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Fig. 1

image

a): Schematic depiction of a poloidal slice of the magnetosphere of an isolated pulsar, reproduced from GLP Fig. 1. The vertical dashed lines mark the location of the LC (ρ/RL = 1, with ρ and z being the cylindrical coordinates measuring the distance to and along the rotation axis, and the LC is at ρ = RL). The red curves represent the CSs that demarcate the different magnetic domains (1) (inside the shaded bubble containing closed field lines) and (2) (open field line region). b): A depiction of the split monopole solution, with a CS on the equatorial plane, facilitating the change of field line direction across it.

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