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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Main Authors: R. A. Treumann, Wolfgang Baumjohann
Format: Article
Language:English
Published: Frontiers Media S.A. 2021-09-01
Series:Frontiers in Physics
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2021.711882/full
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spelling 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
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AT ratreumann diffusejosephsonradiationinturbulence
AT wolfgangbaumjohann diffusejosephsonradiationinturbulence
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