Fig. 2: Relationships of φLMI with LMI and genesis latitude in observations and HighResMIP models. | npj Climate and Atmospheric Science

Fig. 2: Relationships of φLMI with LMI and genesis latitude in observations and HighResMIP models.

From: Poleward migration of western North Pacific tropical cyclones driven by genesis location shift under global warming in HighResMIP-PRIMAVERA models

Fig. 2: Relationships of φLMI with LMI and genesis latitude in observations and HighResMIP models.

Scatter plots of a, b \({{\boldsymbol{\varphi }}}_{{\boldsymbol{LMI}}}\) vs. LMI (m s−1) and c, d \({{\boldsymbol{\varphi }}}_{{\boldsymbol{LMI}}}\) vs genesis latitude (\({{\boldsymbol{\varphi }}}_{{\boldsymbol{Genesis}}}\)) for all TCs during 1984–2014 based on the observations (dark dots) and numerical simulations (color dots) by a, c AGCMs and b, d CGCMs. Red dots represent CMCC-CM2, green dots represent CNRM-CM6-1, blue dots represent HadGEM3-GC31, cyan dots represent EC-Earth3P and purple dots represent MPI-ESM1.2. The best-fit curves for each model with their 95% two-sided confidence intervals (shading) are interpolated. The solid and dashed lines represent HR and LR models, respectively.

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