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E. Panetier

3 papers here

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

author position
  • first author1
  • middle author1
  • last author1

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

fields
  • astro-ph.SR3
ORCID 0009-0000-7269-9621

identity via Semantic Scholar / OpenAlex

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

9 citations · 9 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024

Solar p-modes excitation rate along the magnetic activity cycle

E. Panetier, S. N. Breton, R. A. García +2

Magnetic cycles of solar-like stars influence their internal physics. Thus, the frequency, amplitude, excitation rate, and damping of the acoustic oscillation modes (p-modes) vary…

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.SR2024

Measuring stellar surface rotation and activity with the PLATO mission -- I. Strategy and application to simulated light curves

S. N. Breton, A. F Lanza, S. Messina +20

The Planetary Transits and Oscillations of stars mission (PLATO) will allow us to measure surface rotation and monitor photometric activity of tens of thousands of main sequence so…

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