled with a decrease in *** rate of energy transfer to resonant particles intensifies with higher temperatures and reduced parallel wavenumber and particle number *** with higher initial velocities actively participate in Landau damping,especially in regions with a stronger ambient magnetic field.