A New Way to Model the Solar Oscillation ℓ-ν Power Spectrum

Details A New Way to Model the Solar Oscillation ℓ-ν Power Spectrum A New Way to Model the Solar Oscillation ℓ-ν Power Spectrum

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..220..347j&link_type=abstract

Solar Physics, Volume 220, Issue 2, pp.347-359

Physics

7

Scientific paper

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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