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
46 papers · 1 filter
Solar jet-like features rooted in flare ribbons
Xiaohong Li, Jun Zhang, Shuhong Yang +1
Employing the high spatio-temporal Interface Region Imaging Spectrograph 1330 Å observations, we investigated the jet-like features that occurred during the X8.2 class flare in NOA…
A secondary fan-spine magnetic structure in active region 11897
Yijun Hou, Ting Li, Shuhong Yang +1
Fan-spine is a special topology in solar atmosphere and is closely related to magnetic null point as well as circular-ribbon flares, which can provide important information for und…
Imaging observations of chromospheric evaporation in a circular-ribbon flare
Q. M. Zhang, D. Li, Y. Huang
In this paper, we report our multiwavelength imaging observations of chromospheric evaporation in a C5.5 circular-ribbon flare (CRF) on 2014 August 24. The flare was observed by th…
A giant dark channel across the solar equator consisting of two filament channels with different chiralities
Zhiping Song, Yijun Hou, Jun Zhang
Solar filaments are the largest magnetic structure that can be physically traced to the chromosphere. The structure and evolution of solar filaments are important for our understan…
Non-equilibrium Ionization Effects on Extreme-Ultraviolet Emissions Modulated by Standing Sausage Modes in Coronal Loops
Mijie Shi, Bo Li, Tom Van Doorsselaere +2
Forward-modeling the emission properties in various passbands is important for confidently identifying magnetohydrodynamic waves in the structured solar corona. We examine how Non-…
Subarcsecond blobs in flare-related coronal jets
Q. M. Zhang, L. Ni
In this paper, we report our multiwavelength observations of subarcsecond blobs in coronal jets. In AR 12149, a C5.5 circular-ribbon flare occurred on 2014 August 24. Two jets (jet…
Current sheets in the wake of an eruption of two crossing filaments
Jun Dai, Jiayan Yang, Leping Li +1
Employing Solar Dynamic Observatory/Atmosphertic Imaging Assembly (AIA) multi-wavelength images, we study an eruption of two crossing filaments, and firstly report the current shee…
On Midrange Periodicities in Solar Radio Flux and Sunspot Areas
Ying Mei, Hui Deng, Feng Wang
Using the Hilbert-Huang transform technique, we investigate the midrange periodicities in solar radio flux at 2800 MHz (F10.7) and sunspot areas (SAs) from February 1, 1947 to Sept…
Signatures of magnetic reconnection at the footpoints of fan shape jets on a light bridge driven by photospheric convective motions
Xianyong Bai, Hector Socas-Navarro, Daniel Nóbrega-Siverio +5
Dynamical jets are generally found on Light bridges (LBs), which are key to studying sunspots decays. So far, their formation mechanism is not fully understood. In this paper, we u…
Three-dimensional Magnetic Reconnection Triggering an X-class Confined Flare in Active Region 12192
Ting Li, Yijun Hou, Shuhong Yang +1
We present an extensive analysis of the X2.0-class confined flare on 2014 October 27 in the great active region AR 12192, observed by the \emph{Interface Region Imaging Spectrograp…
Transition-region explosive events produced by plasmoid instability
Dong Li
Magnetic reconnection is thought to be a key process in most of solar eruptions. Thanks to high-resolution observations and simulations, the studied scale of reconnection process h…
Quasi-periodic Fast Propagating Magnetoacoustic Waves during the Magnetic Reconnection Between Solar Coronal Loops
Leping Li, Jun Zhang, Peter Hardi +5
Employing Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA) multi-wavelength images, we have presented coronal condensations caused by magnetic reconnection between a s…
Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters
Tanda Li, Timothy R. Bedding, Hans Kjeldsen +3
We model the oscillations of the SONG target Herculis to estimate the parameters of the star. The = 1 mixed modes of Her provide strong constraints on stellar proper…
Onset of secondary instabilities and plasma heating during magnetic reconnection in strongly magnetized regions of the low solar atmosphere
Lei Ni, Vyacheslav S. Lukin
We numerically study magnetic reconnection on different spatial scales and at different heights in the weakly ionized plasma of the low solar atmosphere (around ~km above…
Investigation of white-light emission in circular-ribbon flares
Yongliang Song, Hui Tian
Using observations by the Solar Dynamics Observatory from June 2010 to December 2017, we have performed the first statistical investigation of circular-ribbon flares (CFs) and exam…
Chirality and magnetic configuration associated with two-ribbon solar flares: AR 10930 versus AR 11158
Han He, Huaning Wang, Yihua Yan +2
The structural property of the magnetic field in flare-bearing solar active regions (ARs) is one of the key aspects for understanding and forecasting solar flares. In this paper, w…
Coronal condensations caused by magnetic reconnection between solar coronal loops
Leping Li, Jun Zhang, Hardi Peter +5
Employing Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA) multi-wavelength images, we report the coronal condensation during the magnetic reconnection (MR) betw…
The Characteristics of Valley Phase as Predictor of the Forthcoming Solar Cycle
Baolin Tan
Is Solar Cycle 24 anomalous? How do we predict the main features of a forthcoming cycle? In order to reply such questions, this work partitions quantitatively each cycle into valle…
Eruption of a multi-flux-rope system in solar active region 12673 leading to the two largest flares in Solar Cycle 24
Y. J. Hou, J. Zhang, T. Li +2
Solar active region (AR) 12673 in 2017 September produced two largest flares in Solar Cycle 24: the X9.3 flare on September 06 and the X8.2 flare on September 10. We attempt to inv…
Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST
Dong Li, Yuandeng Shen, Zongjun Ning +2
We present high-resolution observations of two kinds of dynamic behavior in a quiescent prominence using the New Vacuum Solar Telescope, i.e., Kelvin-Helmholtz instabilities (KHIs)…
Is It Small-scale Weak Magnetic Activity That Effectively Heats the Upper Solar Atmosphere?
K. J. Li, J. C. Xu, W. Feng
Solar chromosphere and coronal heating is a big question for astrophysics. Daily measurement of 985 solar spectral irradiances (SSIs) at the spectral intervals 1-39 nm and 116-2416…
Predictability of the solar cycle over one cycle
Jie Jiang, Jing-Xiu Wang, Qi-Rong Jiao +1
The prediction of the strength of future solar cycles is of interest because of its practical significance for space weather and as a test of our theoretical understanding of the s…
Spectroscopic and imaging observations of small-scale reconnection events
Dong Li, Leping Li, Zongjun Ning
We present spectroscopic and imaging observations of small-scale reconnection events on the Sun. Using the Interface Region Imaging Spectrograph (IRIS) observations, one reconnecti…
EUV Waves Driven by the Sudden Expansion of Transequatorial Loops Caused by Coronal Jets
Yuandeng Shen, Zehao Tang, Yuhu Miao +2
We present two events to study the driving mechanism of extreme-ultraviolet (EUV) waves that are not associated with coronal mass ejections (CMEs), by using high resolution observa…