Magnetoacoustic cutoff frequency rises with height from 3.0 mHz at 0.38 Mm to 8.5 mHz at 1.2 Mm based on cross-wavelet analysis of IRIS Doppler velocities.
and Gough , D., 1984, `` Helioseismology: Oscillations as a Diagnostic of the Solar Interior '', \/ , 22 , 593--619
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.SR 2representative citing papers
This review summarizes the development, techniques, and open questions in asteroseismology of solar-type stars whose oscillations are stochastically excited by surface convection.
citing papers explorer
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Height Variations of Magnetoacoustic Cutoff Frequency in the Solar Atmosphere
Magnetoacoustic cutoff frequency rises with height from 3.0 mHz at 0.38 Mm to 8.5 mHz at 1.2 Mm based on cross-wavelet analysis of IRIS Doppler velocities.
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Asteroseismology of solar-type stars
This review summarizes the development, techniques, and open questions in asteroseismology of solar-type stars whose oscillations are stochastically excited by surface convection.