supported by the National Natural Science Foundation of China(Grant Nos.41174148,41222032,40931055,41231069,41274172);supported by a foundation for the Author of National Excellent Doctoral Dissertation of China(FANEDD)(Grant No.201128)
Using observations from the EUV Imaging Spectrometer (EIS) onboard Hinode, we exam the plasma dynamics around the edge of the active region 10977, possibly associated with the source of nascent slow/intermediate sol...
supported by the Fundamental Research Funds for the Central Universities(2011YYL127);supported by the National Natural Science Foundation of China(40874090,40931055 and 40890162)
This work detects multi-scale, from hour to seconds, pressure-balanced structures (PBSs) in the solar wind based on the anti- correlation between the plasma thermal pressure and the magnetic pressure measured by WIND ...
supported by the National Natural Science Foundation of China (Grant Nos.40874090 and 40931055)
Persistent outflows have recently been detected at the boundaries of some active regions. Although these outflows are suggested to be possible sources of the slow solar wind, the nature of these outflows is poorly und...