File Download
There are no files associated with this item.
SFX Link
- Find it @ UNIST can give you direct access to the published full text of this article. (UNISTARs only)
- Ryu, Dongsu
- Astrophysics Lab.
Views & Downloads
Detailed Information
Cited time in 
Cited time in 
Cited time in
Metadata Downloads
Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.citation.conferencePlace | JA | - |
| dc.citation.conferencePlace | 일본 Kagoshima | - |
| dc.citation.title | Cosmic Magnetism in the Pre-SKA Era | - |
| dc.contributor.author | Ryu, Dongsu | - |
| dc.date.accessioned | 2024-12-13T14:35:08Z | - |
| dc.date.available | 2024-12-13T14:35:08Z | - |
| dc.date.created | 2024-12-12 | - |
| dc.date.issued | 2024-05-30 | - |
| dc.description.abstract | Turbulence Dynamo as the Origin of Magnetic Fields in Clusters of Galaxies Dongsu Ryu (UNIST) Magnetic fields are ubiquitous in astrophysical environments. The distribution and strength of magnetic fields in the large-scale structure of the universe, especially in clusters of galaxies, have been established through various observations, such as Faraday rotation and synchrotron emission. Yet their origins are still under debate. In this talk, I discuss whether the magnetic fields observed in clusters of galaxies could be described by the small-scale turbulence dynamo amplification. |
- |
| dc.identifier.bibliographicCitation | Cosmic Magnetism in the Pre-SKA Era | - |
| dc.identifier.uri | https://scholarworks.unist.ac.kr/handle/201301/84812 | - |
| dc.language | 영어 | - |
| dc.publisher | National Astronomical Observatory of Japan | - |
| dc.title | Turbulence Dynamo as the “Origin” of Magnetic Fields in Clusters of Galaxies (Studies of the “Origin” of Cosmic Magnetic Fields ) | - |
| dc.type | Conference Paper | - |
| dc.date.conferenceDate | 2024-05-27 | - |
Items in Repository are protected by copyright, with all rights reserved, unless otherwise indicated.