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Fig. 6.
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Evolution of the various energy contributions along a magnetic surface of anchoring radius r0 = 100 for the simulation K2 at tend: the Bernoulli invariant E, the gravitational potential ΦG, the total specific kinetic energy u2/2, the enthalpy H, and the magnetic energy −Ω*rBΦ/η. The absicssa is the altitude Z(Ψ).
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