Abstract
We present a simple idealized model of stochastically forced solar oscillations, and compare the distribution function of energy, averaged over 12-hour intervals, with that of low-degree solar modes. We find that the simulated energy distribution is similar to the observations, except at extremely high energy.
Original language | English |
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Pages (from-to) | 251-263 |
Number of pages | 13 |
Journal | Solar Physics |
Volume | 181 |
Issue number | 2 |
DOIs | |
State | Published - 1998 |