Abstract
In a recent Letter, Litvinenko, Forbes, and Priest (1996) claimed that the rate of the very fast flux-pile rip reconnection is severely limited by the effects of plasma pressure. They considered however only two-dimensional, zero-vorticity flows. Here we show that this limitation is a feature of these restrictive assumptions and can be removed by relaxing either of them.
| Original language | English |
|---|---|
| Pages (from-to) | 411-414 |
| Number of pages | 4 |
| Journal | Solar Physics |
| Volume | 177 |
| Publication status | Published - Jan 1998 |
Keywords
- MAGNETIC-FIELD ANNIHILATION
- STAGNATION-POINT FLOWS
- STEADY-STATE
- CURRENT SHEET