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B. Tan

48 papers hereh-index 231.3k citations100 works total

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

author position
  • sole author8
  • first author14
  • middle author15
  • last author9

Across the 46 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR47
  • physics.ao-ph1
same name
  • B. Tan — 26 papers, h 15
  • B. Tan — 6 papers, h 7
  • B. Tan — 4 papers, h 11
  • B. Tan — 3 papers, h 2
  • B. Tan — 2 papers, h 12
  • B. Tan — 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
20092026
most citedMicrowave Quasi-periodic Pulsations in Multi-timescales Associated with a Solar Flare/CME Event

72 citations · 871 across the 47 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.SR2021★ 3 cited

The early evolution of solar flaring plasma loops

Baolin Tan

Plasma loops are the elementary structures of solar flaring active regions which dominate the whole processes of flaring eruptions. The standard flare models are well explained the…

astro-ph.SR2021★ 4 cited

Energy and spectral analysis of confined solar flares from radio and X-ray observations

Chengming Tan, Karl-Ludwig Klein, Yihua Yan +4

The energy and spectral shape of radio bursts may help us understand the generation mechanism of solar eruptions, including solar flares, CMEs, eruptive filaments, and various scal…

astro-ph.SR2021★ 29 cited

Characteristic time of stellar flares on Sun-like stars

Y. Yan, H. He, C. Li +4

Using the short-cadence data (1-min interval) of the Kepler space telescope, we conducted a statistical analysis for the characteristic time of stellar flares on Sun-like stars (SL…

astro-ph.SR2021★ 19 cited

PIC Simulation of Double Plasma Resonance and Zebra Pattern of Solar Radio Bursts

Chuanyang Li, Yao Chen, Sulan Ni +3

Latest study reports that plasma emission can be generated by energetic electrons of DGH distribution via the electron cyclotron maser instability (ECMI) in plasmas characterized b…

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