Hot Jupiters were the first type of planet to be discovered around a Sun-like star, the first to have their atmospheres characterized, and the first to have measurements that constrained wind and temperature structures. While these big and bright planets are observationally favorable, they are also interesting laboratories of atmospheric physics under extreme conditions. While we have been working to model their 3D structure for two decades, there are still many complicated pieces of physics that challenge our efforts and prevent model predictions from fully matching observations. To accurately model these atmospheres in 3D, we must consider: clouds/hazes, molecular dissociation (of opacity sources and even hydrogen), magnetic effects resulting from thermal ionization, and how these all work in concert with the full atmospheric dynamics and radiative transfer. In this talk I will give a brief overview of where the field currently stands in addressing these challenges.
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