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机译:行星际CMEs及其太阳源区域的螺旋征比较
Korea Astronomy and Space Science Institute">(1);
NASA Goddard Space Flight Center">(2);
Department of Physics The Catholic University of America">(3);
Korea Astronomy and Space Science Institute">(1);
Korea Astronomy and Space Science Institute">(1);
NASA Goddard Space Flight Center">(2);
NASA Goddard Space Flight Center">(2);
Department of Physics The Catholic University of America">(3);
NASA Goddard Space Flight Center">(2);
Department of Physics The Catholic University of America">(3);
NASA Goddard Space Flight Center">(2);
Department of Physics The Catholic University of America">(3);
Big Bear Solar Observatory New Jersey Institute of Technology">(4);
Coronal mass ejections; Magnetic cloud; Photospheric helicity; Solar surface magnetic field; Interplanetary magnetic field;
机译:行星际CME及其太阳源区域的螺旋征比较
机译:太阳源地区螺旋藻注射的两种特征演化模式相关的CMEs的发生和速度
机译:在太阳周期23中CME和ICME与其他太阳和行星际参数的变化比较
机译:太阳风的流结构和冠状源比较了1997年4月12日哈洛CMES
机译:太阳活动区的磁螺旋关系及其与太阳爆发的关系研究
机译:行星际磁云的太阳源导致螺旋度预测
机译:CmEs的发生和速度与太阳能源区螺旋注射的两种特征演化模式有关