121 citations · 1.3k across the 60 of their papers we have counts for
60 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…
The fine dynamics in homologous and recurrent jets induced by persistent rising loops and mini-filaments
Hengyuan Wei, Zhenghua Huang, Yadan Duan +1
Jets are common eruptive phenomena in the solar atmosphere which may occur repeatedly. Many studies of their fine dynamics have been conducted. However, the fine dynamics of persis…
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…
Tracking an eruptive prominence using multiwavelength and multiview observations on 2023 March 7
Qingmin Zhang, Yudi Ou, Zhenghua Huang +2
In this paper, we carry out multiwavelength and multiview observations of the prominence eruption, which generates a C2.3 class flare and a coronal mass ejection (CME) on 2023 Marc…
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…
Internal activities in a solar filament and heating to its threads
Hengyuan Wei, Zhenghua Huang, Chuan Li +5
Filaments are one of the most common features in the solar atmosphere, and are of significance in solar, stellar and laboratory plasma physics. Using data from the Chinese H Sol…
Why "solar tsunamis" rarely leave their imprints in the chromosphere
Ruisheng Zheng, Yihan Liu, Wenlong Liu +10
Solar coronal waves frequently appear as bright disturbances that propagate globally from the eruption center in the solar atmosphere, just like the tsunamis in the ocean on Earth.…
The properties of small magnetic flux ropes inside the solar wind come from coronal holes, active regions, and quiet Sun
Changhao Zhai, Hui Fu, Jiachen Si +2
The origination and generation mechanisms of small magnetic flux ropes (SFRs), which are important structures in solar wind, are not clearly known. In present study, 1993 SFRs imme…
Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere
Yuming Wang, Xianyong Bai, Changyong Chen +50
Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360° perspective in the ecliptic plane. It will deploy three 120…
An EUV jet driven by a series of transition region micro-jets
Hengyuan Wei, Zhenghua Huang, Hui Fu +5
Jets are one of the most common eruptive events in the solar atmosphere, and they are believed to be important in the context of coronal heating and solar wind acceleration. We pre…
Monitoring AGNs with H Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars
Dong-Wei Bao, Michael S. Brotherton, Pu Du +42
In this third paper of the series reporting on the reverberation mapping (RM) campaign of active galactic nuclei with asymmetric H emission-line profiles, we present results for…
Statistical properties of Hα jets in the polar coronal hole and their implications in coronal activities
Youqian Qi, Zhenghua Huang, Lidong Xia +6
Dynamic features, such as chromospheric jets, transition region network jets, coronal plumes and coronal jets, are abundant in the network regions of the solar polar coronal holes.…
Dynamics in the transition region beneath active region upflows viewed by IRIS
Zhenghua Huang, Lidong Xia, Hui Fu +2
Coronal upflows at the edges of active regions (AR), which are a possible source of slow solar wind, have been found to connect with dynamics in the transition region. To infer at…
Formation of solar quiescent coronal loops through magnetic reconnection in an emerging active region
Zhenyong Hou, Hui Tian, Hechao Chen +6
Coronal loops are building blocks of solar active regions. However, their formation mechanism is still not well understood. Here we present direct observational evidence for the fo…
Population of Bright Plume Threads in Solar Polar Coronal Holes
Zhenghua Huang, Quanhao Zhang, Lidong Xia +8
Coronal holes are well accepted to be source regions of the fast solar wind. As one of the common structures in coronal holes, coronal plumes might contribute to the origin of the…
Monitoring AGNs with Hβ Asymmetry. II. Reverberation Mapping of Three Seyfert Galaxies Historically Displaying Hβ Profiles with Changing Asymmetry: Mrk 79, NGC 3227, and Mrk 841
Michael S. Brotherton, Pu Du, Ming Xiao +17
We report the results of reverberation mapping three bright Seyfert galaxies, Mrk 79, NGC 3227, and Mrk 841, from a campaign conducted from December 2016 to May 2017 with the Wyomi…