Fig. 5From: Earth atmospheric loss through the plasma mantle and its dependence on solar wind parametersZoom of two coupling functions for \({\hbox{O}}^+\) in the plasma mantle. Zoom of two functions \(\hbox {E}_{\mathrm{in}}\) and \(\hbox {P}_{\alpha =0.3}\) from Fig. 4. The increase of \({\hbox{O}}^+\) escape rate after the threshold is almost linearBack to article page