activity
19972024
most citedSeismic evidence for a rapidly rotating core in a lower-giant-branch star observed with Kepler

402 citations · 5k across the 157 of their papers we have counts for

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Showing 2013Show all

8 papers · 1 filter

astro-ph.SR2013★ 7 cited

Propagating Linear Waves in Convectively Unstable Stellar Models: a Perturbative Approach

Emanuele Papini, Laurent Gizon, Aaron C. Birch

Linear time-domain simulations of acoustic oscillations are unstable in the stellar convection zone. To overcome this problem it is customary to compute the oscillations of a stabi…

astro-ph.SR2013

Precise and accurate interpolated stellar oscillation frequencies on the main sequence

Warrick H. Ball, Jesper Schou, Laurent Gizon +1

High-quality data from space-based observatories present an opportunity to fit stellar models to observations of individually-identified oscillation frequencies, not just the large…

astro-ph.SR2013★ 98 cited

Seismic constraints on rotation of Sun-like star and mass of exoplanet

Laurent Gizon, Jérome Ballot, Eric Michel +32

Rotation is thought to drive cyclic magnetic activity in the Sun and Sun-like stars. Stellar dynamos, however, are poorly understood owing to the scarcity of observations of rotati…

astro-ph.EP2013★ 11 cited

Propagation of seismic waves through a spatio-temporally fluctuating medium: Homogenization

Shravan Hanasoge, Laurent Gizon, Guillaume Bal

Measurements of seismic wave travel times at the photosphere of the Sun have enabled inferences of its interior structure and dynamics. In interpreting these measurements, the simp…

astro-ph.SR2013★ 27 cited

Comparison of solar surface flows inferred from time--distance helioseismology and coherent structure tracking using HMI/SDO observations

M. Svanda, Th. Roudier, M. Rieutord +2

We compare measurements of horizontal flows on the surface of the Sun using helioseismic time--distance inversions and coherent structure tracking of solar granules. Tracking provi…

astro-ph.SR2013★ 36 cited

Helioseismology of sunspots: how sensitive are travel times to the Wilson depression and to the subsurface magnetic field?

Hannah Schunker, Laurent Gizon, Robert H. Cameron +1

In order to assess the ability of helioseismology to probe the subsurface structure and magnetic field of sunspots, we need to determine how helioseismic travel times depend on per…