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Lijuan Liu

23 papers hereh-index 14450 citations34 works total

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

author position
  • sole author1
  • first author10
  • middle author10
  • last author1

Across the 22 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR23
same name
  • Lijuan Liu — 6 papers, h 6
  • Lijuan Liu — 5 papers, h 3
  • Lijuan Liu — 2 papers, h 2
  • Lijuan Liu — 2 papers, h 2
  • Lijuan Liu — 2 papers, h 2
  • Lijuan Liu — 2 papers, h 2

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
20132026
most citedWhy is a flare-rich active region CME-poor?

57 citations · 401 across the 23 of their papers we have counts for

collaborators
Showing 2019Show all

4 papers · 1 filter

astro-ph.SR2019★ 24 cited

Formation of a Magnetic Flux Rope in the Early Emergence Phase of NOAA Active Region 12673

Lijuan Liu, Xin Cheng, Yuming Wang +1

In this work, we investigate the formation of a magnetic flux rope (MFR) above the central polarity inversion line (PIL) of NOAA Active Region 12673 during its early emergence phas…

astro-ph.SR2019

Two Types of Solar Confined Flares

Ting Li, Lijuan Liu, Yijun Hou +1

With the aim of understanding the physical mechanisms of confined flares, we selected 18 confined flares during 2011-2017, and classified the confined flares into two types based o…

astro-ph.SR2019★ 15 cited

Extreme-ultraviolet Late Phase Caused by Magnetic Reconnection over Quadrupolar Magnetic Configuration in a Solar Flare

Zhenjun Zhou, Xin Cheng, Lijuan Liu +3

A second emission enhancement in warm coronal extreme-ultraviolet (EUV) lines (about 2-7 MK) during some solar flares is known as the EUV late phase. Imaging observations confirm t…

astro-ph.SR2019★ 51 cited

Why torus-unstable solar filaments experience failed eruption?

Zhenjun Zhou, Xin Cheng, Jie Zhang +5

To investigate the factors that control the success and/or failure of solar eruptions, we study the magnetic field and 3-Dimensional (3D) configuration of 16 filament eruptions dur…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.