activity
20072026
most citedInfluence of Low-Degree High-Order p-Mode Splittings on the Solar Rotation Profile

39 citations · 82 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

On the feasibility of inverting the rotation of the solar core with mixed f/g modes

Armand Leclerc, Arthur Le Saux, J. M. Joel Ong +1

Context: Thanks to helioseismology, the rotation profile of the Sun has been measured with great precision down to 20% of its total radius. This rotation profile is used as a calib…

astro-ph.SR2024★ 9 cited

Seismic differences between solar magnetic cycles 23 and 24 for low-degree modes

Rafael A. Garcia, Sylvain N. Breton, David Salabert +4

Solar magnetic activity follows regular cycles of about 11 years with an inversion of polarity in the poles every 22 years. This changing surface magnetism impacts the properties o…

astro-ph.SR2019★ 1 cited

Automatic classification of K2 pulsating stars using machine learning techniques

A. Le Saux, L. Bugnet, S. Mathur +2

The second mission of the NASA Kepler satellite, K2, has collected hundreds of thousands of lightcurves for stars close to the ecliptic plane. This new sample could increase the nu…

astro-ph.SR2014★ 8 cited

Oscillating red-giant stars in eccentric binary systems

P. G. Beck, K. Hambleton, J. Vos +4

The unparalleled photometric data obtained by NASA's Kepler Space Telescope has led to improved understanding of red-giant stars and binary stars. We discuss the characterization o…

astro-ph.SR2010

Can major solar flares excite high-frequency global waves in the Sun ?

Brajesh Kumar, Savita Mathur, R. A. Garcia +1

The study of low-degree high-frequency waves in the Sun can provide new insight into the dynamics of the deeper layers of the Sun. Here, we present the analysis of the velocity obs…

astro-ph.SR2009★ 1 cited

Low-Degree High-Frequency p and g Modes in the Solar Core

S. Mathur, R. A. Garcia, A. Eff-Darwich

Solar gravity (g) modes propagate within the radiative part of the solar interior and are highly sensitive to the physical conditions of the solar core. They would represent the be…