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GONG p-Mode Parameters Through Two Solar Cycles.

René Kiefer1,2,3, Rudi Komm3, Frank Hill3

  • 11Centre for Fusion, Space, and Astrophysics, Department of Physics, University of Warwick, Coventry, CV4 7AL UK.

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|March 19, 2019
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Summary
This summary is machine-generated.

This study analyzes solar p-mode oscillations using Global Oscillation Network Group data from two solar cycles. Mean squared velocities and energies of p-modes are anticorrelated with solar activity, while energy supply rates show no significant correlation.

Keywords:
Helioseismology, observationsOscillations, solarSolar Cycle, observations

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Area of Science:

  • Heliophysics
  • Solar Physics
  • Asteroseismology

Background:

  • Solar p-mode oscillations are acoustic waves that travel through the Sun.
  • Understanding their parameters, like amplitude and damping, is crucial for studying solar activity.
  • Previous studies have explored temporal variations, but a comprehensive analysis across two solar cycles is needed.

Purpose of the Study:

  • To investigate the parameters of global solar p-mode oscillations over two solar cycles (1996-2018).
  • To analyze the relationship between these parameters and solar activity, specifically solar radio flux.
  • To expand understanding of the excitation and damping mechanisms of solar p-modes.

Main Methods:

  • Utilized time series data from the Global Oscillation Network Group (GONG) for harmonic degrees.
  • Corrected mode amplitudes for fill factor, apparent solar radius, and spurious jumps.
  • Analyzed mode parameters (damping width, amplitude, mean squared velocity, energy, energy supply rate) as a function of frequency and harmonic degree.

Main Results:

  • Activity-related changes in amplitude and damping width depend on mode frequency and harmonic degree.
  • Mean squared velocities and energies of p-modes are anticorrelated with solar activity, varying by 10% and 5% respectively.
  • Mode energy supply rates showed no significant correlation with solar activity.

Conclusions:

  • Solar p-mode velocities and energies decrease during periods of high solar activity.
  • The interplay between convection, magnetic fields, and acoustic oscillations is complex and varies with mode properties.
  • This research provides a robust dataset for future studies on solar interior dynamics and activity cycles.