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Fig. 9

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Poloidal magnetic field in the gap for the run Mj-β3, averaged in azimuth and over the last 100 orbits (episode ℰ2). The background color represents the logarithm of the poloidal magnetic field. The black streamlines and the LIC correspond to the radial and vertical components of the poloidal magnetic field. The white curves represents the radial profile of log(Σ), also averaged in azimuth and over the last 100 orbits. The red cross and solid black line pinpoint the location of the planet. Vertical black dashed lines delineate the gap edges at RRp − 2Rhill and RRp + 5Rhill. The upper and lower surfaces ±zw±4H(R) are indicated by the black dotted lines.

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