207 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN179 papers
- National Astronomical ObservatoriesCN175 papers
- University of Chinese Academy of SciencesCN55 papers
- Yunnan ObservatoriesCN32 papers
- Purple Mountain ObservatoryCN22 papers
- Max Planck Institute for Solar System ResearchDE16 papers
- Shandong UniversityCN14 papers
- Nanjing UniversityCN12 papers
- State Key Laboratory of Space Weather10 papers
- Institute of Solar-Terrestrial PhysicsRU9 papers
- Kunming University of Science and TechnologyCN9 papers
- Russian Academy of SciencesRU7 papers
15 papers · 2 filters
Cusp-shaped structure of a jet observed by IRIS and SDO
Zhang Yuzong, Zhang Jun
On 29 August 2014, the trigger and evolution of a cusp-shaped jet were captured in detail at 1330 Å by the Interface Region Imaging Spectrograph.At first, two neighboring mini-prom…
Magnetic Helicity Reversals in a Cyclic Convective Dynamo
Mark S. Miesch, Mei Zhang, Kyle C. Augustson
We investigate the role of magnetic helicity in promoting cyclic magnetic activity in a global, 3D, magnetohydrodynamic (MHD) simulation of a convective dynamo. This simulation is…
Magnetic reconnection between a solar filament and nearby coronal loops
Leping Li, Jun Zhang, Hardi Peter +5
Magnetic reconnection, the rearrangement of magnetic field topology, is a fundamental physical process in magnetized plasma systems all over the universe1,2. Its process is difficu…
Explosive Chromospheric Evaporation in a Circular-ribbon Flare
Q. M. Zhang, D. Li, Z. J. Ning +3
In this paper, we report our multiwavelength observations of the C4.2 circular-ribbon flare in active region (AR) 12434 on 2015 October 16. The short-lived flare was associated wit…
Automatic Recognition of Sunspots in HSOS Full-Disk Solar Images
Cui Zhao, GangHua Lin, YuanYong Deng +1
A procedure is introduced to recognise sunspots automatically in solar full-disk photosphere images obtained from Huairou Solar Observing Station, National Astronomical Observatori…
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…
On the relationship between sunspot structure and magnetic field changes associated with solar flares
Yongliang Song, Mei Zhang
Many previous studies have shown that magnetic fields as well as sunspot structures present rapid and irreversible changes associated with solar flares. In this paper we first use…
Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms
M. Dasi-Espuig, J. Jiang, N. A. Krivova +3
We present a reconstruction of the spectral solar irradiance since 1700 using the SATIRE-T2 (Spectral And Total Irradiance REconstructions for the Telescope era version 2) model. T…
Light Walls Around Sunspots Observed by the Interface Region Imaging Spectrograph
Y. J. Hou, T. Li, S. H. Yang +1
The Interface Region Imaging Spectrograph (IRIS) mission provides high-resolution observations of the chromosphere and transition region. We try to determine whether the light wall…
On the relationship between G-band bright point dynamics and their magnetic field strengths
Yunfei Yang, Qiang Li, Kaifan Ji +4
G-band bright points (GBPs) are regarded as good manifestations of magnetic flux concentrations. We aim to investigate the relationship between the dynamic properties of GBPs and t…
Subarcsecond Bright Points and Quasi-periodic Upflows Below a Quiescent Filament Observed by the IRIS
Ting Li, Jun Zhang
Using UV spectra and SJIs from the IRIS, and coronal images and magnetograms from the Solar Dynamics Observatory (SDO), we present the new features in a quiescent filament channel:…
Oscillation of Newly Formed Loops After Magnetic Reconnection in the Solar Chromosphere
Shuhong Yang, Yongyuan Xiang
With the high spatial and temporal resolution H images from the New Vacuum Solar Telescope, we focus on two groups of loops with a X-shaped configuration in the dynamic chromosp…
Activity Analyses for Solar-Type Stars Observed With Kepler. I. Proxies of Magnetic Activity
Han He, Huaning Wang, Duo Yun
Light curves of solar-type stars often show gradual fluctuations due to rotational modulation by magnetic features (starspots and faculae) on stellar surfaces. Two quantitative mea…
Tether-cutting Reconnection between Two Solar Filaments Triggering Outflows and a Coronal Mass Ejection
Huadong Chen, Jun Zhang, Leping Li +1
Triggering mechanisms of solar eruptions have long been a challenge. A few previous case studies have indicated that preceding gentle filament merging via magnetic reconnection may…
Microwave Type III Pair Bursts in Solar Flares
Baolin Tan, Hana Meszarosova, Marian Karlicky +2
Solar microwave type III pair burst is composed of normal and reverse-sloped (RS) burst branches with oppositely fast frequency drifts. It is the most sensitive signature of the pr…