Fig. 3

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Comparison between the 2D temperature maps of hot Jupiter GCMs in the upper row (Perna et al. 2012), and the 2D temperature maps represented with the hmℓ basis in the middle and lower rows with ℓmax = 1 and 50, respectively. The horizontal axis is longitude, the vertical axis is latitude, and the center of each map is the substellar point. For model input parameters see Table 1; for an outline of the linear algorithm used to fit maps with ℓmax = 50, see Appendix A.
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