Fig. 17


Download original image

FACs and ground magnetic perturbations due to shock compression on 17 March 2015 from a high-resolution BATSRUS run coupled with CRCM and IE. The simulated magnetic perturbations at Poker Flat were compared with the real magnetometer observations. The results shown here illustrate the capacity of the SWMF to resolve mesoscale features of the magnetospheric dynamics in high-resolution MHD (Zou et al., 2017).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.