Abstract
We present a new approach for the precise and accurate forward modeling of the solar oscillation ℓ−ν power spectrum. The approach is designed to provide the basis for a streamlined solar seismic inversion without measurements of the p-mode frequencies. The new strategy represents a paradigm change in how information is extracted from the oscillation spectrum. It also represents a step toward the ideal case of inferring the Sun's properties directly from the raw observations.
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Jefferies, S.M., Vorontsov, S.V. A New Way to Model the Solar Oscillation ℓ−ν Power Spectrum. Solar Physics 220, 347–359 (2004). https://doi.org/10.1023/B:SOLA.0000031404.13076.73
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DOI: https://doi.org/10.1023/B:SOLA.0000031404.13076.73