Articles | Volume 39, issue 1
https://doi.org/10.5194/angeo-39-165-2021
https://doi.org/10.5194/angeo-39-165-2021
ANGEO Communicates
 | 
22 Feb 2021
ANGEO Communicates |  | 22 Feb 2021

Wavevector spectral signature of decay instability in space plasmas

Horia Comişel, Yasuhito Narita, and Uwe Motschmann

Viewed

Total article views: 1,479 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,006 387 86 1,479 66 61
  • HTML: 1,006
  • PDF: 387
  • XML: 86
  • Total: 1,479
  • BibTeX: 66
  • EndNote: 61
Views and downloads (calculated since 18 May 2020)
Cumulative views and downloads (calculated since 18 May 2020)

Viewed (geographical distribution)

Total article views: 1,479 (including HTML, PDF, and XML) Thereof 1,379 with geography defined and 100 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 23 Nov 2024
Download
Short summary
Identification of a large-amplitude Alfvén wave decaying into a pair of ion-acoustic and daughter Alfvén waves is one of the major goals in the observational studies of space plasma nonlinearity. Growth-rate maps may serve as a useful tool for predictions of the wavevector spectrum of density or magnetic field fluctuations in various scenarios for the wave–wave coupling processes developing at different stages in space plasma turbulence.