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Chao Zhang

4 papers hereh-index 315 citations8 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • Chao Zhang — 40 papers, h 21
  • Chao Zhang — 38 papers, h 38
  • Chao Zhang — 28 papers, h 10
  • Chao Zhang — 26 papers, h 22
  • Chao Zhang — 23 papers, h 7
  • Chao Zhang — 23 papers, h 11

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
20222025
most citedAn EUV jet driven by a series of transition region micro-jets

5 citations · 5 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025

Sequential ejections of plasma blobs due to unbraiding of tangled loops in the solar atmosphere

Xiuhui Zuo, Zhenghua Huang, Hengyuan Wei +8

Nanoflares, which are consequences of braids in tangled magnetic fields, are an important candidate to heat the solar corona to million degrees. However, their observational eviden…

astro-ph.SR2025

Multi-episodes of remote brightenings driven by a coronal EUV jet on the Sun

Chao Zhang, Zhenghua Huang, Hengyuan Wei +8

Remote brightening (RB) is compact brightening at footpoints of magnetic loops, which are remotely-connecting to and confining an eruption in the solar atmosphere. Here, we report…

astro-ph.SR2024

Formation of a streamer blob via the merger of multiple plasma clumps below 2Rs

Haiyi Li, Zhenghua Huang, Kaiwen Deng +7

Context. Propagating streamer blobs could be an important source of disturbances in the solar wind. Direct observations on formation of streamer blobs could be a proxy for understa…

astro-ph.SR2022★ 5 cited

An EUV jet driven by a series of transition region micro-jets

Hengyuan Wei, Zhenghua Huang, Hui Fu +5

Jets are one of the most common eruptive events in the solar atmosphere, and they are believed to be important in the context of coronal heating and solar wind acceleration. We pre…

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