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Dynamo-generated turbulence and out ° ows from accretion discs
| Content Provider | Semantic Scholar |
|---|---|
| Author | Brandenburg, By Axel |
| Copyright Year | 1996 |
| Abstract | Local hydromagnetic simulations of accretion-disc turbulence currently provide the most convincing evidence that the origin of turbulence in discs could be the Balbus{ Hawley magnetorotational instability. The main results of such calculations are highlighted with particular emphasis on the generation of large-scale magnetic elds. Comparison with mean- eld dynamo theory is made. This theory is then used to address the question of the launching and collimation of winds emanating from the disc surfaces. |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://antares.ncl.ac.uk/~brandenb/papers/rs.ps.gz |
| Alternate Webpage(s) | http://www.nordita.org/~brandenb/Own_Papers/2000/Bran_philtrans00.pdf |
| Alternate Webpage(s) | http://www.nordita.org/~brandenb/Own_Papers/Bran_philtrans00.pdf |
| Alternate Webpage(s) | http://www.nordita.org/~brandenb/own/Bran_philtrans00.pdf |
| Language | English |
| Access Restriction | Open |
| Subject Keyword | ARID1A wt Allele Collimator Device Component Environmental Wind Instability Simulation Turbulence |
| Content Type | Text |
| Resource Type | Article |
