An investigation of ground-based observations of solar oscillations at Stanford

Mathematics

Scientific paper

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Doppler Effect, Error Analysis, Image Processing, Mathematical Models, Solar Oscillations, Spectral Signatures, Asymptotic Methods, Circular Polarization, Magnetic Fields, Power Spectra, Signal To Noise Ratios, Time Series Analysis

Scientific paper

Data obtained in the last 8 years of solar differential Doppler observations at Stanford were considered. The four best time series of data were examined in detail. The sources of error in the data were investigated and removed where possible. In particular, the contribution resulting from transparency variations in the sky was examined. Detection method applicable to data with low signal to noise ratio and low filling factor were developed and utilized for the investigation of global solar modes of oscillations in the data. The frequencies of p-modes were measured and identified. The presence of g-modes were also determined in the Stanford data.

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