BibTeX
CSL-JSON
MLA
Harvard
Galactic dynamo simulations
release_nbh7ktem2jdqpmuu6xseeey6ea
by
Detlef Elstner,
Oliver Gressel,
Günther Rüdiger
Published
in Proceedings of the International Astronomical Union
by Cambridge University Press (CUP).
2008 Issue S259, p467-478
Abstract
<jats:title>Abstract</jats:title>Recent simulations of supernova-driven turbulence within the ISM support the existence of a large-scale dynamo. With a growth time of about two hundred million years, the dynamo is quite fast – in contradiction to many assertions in the literature. We here present details on the scaling of the dynamo effect within the simulations and discuss global mean-field models based on the adopted turbulence coefficients. The results are compared to global simulations of the magneto-rotational instability.
In application/xml+jats format
Archived Files and Locations
application/pdf
931.4 kB
file_da4uivxaibbtvl4ej5ux66nuvu
| |
application/pdf
957.1 kB
file_gkrbsn4ez5aankhq32p6w4jmea
|
www.cambridge.org (web) web.archive.org (webarchive) |
application/pdf
957.0 kB
file_bmivue7uvnbbfmnfvjmb5dy2xq
|
web.archive.org (webarchive) www.cambridge.org (web) |
application/pdf
957.1 kB
file_krq6yyocdrgm3dedffv6rg3bfa
|
web.archive.org (webarchive) www.cambridge.org (web) |
Read Archived PDF
Preserved and Accessible
Work Entity
access all versions, variants, and formats of this works (eg, pre-prints)
access all versions, variants, and formats of this works (eg, pre-prints)
Cite This
Lookup Links
oaDOI/unpaywall (OA fulltext)
Crossref Metadata (via API)
Worldcat
SHERPA/RoMEO (journal policies)
wikidata.org
CORE.ac.uk
Semantic Scholar
Google Scholar
Crossref Metadata (via API)
Worldcat
SHERPA/RoMEO (journal policies)
wikidata.org
CORE.ac.uk
Semantic Scholar
Google Scholar