Fig. 5From: Investigations of the degree of asymmetry across the dayside magnetopause under southward interplanetary magnetic field using GEOTAIL observationsPlot of the degree of asymmetry \(k_N, k_T\) and \(k_{B_z}\) as a function of \(y_{\textrm{GSM}}\) in all 81 crossings. The spread in the data of the \(k_N\) is large on the dusk side, whereas that of the \(k_{B_z}\) on the dawn sideBack to article page