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Magnetic Effects in Hot Jupiter Atmospheres

  • Authors: T. M. Rogers and T. D. Komacek

Rogers & Komacek 2014 The Astrophysical Journal 794 132.

  • Provider: AAS Journals

Caption: Figure 5.

Day–night temperature differential as a function of pressure. The solid line is the hydrodynamic version, dotted lines are 10 G MHD models, and dashed lines are 30 G MHD models. Red lines represent cool models, M2, M2b1, and M2b2, and black lines represent hot models, M7, M7b1, and M7b2.

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