Solar oscillations instrumentation and measurement theory

Details Solar oscillations instrumentation and measurement theory Solar oscillations instrumentation and measurement theory

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..595a&link_type=abstract

In its Seismology of the Sun and Sun-Like Stars p 595-600 (SEE N89-25819 19-92)

Physics

Helioseismology, Optical Measuring Instruments, Solar Instruments, Solar Oscillations, Solar Physics, Solar Spectra, Spectrum Analysis, Velocity Measurement

Scientific paper

Solar-oscillation instruments are reviewed. Common characteristics include detecting solar radial velocities on Fraunhofer lines with a 2-point measuring technique, high spectral resolution and stability, etc. The choice of the spectral line for getting a high signal to solar noise ratio is addressed. Velocity imaging of solar oscillations modes is detailed, including spatial sampling and span, highest observable degree. Applications of these different analyses is applied to existing or future helioseismology instruments.

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