100 citations · 508 across the 20 of their papers we have counts for
20 papers
The Deep Learning-Based Dual-Branch Multimodal Fusion Model for Solar Flare Prediction
Limin Zhao, Xingyao Chen, Xiaoshuai Zhu +2
Solar flares are intense eruptive events caused by the rapid release of magnetic energy, often impacting Earth's space environment through electromagnetic radiation and high-energy…
Change ratios of magnetic helicity and magnetic free energy during major solar flares
Quan Wang, Mei Zhang, Shangbin Yang +2
Magnetic helicity is an important concept in solar physics, with a number of theoretical statements pointing out the important role of magnetic helicity in solar flares and coronal…
Magnetic field extrapolation in active region well comparable with observations in multiple layers
Fu Yu, Jie Zhao, Yang Su +4
Magnetic field extrapolation is a fundamental tool to reconstruct the three-dimensional magnetic field above the solar photosphere. However, the prevalently used force-free field m…
Magnetohydrostatic Modeling of the Solar Atmosphere
Xiaoshuai Zhu, Thomas Neukirch, Thomas Wiegelmann
Understanding structures and evolutions of the magnetic fields and plasma in multiple layers on the Sun is very important. A force-free magnetic field which is an accurate approxim…
Toward a fast and consistent approach to model solar magnetic fields in multiple layers
Xiaoshuai Zhu, Thomas Wiegelmann
Aims. We aim to develop a fast and consistent extrapolation method to model multiple layers of the solar atmosphere. Methods. The new approach combines the magnetohydrostatic (MHS)…
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…
Preprocessing of vector magnetograms for magnetohydrostatic extrapolations
Xiaoshuai Zhu, Thomas Wiegelmann, Bernd Inhester
Context. Understanding the 3D magnetic field as well as the plasma in the chromosphere and transition region is important. One way is to extrapolate the magnetic field and plasma f…
The high helium abundance and charge states of the interplanetary CME and its material source on the Sun
Hui Fu, R. A. Harrison, J. A. Davies +5
Identifying the source of the material within coronal mass ejections (CMEs) and understanding CME onset mechanisms are fundamental issues in solar and space physics. Parameters rel…
Magnetohydrostatic modeling of AR11768 based on a SUNRISE/IMaX vector magnetogram
Xiaoshuai Zhu, Thomas Wiegelmann, Sami Solanki
Context. High resolution magnetic field measurements are routinely done only in the solar photosphere. Higher layers like the chromosphere and corona can be modeled by extrapolatin…
A White-light Flare Powered by Magnetic Reconnection in the Lower Solar Atmosphere
Yongliang Song, Hui Tian, Xiaoshuai Zhu +3
White-light flares (WLFs), first observed in 1859, refer to a type of solar flares showing an obvious enhancement of the visible continuum emission. This type of enhancement often…
Test magnetohydrostatic extrapolation with radiative MHD simulation of a solar flare
Xiaoshuai Zhu, Thomas Wiegelmann
Context. On the sun, the magnetic field vector is measured routinely only in the photosphere. By using these photospheric measurements as boundary condition, we developed the magne…
Solar Ultraviolet Bursts in a Coordinated Observation of IRIS, Hinode and SDO
Yajie Chen, Hui Tian, Xiaoshuai Zhu +3
Solar ultraviolet (UV) bursts are small-scale compact brightenings in transition region images. The spectral profiles of transition region lines in these bursts are significantly e…
Generalisation of the Magnetic Field Configuration of typical and atypical Confined Flares
Navin Chandra Joshi, Xiaoshuai Zhu, Brigitte Schmieder +6
Atypical flares cannot be naturally explained with standard models. To predict such flares, we need to define their physical characteristics, in particular, their magnetic environm…
On the extrapolation of magneto-hydro-static equilibria on the sun
Xiaoshuai Zhu, Thomas Wiegelmann
Modeling the interface region between solar photosphere and corona is challenging, because the relative importance of magnetic and plasma forces change by several orders of magnitu…
Magnetic reconnection at the earliest stage of solar flux emergence
Hui Tian, Xiaoshuai Zhu, Hardi Peter +3
On 2016 September 20, the Interface Region Imaging Spectrograph observed an active region during its earliest emerging phase for almost 7 hours. The Helioseismic and Magnetic Image…
Observations of a white-light flare associated with a filament eruption
Y. L. Song, Y. Guo, H. Tian +3
We present observations of an M5.7 white-light flare (WLF) associated with a small filament eruption in NOAA active region 11476 on 2012 May 10. During this flare, a circular flare…
Block-induced complex structures building the flare-productive solar active region 12673
Shuhong Yang, Jun Zhang, Xiaoshuai Zhu +1
Solar active region (AR) 12673 produced 4 X-class, 27 M-class, and numerous lower class flares during its passage across the visible solar disk in September 2017. Our study is to a…
A solar blowout jet caused by the eruption of a magnetic flux rope
Xiaoshuai Zhu, Huaning Wang, Xin Cheng +1
We investigate the three-dimensional (3D) magnetic structure of a blowout jet originated in the west edge of NOAA Active Region (AR) 11513 on 02 July 2012 by means of recently deve…
Observational Evidence of Magnetic Reconnection for Brightenings and Transition Region Arcades in IRIS observations
Jie Zhao, Brigitte Schmieder, Hui Li +4
By using a new method of forced-field extrapolation, we study the emerging flux region AR 11850 observed by the Interface Region Imaging Spectrograph (IRIS) and Solar Dynamical Obs…
Forced field extrapolation of the magnetic structure of the Halpha fibrils in solar chromosphere
Xiaoshuai Zhu, Huaning Wang, Zhanle Du +1
We present a careful assess of the forced field extrapolation using Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) magnetogram. The convergence property is c…