Diffuse Josephson Radiation in Turbulence
The possibility of generating diffuse radiation in extended astronomical media by plasma turbulence is investigated under the assumption that the turbulence can be understood as an ensemble of small-scale magnetic filaments (narrow current sheets) forming a texture around a large number of magnetic...
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2021-09-01
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doaj-5dfe1e0b710b4130a1bb42bb7622980d2021-09-21T06:06:17ZengFrontiers Media S.A.Frontiers in Physics2296-424X2021-09-01910.3389/fphy.2021.711882711882Diffuse Josephson Radiation in TurbulenceR. A. Treumann0R. A. Treumann1Wolfgang Baumjohann2International Space Science Institute (ISSI), Bern, SwitzerlandGeophysics, Department Geoscience and Environment, Munich University (LMU), Munich, GermanySpace Research Institute (IWF), Austrian Academy of Sciences, Graz, AustriaThe possibility of generating diffuse radiation in extended astronomical media by plasma turbulence is investigated under the assumption that the turbulence can be understood as an ensemble of small-scale magnetic filaments (narrow current sheets) forming a texture around a large number of magnetic depletions or voids. On astronomically microscopic scales, the dilute high temperature medium (plasma) is to be considered ideally conducting, forming a collection of Josephson junctions between two such adjacent quasi-superconductors. The oscillation frequency of those junctions depends on the part of the spectrum that contributes to the oscillation, causing weak radio backgrounds. Lowest Josephson frequencies/energies near zero may become sources of quasi-stationary magnetic fields.https://www.frontiersin.org/articles/10.3389/fphy.2021.711882/fullintracluster gasplasma turbulenceJosephson junctionsradio radiationcosmic magnetic fields |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
R. A. Treumann R. A. Treumann Wolfgang Baumjohann |
spellingShingle |
R. A. Treumann R. A. Treumann Wolfgang Baumjohann Diffuse Josephson Radiation in Turbulence Frontiers in Physics intracluster gas plasma turbulence Josephson junctions radio radiation cosmic magnetic fields |
author_facet |
R. A. Treumann R. A. Treumann Wolfgang Baumjohann |
author_sort |
R. A. Treumann |
title |
Diffuse Josephson Radiation in Turbulence |
title_short |
Diffuse Josephson Radiation in Turbulence |
title_full |
Diffuse Josephson Radiation in Turbulence |
title_fullStr |
Diffuse Josephson Radiation in Turbulence |
title_full_unstemmed |
Diffuse Josephson Radiation in Turbulence |
title_sort |
diffuse josephson radiation in turbulence |
publisher |
Frontiers Media S.A. |
series |
Frontiers in Physics |
issn |
2296-424X |
publishDate |
2021-09-01 |
description |
The possibility of generating diffuse radiation in extended astronomical media by plasma turbulence is investigated under the assumption that the turbulence can be understood as an ensemble of small-scale magnetic filaments (narrow current sheets) forming a texture around a large number of magnetic depletions or voids. On astronomically microscopic scales, the dilute high temperature medium (plasma) is to be considered ideally conducting, forming a collection of Josephson junctions between two such adjacent quasi-superconductors. The oscillation frequency of those junctions depends on the part of the spectrum that contributes to the oscillation, causing weak radio backgrounds. Lowest Josephson frequencies/energies near zero may become sources of quasi-stationary magnetic fields. |
topic |
intracluster gas plasma turbulence Josephson junctions radio radiation cosmic magnetic fields |
url |
https://www.frontiersin.org/articles/10.3389/fphy.2021.711882/full |
work_keys_str_mv |
AT ratreumann diffusejosephsonradiationinturbulence AT ratreumann diffusejosephsonradiationinturbulence AT wolfgangbaumjohann diffusejosephsonradiationinturbulence |
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1717373713036345344 |