Fig. 1From: Earth atmospheric loss through the plasma mantle and its dependence on solar wind parametersSolar wind dynamic pressure subsets. \({\hbox{O}}^{+}\) flux (colour bar in \({\hbox{log}}_{10} ~{\hbox{m}}^{-2} {\hbox{s}}^{-1}\)) in the plasma mantle for 9 different solar wind dynamic pressure conditions numbered from 1 to 9 or, respectively, from the lowest to the highest dynamic pressureBack to article page