activity
19972011
most citedThe Non-Homologous Nature of Solar Diameter Variations

44 citations · 131 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2011★ 27 cited

Solar Models with Revised Abundance

Shaolan Bi, Tanda Li, Linghuai Li +1

We present new solar models in which we use the latest low abundances and we further include the effects of rotation, magnetic fields and extra-mixing processes. We assume that the…

astro-ph2008

Calculation of Solar P-mode Oscillation Frequency Splittings Based on a Two-dimensional Solar Model

Linghuai Li, Sarbani Basu, Sabatino Sofia +1

We compute the p-mode oscillation frequencies and frequency splittings that arise in a two-dimensional model of the Sun that contains toroidal magnetic fields in its interior.

astro-ph2008★ 9 cited

Two-Dimensional Stellar Evolution Code Including Arbitrary Magnetic Fields. II. Precision Improvement and Inclusion of Turbulence and Rotation

Linghuai Li, Sabatino Sofia, Paolo Ventura +4

In the second paper of this series we pursue two objectives. First, in order to make the code more sensitive to small effects, we remove many approximations made in Paper I. Second…

astro-ph2008★ 10 cited

Interpreting Helioseismic Structure Inversion Results of Solar Active Regions

Chia-Hsien Lin, Sarbani Basu, Linghuai Li

Helioseismic techniques such as ring-diagram analysis have often been used to determine the subsurface structural differences between solar active and quiet regions. Results obtain…

astro-ph2005★ 44 cited

The Non-Homologous Nature of Solar Diameter Variations

Sabatino Sofia, Sarbani Basu, Pierre Demarque +2

We show in this paper that the changes of the solar diameter in response to variations of large scale magnetic fields and turbulence are not homologous. For the best current model,…

astro-ph2005★ 31 cited

Space and Ground Based Pulsation Data of Eta Bootis Explained with Stellar Models Including Turbulence

Christian W. Straka, Pierre Demarque, D. B. Guenther +2

The space telescope MOST is now providing us with extremely accurate low frequency p-mode oscillation data for the star Eta Boo. We demonstrate in this paper that these data, when…