Articles | Volume 37, issue 4
https://doi.org/10.5194/angeo-37-763-2019
https://doi.org/10.5194/angeo-37-763-2019
Comment/reply
 | 
29 Aug 2019
Comment/reply |  | 29 Aug 2019

Comment on “Cavitons and spontaneous hot flow anomalies in a hybrid-Vlasov global magnetospheric simulation” by Blanco-Cano et al. (2018)

Gábor Facskó

Viewed

Total article views: 2,089 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,444 597 48 2,089 56 53
  • HTML: 1,444
  • PDF: 597
  • XML: 48
  • Total: 2,089
  • BibTeX: 56
  • EndNote: 53
Views and downloads (calculated since 22 Jan 2019)
Cumulative views and downloads (calculated since 22 Jan 2019)

Viewed (geographical distribution)

Total article views: 2,089 (including HTML, PDF, and XML) Thereof 1,712 with geography defined and 377 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Discussed (preprint)

Latest update: 20 Nov 2024
Short summary
Blanco-Cano et al. (2018) intended to find a type of transient event in the solar wind before the terrestrial bow shock using a special type of simulation. However, the simulation results cannot reproduce the main features of the event. Based on the remarks described below, I am sure that the features in the simulations are not those types of events. The Vlasiator code simulated proto-SHFAs.