353 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of Science and Technology of ChinaCN34 papers
- Purple Mountain ObservatoryCN31 papers
- Chinese Academy of SciencesCN13 papers
- Instituto de Astrofísica de CanariasES9 papers
- Universidad de La LagunaES9 papers
- Macau University of Science and TechnologyMO6 papers
- Nanjing UniversityCN6 papers
- Tsinghua UniversityCN5 papers
- Christian-Albrechts-Universität zu KielDE4 papers
- Max Planck Institute for Solar System ResearchDE4 papers
- National Space Science CenterCN4 papers
- Shanghai Institutes for Biological SciencesCN4 papers
14 papers · 1 filter
Effects of supra-arcade downflows interacting with the post-flare arcade
Arun Kumar Awasthi, Rui Liu, Tingyu Gou
Supra-arcade downflows (SADs) are dark voids descending through plasma above the post-flare arcade. Although they are generally viewed as byproducts of flare reconnections in the c…
Sigmoid Formation Through Slippage of A Single J-shaped Coronal Loop
Hanya Pan, Tingyu Gou, Rui Liu
A well-known precursor of an imminent solar eruption is the appearance of a hot S-shaped loop, also known as sigmoid, in an active region (AR). Classically, the formation of such a…
Investigating the stability of mass transfer in neutron star-helium white dwarf binaries
Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen +1
Neutron star-helium white dwarf (NS+He WD) binaries are important evolutionary products of close-orbit binary star systems. They are often observed as millisecond pulsars and may c…
Successive Coronal Mass Ejections Associated with Weak Solar Energetic Particle Events
Bin Zhuang, Noé Lugaz, Tingyu Gou +1
The scenario of twin coronal mass ejections (CMEs), i.e., a fast and wide primary CME (priCME) preceded by previous CMEs (preCMEs), has been found to be favorable to a more efficie…
Radial Evolution of the April 2020 Stealth Coronal Mass Ejection between 0.8 and 1 AU -- A Comparison of Forbush Decreases at Solar Orbiter and Earth
Johan L. Freiherr von Forstner, Mateja Dumbović, Christian Möstl +40
Aims. We present observations of the first coronal mass ejection (CME) observed at the Solar Orbiter spacecraft on April 19, 2020, and the associated Forbush decrease (FD) measured…
The configuration and failed eruption of a complex magnetic flux rope above a δ sunspot region
Lijuan Liu, Jiajia Liu, Jun Chen +4
Aims. We investigate the configuration of a complex flux rope above a δ sunspot region in NOAA AR 11515, and its eruptive expansion during a confined M5.3-class flare. Methods. We…
Pre-eruption Splitting of the Double-Decker Structure in a Solar Filament
Hanya Pan, Rui Liu, Tingyu Gou +4
Solar filaments often erupt partially. Although how they split remains elusive, the splitting process has the potential of revealing the filament structure and eruption mechanism.…
Parametric simulation studies on the wave propagation of solar radio emission: the source size, duration, and position
PeiJin Zhang, ChuanBing Wang, Eduard P. Kontar
The observed features of the radio sources indicate complex propagation effects embedded in the waves of solar radio bursts. In this work, we perform ray-tracing simulations on rad…
First Solar energetic particles measured on the Lunar far-side
Zigong Xu, Jingnan Guo, Robert. F. Wimmer-Schweingruber +6
On 2019 May 6, the Lunar Lander Neutron & Dosimetry (LND) Experiment on board the Chang'E-4 on the far-side of the Moon detected its first small solar energetic particle (SEP) even…
Evolution of coronal mass ejections and the corresponding Forbush decreases: modelling vs multi-spacecraft observations
Mateja Dumbović, Bojan Vršnak, Jingnan Guo +9
One of the very common in situ signatures of interplanetary coronal mass ejections (ICMEs), as well as other interplanetary transients, are Forbush decreases (FDs), i.e. short-term…
Interferometric Imaging with LOFAR Remote Baselines of the Fine Structures of a Solar Type IIIb Radio Burst
PeiJin Zhang, Pietro Zucca, Sarrvesh Seethapuram Sridhar +8
Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A subcategory of solar r…
Mass motion in a prominence bubble revealing a kinked flux rope configuration
Arun Kumar Awasthi, Rui Liu
Prominence bubbles are cavities rising into quiescent prominences from below. The bubble-prominence interface is often the active location for the formation of plumes, which flow t…
Mass Loss via Solar Wind and Coronal Mass Ejections During Solar Cycle 23 and 24
Wageesh Mishra, Nandita Srivastava, Yuming Wang +3
Similar to the Sun, other stars shed mass and magnetic flux via ubiquitous quasi-steady wind and episodic stellar coronal mass ejections (CMEs). We investigate the mass loss rate v…
Double-Decker Filament Configuration Revealed by Mass Motions
Arun Kumar Awasthi, Rui Liu, Yuming Wang
It is often envisaged that dense filament material lies in the dips of magnetic field lines belonging to either a sheared arcade or a magnetic flux rope. But it is also debated whi…