28 citations · 35 across the 12 of their papers we have counts for
12 papers
Statistics of blob properties in two types of coronal streamers
Haiyi Li, Zhenghua Huang, Maria S. Madjarska +4
Previous studies have shown that a streamer blob might originate in the lower corona and thus be affected by activity in that region. While the base of one streamer might differ fr…
Statistics of transition-region loop brightenings and their heating implication
Xiuhui Zuo, Zhenghua Huang, Maria S. Madjarska +4
Transition-region loops are a type of critical magnetic structure in the solar atmosphere, yet their physical properties and evolutionary characteristics remain statistically poorl…
Propagating Kink Waves in Chromospheric Jet-like Structures and Coronal Plumelets
Youqian Qi, Mingzhe Guo, Zhenghua Huang +5
Coronal plumes and chromospheric jet-like structures are believed to be highly dynamic. We report the first direct observations of a propagating kink wave in a chromospheric jet-li…
Enhanced Non-Thermal Line Broadening inside Coronal Cavities above Solar Prominences revealed by Spectral Imaging CoronaGraph
Chenxi Huangfu, Hui Fu, Bo Li +5
Coronal cavities, often associated with prominences, are crucial structures in understanding coronal heating and the eruption mechanism of Coronal Mass Ejections (CMEs). Previous s…
The Influence of Magnetic Complexity of Active Regions on Solar Wind Properties During Solar Cycles 23 and 24
Xinzheng Shi, Hui Fu, Zhenghua Huang +3
Linking solar wind properties to the activities and characteristics of its source regions can enhance our understanding of its origin and generation mechanisms. Using the Mount Wil…
Sequential ejections of plasma blobs due to unbraiding of tangled loops in the solar atmosphere
Xiuhui Zuo, Zhenghua Huang, Hengyuan Wei +8
Nanoflares, which are consequences of braids in tangled magnetic fields, are an important candidate to heat the solar corona to million degrees. However, their observational eviden…
Multi-episodes of remote brightenings driven by a coronal EUV jet on the Sun
Chao Zhang, Zhenghua Huang, Hengyuan Wei +8
Remote brightening (RB) is compact brightening at footpoints of magnetic loops, which are remotely-connecting to and confining an eruption in the solar atmosphere. Here, we report…
The differences in the origination and properties of the near-Earth solar wind between solar cycles 23 and 24
Xinzheng Shi, Hui Fu, Zhenghua Huang +5
The dependence of the sources and properties of the near-Earth solar wind on solar cycle activity is an important issue in solar and space physics. We use the improved two-step map…
Electron densities of Transition Region Loops derived from IRIS O IV spectral data
Shiyu Liang, Ziyuan Wang, Zhenghua Huang +4
Loops are fundamental structures in the magnetized atmosphere of the sun. Their physical properties are crucial for understanding the nature of the solar atmosphere. Transition reg…
Formation of a streamer blob via the merger of multiple plasma clumps below 2Rs
Haiyi Li, Zhenghua Huang, Kaiwen Deng +7
Context. Propagating streamer blobs could be an important source of disturbances in the solar wind. Direct observations on formation of streamer blobs could be a proxy for understa…
The contribution and FIP bias of three types of materials inside ICMEs associated with different flare intensities
Hui Fu, Xinzheng Shi, Zhenghua Huang +2
The studies on the origination and generation mechanisms of ICME materials are crucial for understanding the connection between CMEs and flares. The materials inside ICMEs can be c…
Eruptions from quiet Sun coronal bright points. I. Observations
Chauzhou Mou, Maria S. Madjarska, Klaus Galsgaard +1
Observations of the full lifetime of CBPs in data taken with the AIA on board SDO in four passbands, He II 304 A, Fe IX/X 171 A, Fe XII 193 A, and Fe XVIII 94 A are investigated fo…