The signature of granulation in a solar power spectrum as seen with CO5BOLD 

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DOI

  • Mia S. Lundkvist
  • Hans Günter Ludwig, Heidelberg University 
  • ,
  • Remo Collet
  • ,
  • Thomas Straus, Osservatorio Astronomico di Capodimonte

The granulation background seen in the power spectrum of a solar-like oscillator poses a serious challenge for extracting precise and detailed information about the stellar oscillations. Using a 3D hydrodynamical simulation of the Sun computed with co5bold, we investigate various background models to infer, using a Bayesian methodology, which one provides the best fit to the background in the simulated power spectrum. We find that the best fit is provided by an expression including the overall power level and two characteristic frequencies, one with an exponent of two and one with a free exponent taking on a value around six. We assess the impact of the 3D hydro-code on this result by repeating the analysis with a simulation from S tagger and find that the main conclusion is unchanged. However, the details of the resulting best fits differ slightly between the two codes, but we explain this difference by studying the effect of the spatial resolution and the duration of the simulation on the fit. Additionally, we look into the impact of adding white noise to the simulated time series as a simple way to mimic a real star. We find that, as long as the noise level is not too low, the results are consistent with the no-noise case.

OriginalsprogEngelsk
TidsskriftMonthly Notices of the Royal Astronomical Society
Vol/bind501
Nummer2
Sider (fra-til)2512-2521
Antal sider10
ISSN0035-8711
DOI
StatusUdgivet - feb. 2021

Bibliografisk note

Funding Information:
The authors wish to thank Guy R. Davies for valuable discussions and python routines implementing PYSTAN, Ren? Salhab for sharing PYTHON routines for reading CO5BOLD files, and Matthias Steffen for providing the solar model c600. Additionally, the authors would like to thank the anonymous referee for providing comments that improved the manuscript. MSL is supported by the Carlsberg Foundation (Grant agreement no.: CF17-0760). Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant DNRF106). HGL acknowledges financial support by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) - Project-ID 138713538 - SFB 881 ('The Milky Way System', subproject A04). The simulations of our Reference model were carried out at CINECA (Bologna/Italy)with CPU time assigned under INAF/CINECA agreement 2008/2010.

Publisher Copyright:
© 2021 The Author(s).

Copyright:
Copyright 2021 Elsevier B.V., All rights reserved.

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