Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 35, issue 2
Articles | Volume 35, issue 2
https://doi.org/10.5194/angeo-35-239-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-35-239-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
Articles | Volume 35, issue 2
Regular paper
 | 
22 Feb 2017
Regular paper |  | 22 Feb 2017

The generation of Ganymede's diffuse aurora through pitch angle scattering

Arvind K. Tripathi, Rajendra P. Singhal, and Onkar N. Singh II

Viewed

Total article views: 1,253 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
765 394 94 1,253 65 80
  • HTML: 765
  • PDF: 394
  • XML: 94
  • Total: 1,253
  • BibTeX: 65
  • EndNote: 80
Views and downloads (calculated since 22 Feb 2017)
Cumulative views and downloads (calculated since 22 Feb 2017)

Cited

Latest update: 14 Dec 2024
Download
Short summary
In the present paper diffuse auroral intensities of OI λ1356 Å emission have been calculated, resulting from pitch angle diffusion of magnetospheric electrons by whistler-mode waves. Three cases are considered for estimating precipitation flux into the atmospheric loss cone. An analytical yield spectrum (AYS) approach is used to calculate energy deposition of electrons in the atmosphere of Ganymede. It is found that the intensities are inadequate to account for the observational intensities.
Read more