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K. Chan

4 papers hereh-index 13631 citations60 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • K. Chan — 164 papers, h 87
  • K. Chan — 37 papers, h 17
  • K. Chan — 27 papers, h 18
  • K. Chan — 18 papers
  • K. Chan — 17 papers, h 13
  • K. Chan — 14 papers, h 7

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
20002005
most cited3D convection simulations of the outer layers of the Sun using realistic physics

101 citations · 147 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph2005★ 29 cited

Effect of the radiative background flux in convection

A. Brandenburg, K. L. Chan, A. Nordlund +1

Numerical simulations of turbulent stratified convection are used to study models with approximately the same convective flux, but different radiative fluxes. As the radiative flux…

astro-ph2005★ 17 cited

Simulating the outer layers of Procyon A: a comparison with the Sun

F. J. Robinson, P. Demarque, D. B. Guenther +2

Compared to the Sun, the atmospheric structure and convective flow in Procyon A exhibit the following characteristics: (1) the highly superadiabatic transition layer (SAL) is locat…

astro-ph2002★ 101 cited

3D convection simulations of the outer layers of the Sun using realistic physics

F. J. Robinson, P. Demarque, L. H. Li +4

This paper describes a series of 3D simulations of shallow inefficient convection in the outer layers of the Sun. The computational domain is a closed box containing the convection…

astro-ph2000

The effect of turbulent pressure on the p-mode frequencies in stellar models

P. Demarque, L. H. Li, F. J. Robinson +4

We have constructed models for the sun at three stages of its evolution: a zero-age main sequence model, the present sun, and a subgiant model. For each model, the turbulent pressu…

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