日本地球惑星科学連合2019年大会

講演情報

[E] 口頭発表

セッション記号 A (大気水圏科学) » A-AS 大気科学・気象学・大気環境

[A-AS02] 台風研究の新展開~過去・現在・未来

2019年5月30日(木) 09:00 〜 10:30 104 (1F)

コンビーナ:金田 幸恵(名古屋大学宇宙地球環境研究所)、和田 章義(気象研究所台風・災害気象研究部)、伊藤 耕介(琉球大学)、宮本 佳明(慶應義塾大学 環境情報学部)、座長:金田 幸恵(名古屋大学)、和田 章義(気象研究所)

09:45 〜 10:00

[AAS02-04] Potential impacts of tropical cyclone inner-core convective activity on the predictability of rapid intensification

*南出 将志1Derek Posselt1 (1.Jet Propulsion Laboratory, California Institute of Technology)

キーワード:台風、数値予報、全天輝度温度同化、対流

Predictions of significant changes in tropical cyclone (TC) intensity, such as rapid intensification (RI), have emerged as a more challenging topic than forecasting TC tracks, since intensification of TCs involves multi-scale physical processes with significant contributions from convective-scale phenomena. Before the onset of RI, intensifying TCs are known to experience a precession process, in which tilted vortex rotates counter-clockwise to develop axisymmetric structure. From both modeling and observational studies, there is an agreement in the qualitative features of precession process among TCs, but the quantitative features, such as the vortex tilt magnitude, the duration of the precession process and whether or not the vortex is able to complete the precession process, vary among TCs. The predictability of the variety of precession process and subsequent RI is reported to be ultimately dominated by the chaotic nature of moist convection. Given the large influence of RI on the TC intensity forecasts, the further understandings in its uncertainty sources are necessary.

In this study, mechanisms that determine the variability of these precession processes are explored through sets of sensitivity and ensemble forecast experiments. We have used the Pennsylvania State University’s experimental real-time ensemble Kalman filter analysis of Hurricane Harvey (2017) that assimilated GOES-16 all-sky satellite radiances (which has an equivalent monitoring capability to Himawari-8) in convection-permitting Weather Research and Forecasting model (WRF-ARW) simulations. This analysis resulted in a highly accurate forecast of intensity and track, and realistically represented the storm’s rapid intensification. Starting with an analysis based on 18 hours of cycling data assimilation, we have conducted sensitivity experiments in which we reduced the initial atmospheric moisture amount by 5 to 20 %. Even initialized with the same wind field, and with fully developed convective updrafts and organization, the vortex tilt magnitude and the duration of precession are significantly modified by the inner-core moist processes. We explore the characteristics of the vortex structures that underwent short/long/uncompleted precession process, together with the theoretical background for these varieties of precession process by using a simplified toy-model. The results have implications for the design of future observation networks tasked with providing constraint on predictions of convections and rapidly intensifying tropical cyclones.