supported by the National Natural Science Foundation of China (40825014, 40890162, 41028004 and 41274175);the National Basic Research Program of China (2012CB825601)
In this article I present a review of recent studies on coronal dynamics, including research progresses on the physics of coronal streamers that are the largest structure in the corona, physics of coronal mass ejectio...
supported by the National Natural Science Foundation of China(40904047,40825014,40890162 and 40974105);the Specialized Research Fund for State Key Laboratories
At present it remains to address why the fast solar wind is fast and the slow wind is slow.Recently we have shown that the field line curvature may substantially influence the wind speed v,thereby offering an explanat...
supported by the National Natural Science Foundation of China(Grant Nos.11103090,11025315,40890161,10921303,40825014, and 40890162);the CAS project KJCX2-YW-T04,the National Basic Research Program of China (973 Program,No.2011CB811403);the Shandong Provincial Natural Science Foundation, China(ZR 2011AQ009)
Using the multi-wavelength data from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) spacecraft, we study a jet occurring in a coronal hole near the northern pole of the Sun. Th...