In a solar-minimum-like coronal MHD model, slip-back mapping shows a median 3.5% of total open flux is processed through interchange reconnection in any 24-hour period.
Otherwise, the connectivity is recorded as closed (C, if both footpoints of the field line are atR 0) or disconnected (D, if both footpoints are atR 1)
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Tracking Magnetic Topological Change in a Time-Dependent Coronal Model
In a solar-minimum-like coronal MHD model, slip-back mapping shows a median 3.5% of total open flux is processed through interchange reconnection in any 24-hour period.