日本地球惑星科学連合2025年大会

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[J] ポスター発表

セッション記号 A (大気水圏科学) » A-CG 大気海洋・環境科学複合領域・一般

[A-CG47] 海洋と大気の波動・渦・循環の力学

2025年5月25日(日) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:大貫 陽平(九州大学 応用力学研究所)、久木 幸治(琉球大学)、杉本 憲彦(慶應義塾大学 法学部 日吉物理学教室)、松田 拓朗(北海道大学地球環境科学研究院)

17:15 〜 19:15

[ACG47-P03] Intercomparison of dynamic energy cycles between JRA-55 and JRA-3Q

*小原 弘聖1菅野 湧貴2伊藤 純至1岩崎 俊樹1 (1.東北大学、2.電力中央研究所)


キーワード:波動平均流相互作用、子午面循環、エネルギーサイクル

In this study, the dynamic energy balances of reanalyses are estimated using the three-box model in the mass-weighted isentropic zonal mean framework (Uno and Iwasaki, 2006). In this box model, atmospheric energy is classified into three forms: zonal available potential energy (Az), zonal mean kinetic energy (Kz), and wave energy (W). By computing residuals between energy conversion and generation, the dynamic energy balances for Az (Error-Z) and W (Error-W) were evaluated as indices of the precision of reanalysis datasets.
Reanalysis datasets are crucial for better understanding atmospheric dynamics and the historical climate changes. It is useful to clearly evaluate the precision of reanalysis. Kosaka et al. (2024) reported that forecast models used for the Japanese Reanalysis for Three Quarters of a Century (JRA-3Q) improved temperature and heating profiles, as well as radiation budgets, compared to the previous Japanese 55-year Reanalysis (JRA-55; Kobayashi et al. 2015). JRA-3Q was validated with other datasets or observations. Meanwhile, evaluating reanalysis datasets from various perspectives remains essential. Therefore, in this study, JRA-3Q was assessed from the standpoint of dynamic energy balance consistency.
We evaluated the JRA55 and JRA3Q using the two indices for the period from December 1990 to November 2020, focusing in particular on December–February (DJF) and June–August (JJA). The mean values of the two indices show that dynamic energy balances are improved in JRA-3Q compared to those in JRA-55. In DJF (JJA), Error-Z decreased from 3.2% (22%) in JRA-55 to 2.8% (20%) in JRA-3Q. Similarly, Error-W decreased from -9.4% (19%) in JRA-55 to -6.1% (-9.9%) in JRA-3Q. These results imply that the systematic part of increment from data assimilation in JRA-3Q could be smaller, resulting from the improvement of physics parameterization packages of the global NWP model. The errors in the dynamic energy balance are much larger in JJA than in DJF, which is caused by strong diurnal variability of global mean diabatic generation of Az and W in JJA.