Abstract
The radiative dissipation of divertor target heat flux on DIII-D is shown to greatly exceed the limitations of energy transport dominated by electron thermal conduction parallel to the magnetic field. More than 80% of the power flowing into the outboard divertor is dissipated through radiation with a broad poloidal profile. It is shown that energy transport dominated by convection over a large region of the divertor is consistent with the data.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 4769-4772 |
| Number of pages | 4 |
| Journal | Physical review letters |
| Volume | 78 |
| Issue number | 25 |
| DOIs | |
| State | Published - Jun 23 1997 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy