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Interactions between the Planetary Magnetic Field and the Surrounding Gas Flows in the Final Stage of the Giant Planet Formation. I. Two Distinct Evolutionary Scenarios

  • Authors: Pengfei Tang, Xiaogang Wang, Tianchun Zhou, Jiayong Zhong

Pengfei Tang et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 16.

Time evolution of Lc for simulations G101Dn5In4n3 and G101Dn5In4n4m5 (see the text for the definition). The volume integral is taken over the twisted upper-half magnetosphere in the rθ plane, with the toroidal integral omitted due to axisymmetry. Specifically, the volume element is ﹩dV={r}^{2}\sin (\theta )drd\theta ﹩. The panels share the same y-axis.

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