activity
20002007
most citedYREC: The Yale Rotating Stellar Evolution Code

230 citations · 356 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2007★ 230 cited

YREC: The Yale Rotating Stellar Evolution Code

P. Demarque, D. B. Guenther, L. H. Li +2

The stellar evolution code YREC is outlined with emphasis on its applications to helio- and asteroseismology. The procedure for calculating calibrated solar and stellar models is d…

astro-ph2005★ 20 cited

2-D Stellar Evolution Code Including Arbitrary Magnetic Fields. I. Mathematical Techniques and Test Cases

L. H. Li, P. Ventura, S. Basu +2

A high-precision two-dimensional stellar evolution code has been developed for studying solar variability due to structural changes produced by varying internal magnetic fields of…

astro-ph2005★ 5 cited

A flux tube solar dynamo model based on the competing role of buoyancy and downflows

L. H. Li, S. Sofia, G. Belvedere

A magnetic flux tube may be considered both as a separate body and as a confined field. As a field, it is affected both by differential rotation (-effect) and cyclonic convectio…

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-ph2001

A convection zone dynamo including the effects of magnetic buoyancy and downward flows

L. H. Li, S. Sofia

A magnetic flux tube may be considered both as a separate body and as a confined field. As a field, it is affected both by the cyclonic convection (-effect) and differential rot…

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…