Articles | Volume 36, issue 4
https://doi.org/10.5194/angeo-36-1015-2018
https://doi.org/10.5194/angeo-36-1015-2018
Regular paper
 | Highlight paper
 | 
26 Jul 2018
Regular paper | Highlight paper |  | 26 Jul 2018

The mirror mode: a “superconducting” space plasma analogue

Rudolf A. Treumann and Wolfgang Baumjohann

Viewed

Total article views: 5,221 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
4,365 771 85 5,221 86 91
  • HTML: 4,365
  • PDF: 771
  • XML: 85
  • Total: 5,221
  • BibTeX: 86
  • EndNote: 91
Views and downloads (calculated since 08 May 2018)
Cumulative views and downloads (calculated since 08 May 2018)

Viewed (geographical distribution)

Total article views: 5,221 (including HTML, PDF, and XML) Thereof 4,796 with geography defined and 425 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 17 Jul 2024
Download
Short summary
The physics of the magnetic mirror mode in its final state of saturation, the thermodynamic equilibrium, is re-examined to demonstrate that the mirror mode is the classical analogue of a superconducting effect in an anisotropic-pressure space plasma. Three different spatial correlation scales are identified which control the behaviour of its evolution into large-amplitude chains of mirror bubbles.