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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/100397


    題名: Ensemble singular vectors and their use as additive inflation in EnKF
    作者: 楊舒芝;Yang, Shu-Chih;Kalnay, Eugenia;Enomoto, Takeshi
    貢獻者: 地球科學學院大氣科學學系
    關鍵詞: Colleges & universities;Data assimilation;Data collection;dynamic sensitivity;ensemble Kalman filter;Meteorology;Norms;singular vector
    日期: 2015-01-01
    上傳時間: 2026-04-21 14:00:31 (UTC+8)
    出版者: Taylor and Francis Ltd.;Stockholm: Stockholm University Press
    摘要: 摘要: Given an ensemble of forecasts, it is possible to determine the leading ensemble singular vector (ESV), that is, the linear combination of the forecasts that, given the choice of the perturbation norm and forecast interval, will maximise the growth of the perturbations. Because the ESV indicates the directions of the fastest growing forecast errors, we explore the potential of applying the leading ESVs in ensemble Kalman filter (EnKF) for correcting fast-growing errors. The ESVs are derived based on a quasi-geostrophic multi-level channel model, and data assimilation experiments are carried out under framework of the local ensemble transform Kalman filter. We confirm that even during the early spin-up starting with random initial conditions, the final ESVs of the first analysis with a 12-h window are strongly related to the background errors. Since initial ensemble singular vectors (IESVs) grow much faster than Lyapunov Vectors (LVs), and the final ensemble singular vectors (FESVs) are close to convergence to leading LVs, perturbations based on leading IESVs grow faster than those based on FESVs, and are therefore preferable as additive inflation. The IESVs are applied in the EnKF framework for constructing flow-dependent additive perturbations to inflate the analysis ensemble. Compared with using random perturbations as additive inflation, a positive impact from using ESVs is found especially in areas with large growing errors. When an EnKF is ‘cold-started’ from random perturbations and poor initial condition, results indicate that using the ESVs as additive inflation has the advantage of correcting large errors so that the spin-up of the EnKF can be accelerated.
    出版者: Stockholm: Stockholm University Press
    出版日期: 2015-12
    出處: Tellus A: Dynamic Meteorology and Oceanography, 2015-12, Vol.67 (1), p.26536--20
    資源來源: Taylor & Francis Journals Auto-Holdings Collection
    版權: 2015 S.-C. Yang et al. 2015
    版權: Copyright Co-Action Publishing 2015
    識別號: ISSN: 1600-0870
    識別號: ISSN: 0280-6495
    識別號: EISSN: 1600-0870
    識別號: DOI: 10.3402/tellusa.v67.26536
    顯示於類別:[大氣科學學系] 期刊論文

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