...
机译:水星磁致绝经期传播的开尔文-亥姆霍兹涡的重建
Space and Plasma Physics, School of Electrical Engineering, Royal Institute of Technology (KTH), Stockholm, Sweden;
Heliophysics Science Division, NASA Goddard Space Flight Center, Creenbelt, MD 20771, USA,Goddard Earth Sciences and Technology Center, University of Maryland, Baltimore County, Baltimore, MD 21228, USA;
Heliophysics Science Division, NASA Goddard Space Flight Center, Creenbelt, MD 20771, USA;
Space and Plasma Physics, School of Electrical Engineering, Royal Institute of Technology (KTH), Stockholm, Sweden;
Space and Plasma Physics, School of Electrical Engineering, Royal Institute of Technology (KTH), Stockholm, Sweden, Center for Space Sciences, University of Texas at Dallas, Richardson, TX 75083, USA;
Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 200)5, USA;
The Johns Hopkins University Applied Physics Laboratory, Laurel MD 20723, USA;
The Johns Hopkins University Applied Physics Laboratory, Laurel MD 20723, USA;
mercury; kelvin-helmholtz; magnetopause; MESSENGER;
机译:在土星的磁档边界上识别Active Kelvin-Helmholtz漩涡
机译:在地球的磁寄博的Kelvin-Helmholtz涡旋中产生湍流:磁体多尺度观察
机译:血浆传输到Kelvin-Helmholtz涡流引起的昏昏欲睡的磁档,以响应主题观察到的行星际磁场向北转动
机译:环境参数对磁性迁移的赫尔文 - 亥姆霍兹不稳定性的影响
机译:磁风的太阳风开尔文-赫尔默兹不稳定和地磁活动的年代际变化。
机译:水银磁层磁场的模块模型被限制在平均观测到的绝经中
机译:在水星的磁更年期传播的开尔文-亥姆霍兹涡流的重建