机译:单分量风速在Rankine-Hugoniot分析行星际冲击中的应用
Department of Chemical Engineering, University of New Hampshire, Durham, New Hampshire, USA.;
Space Science Center, Institute for the Study of Earth, Oceans, and Space, Physics Department, University of New Hampshire, Durham, New Hampshire, USA.;
Space Science Center, Institute for the Study of Earth, Oceans, and Space, Physics Department, University of New Hampshire, Durham, New Hampshire, USA.;
Department of Physics and Astronomy, University of Leicester, Leicester, UK.;
CSPAR, University of Alabama in Huntsville, Huntsville, Alabama, USA.;
Code 672, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.;
Los Alamos National Laboratory, Los Alamos, New Mexico, USA.;
Space Radiation Laboratory, California Institute of Technology, Pasadena, California, USA.;
Space Radiation Laboratory, California Institute of Technology, Pasadena, California, USA.;
Space Environment Research Center, Kyushu University, Fukuoka, Japan.;
Electric shock; Wind speed; Uncertainty; Interplanetary; Magnetic fields;
机译:改装的“Rankine-Hugoniot”震动拟合技术:同时解决冲击正常和速度
机译:行星际激波相互作用和演化对“背景”太阳风速的影响
机译:行星际同向相互作用区域(CIR)和高速太阳风流期间的极地夏季中层极端水平漂移速度:太阳风与中层层之间的耦合
机译:太阳风中的弓箭冲击:了解普通震荡的课程
机译:使用WINDMI模型研究行星际冲击,地磁风暴和亚风暴。
机译:Fisher-Shannon高频城市风速时间序列的复杂性分析
机译:单分量风速在Rankine-Hugoniot分析行星际冲击中的应用