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 |
|---|---|
| Pages (from-to) | 251-263 |
| Number of pages | 13 |
| Journal | Solar Physics |
| Volume | 181 |
| Issue number | 2 |
| DOIs | |
| State | Published - 1998 |