Abstract
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 5 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.
Original language | English (US) |
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Pages (from-to) | L27-L30 |
Journal | Astrophysical Journal |
Volume | 495 |
Issue number | 1 PART II |
DOIs | |
State | Published - 1998 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Sun: granulation
- Sun: oscillations
- Sun: photosphere