151 citations · 1.3k across the 39 of their papers we have counts for
39 papers
Jovian Zonal Winds Revealed from Cassini/VIMS Observations
Shenghan Ma, Yuming Wang, Tao Li +3
Understanding Jupiter's zonal winds is crucial to unraveling the dynamics of its atmosphere. Over the last decades, multiple data sources and techniques have been used to study zon…
Photospheric Swirls in a Quiet-Sun Region
Quan Xie, Jiajia Liu, Chris J. Nelson +2
Swirl-shaped flow structures have been observed throughout the solar atmosphere, in both emission and absorption, at different altitudes and locations, and are believed to be assoc…
Improving the Automated Coronal Jet Identification with U-NET
Jiajia Liu, Chunyu Ji, Yimin Wang +5
Coronal jets are one of the most common eruptive activities in the solar atmosphere. They are related to rich physics processes, including but not limited to magnetic reconnection,…
The Fibre Resolved opticAl and Near-ultraviolet Czerny-Turner Imaging Spectropolarimeter (FRANCIS)
D. B. Jess, S. D. T. Grant, W. Bate +9
The solar physics community is entering a golden era that is ripe with next-generation ground- and space-based facilities. With ever-increasing resolving power stemming from the ne…
On the 5-Minute Oscillations of Photospheric and Chromospheric Swirls
Jiajia Liu, David Jess, Robert Erdélyi +1
Swirls are ubiquitous in the solar atmosphere. They are believed to be related to the excitation of different modes of magnetohydrodynamic waves and pulses, as well as spicules. Ho…
Power-law Distribution of Solar-Cycle Modulated Coronal Jets
Jiajia Liu, Anchuan Song, David B. Jess +6
Power-law distributions have been studied as a significant characteristic of non-linear dissipative systems. Since discovering the power-law distribution of solar flares that was l…
Polymeric jets throw light on the origin and nature of the forest of solar spicules
Sahel Dey, Piyali Chatterjee, Murthy O. V. S. N. +4
Spicules are plasma jets, observed in the dynamic interface region between the visible solar surface and the hot corona. At any given time, it is estimated that about 3 million spi…
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…
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…
On the partial eruption of a bifurcated solar filament structure
Aabha Monga, Rahul Sharma, Jiajia Liu +4
The partial eruption of a filament channel with bifurcated substructures is investigated using datasets obtained from both ground-based and space-borne facilities. Small-scale flux…
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
Mark P. Rast, Nazaret Bello González, Luis Bellot Rubio +84
The Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand and model the basic physical processes that control the structure and dynamics of…
Multi-wavelength Observation of a Failed Eruption from a Helical Kink-unstable Prominence
Haiqing Xu, Jiangtao Su, Jie Chen +7
Multi-wavelength observations of prominence eruptions provide an opportunity to uncover the physical mechanism of the triggering and the evolution process of the eruption. In this…
Solar Flare Prediction Using Magnetic Field Diagnostics Above the Photosphere
M. B. Korsos, M. K. Georgoulis, N. Gyenge +7
In this article, we present the application of the weighted horizontal gradient of magnetic field (WGM) flare prediction method to 3-dimensional (3D) extrapolated magnetic configur…
Reconstructing solar wind inhomogeneous structures from stereoscopic observations in white-light: Solar wind transients in 3D
Xiaolei Li, Yuming Wang, Rui Liu +7
White-light images from Heliospheric Imager-1 (HI1) onboard the Solar Terrestrial Relations Observatory (STEREO) provide 2-dimensional (2D) global views of solar wind transients tr…
Co-spatial velocity and magnetic swirls in the simulated solar photosphere
Jiajia Liu, Mats Carlsson, Chris J Nelson +1
Context. Velocity or intensity swirls have now been shown to be widely present throughout the photosphere and chromosphere. It has been suggested that these events could contribute…
How Many Twists Do Solar Coronal Jets Release?
Jiajia Liu, Yuming Wang, Robertus Erdélyi
Highly twisted magnetic flux ropes, with finite length, are subject to kink instabilities, and could lead to a number of eruptive phenomena in the solar atmosphere, including flare…
Reconstructing solar wind inhomogeneous structures from stereoscopic observations in white-light: Small transients along the Sun-Earth line
Xiaolei Li, Yuming Wang, Rui Liu +5
The Heliospheric Imagers (HI) on board the two spacecraft of the Solar Terrestrial Relations Observatory (STEREO) provided white-light images of transients in the solar wind from d…
Observations of Turbulent Magnetic Reconnection Within a Solar Current Sheet
X. Cheng, Y. Li, L. F. Wan +4
Magnetic reconnection is a fundamental physical process in various astrophysical, space, and laboratory environments. Many pieces of evidence for magnetic reconnection have been un…
Automated Swirl Detection Algorithm (ASDA) and Its Application to Simulation and Observational Data
Jiajia Liu, Chris J. Nelson, Robert Erdélyi
Swirling motions in the solar atmosphere have been widely observed in recent years and suggested to play a key role in channeling energy from the photosphere into the corona. Here,…
Understanding the twist distribution inside magnetic flux ropes by anatomizing an interplanetary magnetic cloud
Yuming Wang, Chenglong Shen, Rui Liu +6
Magnetic flux rope (MFR) is the core structure of the greatest eruptions, i.e., the coronal mass ejections (CMEs), on the Sun, and magnetic clouds are post-eruption MFRs in interpl…
A New Tool for CME Arrival Time Prediction Using Machine Learning Algorithms: CAT-PUMA
Jiajia Liu, Yudong Ye, Chenlong Shen +2
Coronal Mass Ejections (CMEs) are arguably the most violent eruptions in the Solar System. CMEs can cause severe disturbances in the interplanetary space and even affect human acti…
Magnetic braids in eruptions of a spiral structure in the solar atmosphere
Zhenghua Huang, Lidong Xia, Chris J. Nelson +6
We report on high-resolution imaging and spectral observations of eruptions of a spiral structure in the transition region, which were taken with the Interface Region Imaging Spect…
Upward and downward catastrophes of coronal magnetic flux ropes in quadrupolar magnetic fields
Quanhao Zhang, Yuming Wang, Youqiu Hu +3
Coronal magnetic flux ropes are closely related to large-scale solar activities. Using a 2.5-dimensional time-dependent ideal magnetohydrodynamic (MHD) model in Cartesian coordinat…
Untwisting Jets Related to Magnetic Flux Cancellation
Jiajia Liu, Robert Erdélyi, Yuming Wang +1
The rotational motion of solar jets is believed to be a signature of the untwisting process resulting from magnetic reconnection, which takes place between twisted closed magnetic…