Abstract
Three-dimensional magnetohydrodynamic simulations of high-β plasmas show that toroidally localized high- n ballooning modes can be driven unstable by the local pressure steepening that arises from the evolution of low- n modes. Nonlinearly, the high- n mode becomes even more localized and produces a strong local pressure bulge that destroys the flux surfaces resulting in a thermal quench. The flux surfaces then recover temporarily but now contain large magnetic islands. This scenario is supported by experimental data.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1763-1766 |
| Number of pages | 4 |
| Journal | Physical review letters |
| Volume | 75 |
| Issue number | 9 |
| DOIs | |
| State | Published - 1995 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy