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: 5,345 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
4,448 803 94 5,345 92 99
  • HTML: 4,448
  • PDF: 803
  • XML: 94
  • Total: 5,345
  • BibTeX: 92
  • EndNote: 99
Views and downloads (calculated since 08 May 2018)
Cumulative views and downloads (calculated since 08 May 2018)

Viewed (geographical distribution)

Total article views: 5,345 (including HTML, PDF, and XML) Thereof 4,917 with geography defined and 428 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 22 Nov 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.