Multi-wavelength emission in resistive pulsar magnetospheres

Open Access

Fig. B.2.

Isocontours of the power j ⋅ E dissipated in the current sheet outside the light cylinder for a perpendicular rotator with conductivity $log \tilde{σ} = {- 1, 0, 1}$ ${\log \tilde{\sigma} = \{-1,0,1\}}$ from left to right. The maximum dissipation is normalised to unity in all cases for better comparison. The grey disk represents the neutron star, and the dashed grey circle represents the light cylinder.

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.