Abstract
The suppression of thermal conduction by a static stochastic magnetic field is calculated for different ratios of the field scale length to the collisional mean free path. The effects of magnetic trapping are determined through a two-scale analysis and Monte Carlo particle simulations. In galaxy-cluster cooling flows, thermal conductivity is reduced from the Spitzer value by a factor of order 102 to 103.
Original language | English (US) |
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Pages (from-to) | 3077-3080 |
Number of pages | 4 |
Journal | Physical review letters |
Volume | 80 |
Issue number | 14 |
DOIs | |
State | Published - 1998 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy