Influence of the Martian crustal magnetic fields on oxygen ion escape at Mars

Open Access

Table 1

Setups for the three groups of simulations.

Run label	Run name	IMF condition^a	Crustal field location^b
A1	+B_Y, No	+B_Y	No
A2	−B_Y, No	−B_Y	No

B1	+B_Y, Dayside	+B_Y	Dayside
B2	−B_Y, Dayside	−B_Y	Dayside

C1	+B_Y, Nightside	+B_Y	Nightside
C2	−B_Y, Nightside	−B_Y	Nightside

Notes. ^a “+B_Y” and “−B_Y” represent +B_Y IMF and +B_Y IMF conditions, as described in text. ^b “No” denotes crustal magnetic fields excluded from the simulation. Other terms indicate the local time of the strongest crustal fields region.

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.