On the origin of solar oscillations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages, 3 figures, typo in title fixed

Scientific paper

10.1086/311203

We have made high resolution observations of the Sun in which we identify individual sunquakes and see power from these seismic events being pumped into the resonant modes of vibration of the Sun. A typical event lasts about five minutes. We report the physical properties of the events and relate them to theories of the excitation of solar oscillations. We also discuss the local seismic potential of these events.

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