supported by the National Natural Science Foundation of China(Grant Nos.40890161 and 40674081);the CAS Project KJCX2-YW-T04,and the National Basic Research Program of China(Grant No.G2006CB806303)
Solar coronal loops show significant plasma motions during their formation and eruption stages. Dynamic cool coronal structures, on the other hand, are often observed to propagate along coronal loops. We report on the...
Supported by the National Natural Science Foundation of China (Grant Nos. G10873020, 10603008, 40890161, 10703020, 40674081, and10703007);the CAS Project (Grant No. KJCX2-YW-T04);the National Basic Research Program of China (Grant No. G2006CB806303)
We examine chromospheric oscillations in both a coronal hole (CH) and a quiet Sun (QS) region, by employing Transition Region and Coronal Explorer (TRACE) and Big Bear Solar Observatory (BBSO) data on September 14 and...
Supported by the National Natural Science Foundation of China (Grant Nos. G10703007, 40890161, 10603008, 40674081, and 10733020);the CAS Project (Grant No. KJCX2-YW-T04);the National Basic Research Program of China (Grant No. G2006CB806303)
After examining the data observed by TRACE 171 and 195 from May 1998 to December 2006, we choose as our sample 190 (39 X-class and 151 M-class) flare events which display post-flare loops (PFLs). We investigate the...
supported by the National Natural Science Foundation of China (10873020, 10703007, G10573025, 40674081, 10603008, 10733020 and 40890161);the Chinese Academy of Sciences Project KJCX2-YW-T04;the National Basic Research Program of China(G2006CB806303)
From the observed vector magnetic fields by the Solar Optical Telescope/ Spectro-Polarimeter aboard the satellite Hinode, we have examined whether or not the quiet Sun magnetic fields are non-potential, and how the G-...
supported by the National Natural Science Foundations of China (Nos. 10573025,40674081 and 40890161);the CAS Project KJCX2-YW-T04;the National Basic Research Program of China under grant G2006CB806303
With the polarimetric observations obtained by the Spectro-Polarimeter on board Hinode, we study the relationship between granular development and magnetic field evolution in the quiet Sun. Six typical cases are displ...
supported by the National Natural Science Foundation of China (10873020,10703007,G10573025, 40674081and 10603008);the CAS Project KJCX2-YW-T04;the National Basic Research Program of China (G2006CB806303)
Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two q...