activity
20152023
most citedA Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

211 citations · 803 across the 25 of their papers we have counts for

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Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR2022

Influence of magnetic reconnection on the eruptive catastrophes of coronal magnetic flux ropes

Quanhao Zhang, Xin Cheng, Rui Liu +3

Large-scale solar eruptive activities have a close relationship with coronal magnetic flux ropes. Previous numerical studies have found that the equilibrium of a coronal flux rope…

astro-ph.SR2022★ 21 cited

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…

astro-ph.SR2021★ 9 cited

Confined and eruptive catastrophes of solar magnetic flux ropes caused by mass loading and unloading

Quanhao Zhang, Rui Liu, Yuming Wang +2

It is widely accepted that coronal magnetic flux ropes are the core structures of large-scale solar eruptive activities, which inflict dramatic impacts on the solar-terrestrial sys…

astro-ph.SR2021★ 11 cited

Radial velocity map of solar wind transients in the field of view of STEREO/HI1 on 3 and 4 April 2010

Xiaolei Li, Yuming Wang, Jingnan Guo +2

The solar wind transients propagating out in the inner heliosphere can be observed in white-light images from Heliospheric Imager-1 (HI1), an instrument of the Sun Earth Connection…

astro-ph.SR2021★ 3 cited

How flux feeding causes eruptions of solar magnetic flux ropes with the hyperbolic flux tube configuration?

Quanhao Zhang, Rui Liu, Yuming Wang +3

Coronal magnetic flux ropes are generally considered to be the core structure of large-scale solar eruptions. Recent observations found that solar eruptions could be initiated by a…

astro-ph.SR2021★ 9 cited

Three-dimensional Reconstruction of Coronal Mass Ejections by CORAR Technique through Different Stereoscopic Angle of STEREO Twin Spacecraft

Shaoyu Lyu, Yuming Wang, Xiaolei Li +3

Recently, we developed the Correlation-Aided Reconstruction (CORAR) method to reconstruct solar wind inhomogeneous structures, or transients, using dual-view white-light images (Li…

astro-ph.SR2020★ 13 cited

Cause and Kinematics of a Jet-Like CME

Reetika Joshi, Yuming Wang, Ramesh Chandra +3

In this article, we present the multi-viewpoint and multi-wavelength analysis of an atypical solar jet based on the data from Solar Dynamics Observatory, SOlar, and Heliospheric Ob…

astro-ph.SR2020★ 19 cited

Eruption of Solar Magnetic Flux Ropes Caused by Flux Feeding

Quanhao Zhang, Yuming Wang, Rui Liu +5

Large-scale solar eruptions are believed to have a magnetic flux rope as the core structure. However, it remains elusive as to how the flux rope builds up and what triggers its eru…

astro-ph.SR2020★ 11 cited

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…

astro-ph.SR2020★ 10 cited

Optimal Stereoscopic Angle for Reconstructing Solar Wind Inhomogeneous Structures

Shaoyu Lyu, Xiaolei Li, Yuming Wang

This paper is aimed at finding the best separation angle between spacecraft for the three-dimensional reconstruction of solar-wind inhomogeneous structures by the CORrelation-Aided…

astro-ph.SR2018★ 14 cited

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…

astro-ph.SR2018★ 73 cited

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…