Our goal is to quantify whether, and if so how, spatio-temporal patterns in tropical cyclone (TC) satellite imagery signal an upcoming rapid intensity change event. To address this question, we propose a new nonparametric test of association between a time series of images and a series of binary event labels. We ask whether there is a difference in distribution between (dependent but identically distributed) 24-h sequences of images preceding an event versus a non-event. By rewriting the statistical test as a regression problem, we leverage neural networks to infer modes of structural evolution of TC convection that are representative of the lead-up to rapid intensity change events. Dependencies between nearby sequences are handled by a bootstrap procedure that estimates the marginal distribution of the label series. We prove that type I error control is guaranteed as long as the distribution of the label series is well-estimated, which is made easier by the extensive historical data for binary TC event labels. We show empirical evidence that our proposed method identifies archetypes of infrared imagery associated with elevated rapid intensification risk, typically marked by deep or deepening core convection over time. Such results provide a foundation for improved forecasts of rapid intensification.
翻译:我们的目标是量化热带气旋(TC)卫星图像中的时空模式是否以及如何显示即将到来的快速强度变化事件。为了解决这一问题,我们提议对一个时间系列图像和一系列二元事件标签之间的关联进行新的非参数性测试。我们问,事件前24小时图像序列与非事件序列之间的分布(独立但同样分布)之间是否有差异。通过将统计测试重写为一个回归问题,我们利用神经网络来推导体现快速强度变化事件前导力的三角对流结构演变模式。附近序列之间的依赖性由测算标签系列边际分布的靴式程序处理。我们证明,只要对标签系列的分布进行精确估计,就保证了对类型I的错误控制,而对于二元技术合作事件标签标签标签的广泛历史数据更容易。我们提供了实证证据,证明我们提出的方法确定了红外图像的成型类型,与快速强化风险有关,通常以深度或深度核心对时间进行快速调整为标志的强化基础,提供这种结果的改进。