Articles | Volume 34, issue 12
https://doi.org/10.5194/angeo-34-1175-2016
https://doi.org/10.5194/angeo-34-1175-2016
Regular paper
 | 
15 Dec 2016
Regular paper |  | 15 Dec 2016

Observations of diffusion in the electron halo and strahl

Chris Gurgiolo and Melvyn L. Goldstein

Viewed

Total article views: 1,503 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
794 648 61 1,503 64 74
  • HTML: 794
  • PDF: 648
  • XML: 61
  • Total: 1,503
  • BibTeX: 64
  • EndNote: 74
Views and downloads (calculated since 15 Dec 2016)
Cumulative views and downloads (calculated since 15 Dec 2016)

Cited

Latest update: 23 Nov 2024
Download
Short summary
Using Cluster data we have noted observations of diffusion-like signatures in the energy range where the the solar wind halo and strahl populations overlap. This includes the development of a proto-halo. At present the source of this diffusion is not known or understood. The prime analysis was carried out through the use of phi–theta plots at individual energy steps. The motivation was to understand if repartitioning in energy was occurring at these locations.