Optimal wavelength strategies for DKIST/VTF enable detection of local acoustic source wavefronts from solar simulations.
and Kumar , P., 1994, `` Excitation of solar p-modes '', \/ , 424 , 466--479
2 Pith papers cite this work. Polarity classification is still indexing.
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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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Assessment of DKIST/VTF Capabilities for the Detection of Local Acoustic Source Wavefronts
Optimal wavelength strategies for DKIST/VTF enable detection of local acoustic source wavefronts from solar simulations.
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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.