74 citations · 226 across the 7 of their papers we have counts for
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Ultra-high-resolution Observations of Persistent Null-point Reconnection in the Solar Corona
X. Cheng, E. R. Priest, H. T. Li +21
Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime possibility to heat the low corona to millions of degrees. Here, we present ultra-high-reso…
Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes
J. H. Guo, Y. W. Ni, Y. H. Zhou +3
Many prominences are supported by magnetic flux ropes. One important question is how we can determine whether the flux rope is weakly-twisted or strongly-twisted. In this paper, we…
Quantifying the Magnetic Structure of a Coronal Shock Producing a Type II Radio Burst
W. Su, T. M. Li, X. Cheng +9
Type II radio bursts are thought to be produced by shock waves in the solar atmosphere. However, what magnetic conditions are needed for the generation of type II radio bursts is s…
Magnetic Twists of Solar Filaments
Jinhan Guo, Yiwei Ni, Ye Qiu +3
Solar filaments are cold and dense materials situated in magnetic dips, which show distinct radiation characteristics compared to the surrounding coronal plasma. They are associate…
Period Increase and Amplitude Distribution of Kink Oscillation of Coronal Loop
W. Su, Y. Guo, R. Erdélyi +4
Coronal loops exist ubiquitously in the solar atmosphere. These loops puzzle astronomers over half a century. Solar magneto-seismology (SMS) provides a unique way to constrain the…
Multiwavelength observations of a partially eruptive filament on 2011 September 8
Q. M. Zhang, Z. J. Ning, Y. Guo +5
In this paper, we report our multiwavelength observations of a partial filament eruption event in NOAA active region 11283 on 2011 September 8. A magnetic null point and the corres…