Fig. 3

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Jovian magnetospheric magnetic field lines near the dayside magnetodisc reconnection in the simulation. The blue, black, and green lines represent the stretched inner, flux rope, and outer magnetic fields passing through areas near the considered x-line (magenta line), respectively. The red lines denote the quasi-dipole fields in the inner magnetosphere. The Bθ zero lines at the equatorial plane are marked in cyan, and the considered x-line is marked in magenta. The equatorial bold black lines represent the magnetopause. The simulation time (ST) is 437 : 00.
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