机译:4种卡林顿旋转的3D AMR SIP–CESE太阳风模型的验证
SIGMA Weather Group, State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100190, China;
SIGMA Weather Group, State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100190, China;
SIGMA Weather Group, State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100190, China;
SIGMA Weather Group, State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100190, China;
SIGMA Weather Group, State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100190, China;
Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntsville, Huntsvi;
Solar wind; Magnetohydrodynamics (MHD); Numerical simulation;
机译:4种卡林顿旋转的3D AMR SIP-CESE太阳风模型的验证
机译:SIP-CESE MHD模型对三种太阳风加热方法的数值验证和比较
机译:通过AMR-CESE-MHD方法模拟太阳风与土星磁层之间的相互作用
机译:太阳风-地面磁层相互作用的大规模3D全球全粒子模拟:IMF旋转对磁层尖端动力学的影响
机译:3D多物种MHD研究未磁化太阳系物体电离层与太阳风或磁层等离子流的相互作用
机译:扩展的MHD建模用于稳定的日冕和太阳风
机译:动力学Alfvén波阻尼引起的太阳风湍流消散模型:与太阳风消散过程的观察结果和含意
机译:Carrington Rotation 2124的全球太阳能自由磁能和电流密度分布。