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Mirror mode junctions as sources of radiation

Treumann, R. A., and Wolfgang Baumjohann (2021), Mirror mode junctions as sources of radiation, Frontiers Astronomy and Space Sciences, 8, 648744, doi:10.3389/fspas.2021.648744.

Abstract
Mirror modes in collisionless high-temperature plasmas represent macroscopic hightemperature
quasi-superconductors with bouncing electrons in discrete-particle
resonance with thermal ion-sound noise contributing to the ion-mode growth beyond
quasilinear stability. In the semi-classical Ginzburg-Landau approximation the conditions
for phase transition are reviewed. The quasi-superconducting state is of second kind
causing a magnetically perforated plasma texture. Focussing on the interaction of mirror
bubbles we apply semi-classical Josephson conditions and show that a mirror perforated
plasma emits weak electromagnetic radiation which in the magnetosheath should be in the
sub-millimeter, respectively, infrared range. This effect might be of astrophysical
importance.
Further information
BibTeX
@article{id2696,
  author = {R. A. Treumann and Wolfgang Baumjohann},
  journal = {Frontiers Astronomy and Space Sciences},
  month = {mar},
  pages = {648744},
  title = {{Mirror mode junctions as sources of radiation}},
  volume = {8},
  year = {2021},
  url = {https://doi.org/10.3389/fspas.2021.648744},
  doi = {10.3389/fspas.2021.648744},
}
EndNote
%0 Journal Article
%A Treumann, R. A.
%A Baumjohann, Wolfgang
%D 2021
%V 8
%J Frontiers Astronomy and Space Sciences
%P 648744
%T Mirror mode junctions as sources of radiation
%U https://doi.org/10.3389/fspas.2021.648744
%U https://arxiv.org/abs/2101.00637
%8 mar
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Printed 01. Dec 2021 17:25