机译:活动区域和日冕孔的磁性拓扑:对日冕流出和太阳风的影响
Mullard Space Science Laboratory, University College London, Dorking, UK;
Mullard Space Science Laboratory, University College London, Dorking, UK;
Mullard Space Science Laboratory, University College London, Dorking, UK;
Observatoire de Paris, LESIA, CNRS, UPMC Univ. Paris 06, Univ. Paris-Diderot, Meudon, France;
Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC. 67, Suc. 28, 1428, Buenos Aires, Argentina;
Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, 94304, USA;
College of Science, George Mason University, Fairfax, VA, 22030, USA;
Space Science Division, Naval Research Laboratory, Washington, DC, 20375, USA;
College of Science, George Mason University, Fairfax, VA, 22030, USA;
Active regions; Magnetic field; Magnetic extrapolations; Solar wind;
机译:活动区域和日冕孔的磁拓扑:对日冕流出和太阳风的影响
机译:低纬度冠状孔,衰变活跃区域和全球冠状磁结构
机译:安静区域和日冕孔中太阳日冕羽的临界磁场强度?
机译:冠状孔和有源区边界在太阳风力形成中的作用
机译:磁流体动力学冲击加热和日冕孔处的太阳风加速。
机译:ACE和STEREO卫星在黄道上测得的高速太阳风的峰值速度对其太阳源日冕孔的面积和共度的依赖性
机译:有源区和冠状孔的磁拓扑:对冠状空流和太阳风的影响
机译:太阳活动区演化对太阳风流,冠状孔边界和地磁暴的影响