Artificial ﹩\mathrm{\log}_{10}( I_{\mathrm{O}\,\,{}^{{\rm{\small VI}}}\,\lambda 1032}) ﹩ edge‐on view (LOS in plane of equatorial current sheet), synthesized from our models 1 (left) and 2 (right). Both images were produced assuming that the oxygen abundance in the streamer closed region is depleted by a factor of 1/100. Black lines are contours of the same intensity with values ﹩10^{-4},3\times 10^{-4},5\times 10^{-4},10^{-3},10^{-2},10^{-1}﹩, and 1 of the maximum intensity. White lines are selected magnetic field lines in the plane of the sky.