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Ying D. Liu

13 papers hereh-index 141k citations33 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • middle author9
  • last author1

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR11
  • physics.space-ph2
same name
  • Ying D. Liu — 10 papers, h 4
  • Ying D. Liu — 7 papers, h 7
  • Ying D. Liu — 5 papers, h 10
  • Ying D. Liu — 1 paper
  • Ying D. Liu — 1 paper, h 22
  • Ying D. Liu — 1 paper, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20132023
most citedSuccessive Two-sided loop Jets Caused by Magnetic Reconnection between Two adjacent Filamentary Threads

41 citations · 194 across the 13 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

astro-ph.SR2022★ 7 cited

Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure

Huidong Hu, Ying D. Liu, Lakshmi Pradeep Chitta +2

On the Sun, Doppler shifts of bidirectional outflows from the magnetic-reconnection site have been found only in confined regions through spectroscopic observations. Without spatia…

astro-ph.SR2022★ 4 cited

Multispacecraft Remote Sensing and In Situ Observations of the 2020 November 29 Coronal Mass Ejection and Associated Shock: From Solar Source to Heliospheric Impacts

Chong Chen, Ying D. Liu, Bei Zhu

We investigate the source eruption, propagation and expansion characteristics, and heliospheric impacts of the 2020 November 29 coronal mass ejection (CME) and associated shock, us…

astro-ph.SR2022★ 11 cited

Analysis of the distribution, rotation and scale characteristics of solar wind switchbacks: comparison between the first and second encounters of Parker Solar Probe

Mingming Meng, Ying D. Liu, Chong Chen +1

The S-shaped magnetic structure in the solar wind formed by the twisting of magnetic field lines is called a switchback, whose main characteristics are the reversal of the magnetic…

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