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Z. Xue

35 papers hereh-index 17977 citations69 works total

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

author position
  • first author1
  • middle author29
  • last author2

Across the 32 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR35
same name
  • Z. Xue — 116 papers, h 28
  • Z. Xue — 52 papers, h 23
  • Z. Xue — 13 papers, h 30
  • Z. Xue — 5 papers, h 6
  • Z. Xue — 4 papers, h 27
  • Z. Xue — 4 papers, h 1

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 citedSimultaneous observation of a flux rope eruption and magnetic reconnection during an X-class solar flare

121 citations · 569 across the 33 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.SR2014★ 50 cited

Unwinding motion of a twisted active-region filament

X. L. Yan, Z. K. Xue, J. H. Liu +2

To better understand the structures of active-region filaments and the eruption process, we study an active-region filament eruption in active region NOAA 11082 in detail on June 2…

astro-ph.SR2014★ 7 cited

Eruptions of Two Coupled Filaments Observed by SDO, GONG and STEREO

Z. K. Xue, X. L. Yan, Z. Q. Qu +2

On 2012 July 11, two solar filaments were observed in the northeast of the solar disk and their eruptions due to the interaction between them are studied by using the data from the…

astro-ph.SR2014

Disappearance of a coronal hole induced by a filament activation

Ma Lin, Qu Zhong-Quan, Yan Xiao-Li +1

We present a rare observation of direct magnetic interaction between an activating filament and a coronal hole (CH). The filament was a quiescent one located at the northwest of th…

astro-ph.SR2014★ 38 cited

Kink instability evidenced by analyzing the leg rotation of a filament

X. L. Yan, Z. K. Xue, J. H. Liu +4

Kink instability is a possible mechanism for solar filament eruption. However, the twist of a solar filament is very difficult to directly measure from observation. In this paper,…

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