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Fig. 14.

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Visual impression of the magnetic field topology in and around one of the clouds. This cloud has formed through TI and is currently falling down. The volume rendering highlights dense gas and the magnetic field lines are coloured according to the local magnetic field strength. The shown magnetic field lines connect the inside of the cloud to the ambient gas above the cloud. The magnetic field inside the cloud is stronger (achieving B∼1 μG) compared to the magnetic field in the ambient gas.

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