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

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Latest update: 26 Feb 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.