Yu Yongfeng, Zhang Lifeng. The effect of different breeding length upon ensemble forecasting based on BGM. J Appl Meteor Sci, 2007, 18(1): 86-93.
Citation: Yu Yongfeng, Zhang Lifeng. The effect of different breeding length upon ensemble forecasting based on BGM. J Appl Meteor Sci, 2007, 18(1): 86-93.

The Effect of Different Breeding Length upon Ensemble Forecasting Based on BGM

  • Received Date: 2005-09-23
  • Rev Recd Date: 2006-08-15
  • Publish Date: 2007-02-28
  • Ensemble of initial conditions is the most important method in ensemble prediction, and how to generate the initial perturbations is crucial. Among all the methods to create perturbations for ensemble forecast, the "breeding of growing modes" (BGM) method has gained more and more favor for its good performance and almost "free" cost of computation. The breeding method simulates how fast-growing errors are "bred" in the analysis cycle. When a breeding cycle starts, an random initial perturbation field is added upon the control analysis. After some time's breeding, the most non-growing or decaying perturbations are filtered and the remainders can be mainly the fast-growing modes (perturbations). Accordingly, the perturbation's growth rate reaches certain value and its shape is also getting to the phase of slow change. In some sense, the perturbation in the breeding cycle reaches "saturation". This saturated status of perturbation is regarded as the estimate of the fast-growing modes in the realistic analysis error, thus is applied as the initial perturbation.From the idea of BGM method, one of the crucial questions may be when the breeding cycle ends, which is called "the breeding length" problem. In fact, the breeding length is the total time of breeding of growing modes (initial perturbations) in the ensemble prediction system. The general steps to determine the breeding length are: defining the saturated character of growing modes; investigating the increasing and saturating process of the growing modes, and defining an approximate saturated time; according to the saturated time, doing a great lot of experiments with different breeding lengths, and determining the final length by the forecast skill.The model is the global media-range forecast spectral model T63L9 and the NCEP/NCAR 6-hour reanalysis data in 1998 are used. The initial modes in the beginning of a breeding cycle are random fields with unified distribution in [-1, 1]. The value of 6-hour is chosen as the length of the integration in each cycle. Besides, "rescaling" method to make the magnitude of growing modes comparable with the initial analysis error in RMSE sense is used.Some researches show that, if an appropriate breeding scheme is adopted, the breeding of the growing modes can present a clear saturation character in both the norm (magnitude) and the form (shape) after 3—4 days of breeding. Based on these results, numerical experiments are done with breeding length of 2, 3 and 4 days. Conclusions from these experiments show that the ensemble prediction with different breeding length can all reach a certain extent improvement upon the control forecast, especially the betterments increase steadily after 4 days of forecast lead time. Results also show the differences among the three breeding lengths in the improvement upon the control forecast. It shows a better improvement in ensemble mean with a breeding length of 3 days than 2 days, but the 4-day breeding seems pretty much the same as the 3-day breeding. A pilot study on the spread and the Talagrand distribution of the ensemble members with different breeding lengths is also made. It seems that the most appropriate way is to choose 3-day as the breeding length in the system.
  • Fig. 1  Improvement quantity (column diagram) and quotiety (curve line) on the global 500 hPa geopotential height by the ensemble forecasts with respect to the control forecast

    Fig. 2  The improvement for the Northern hemisphere 500 hPa fields (others as in Fig. 1)

    Fig. 3  The improvement for the Asian 500 hPa fields (others as in Fig. 1)

    Fig. 4  The Talagrand distribution diagram of 500 hPa geopotential height

    (dash-dotted line represents the expected probability:f=0.125)

    Fig. 5  Spread of the ensemble forecasts relative to respective ensemle mean

    (shown are average values of 32 examples for geopotential height fields at 500 hPa and the Northern hemisphere is selected to be the analysis area)

    Table  1  The root-mean-square error (RMSE) weight skill for 500 hPa geopotential height of four groups of forecasting expriments

    Table  2  The forecasting days in which with 4-day breeding and with 3-day breeding have better improvements on the control forecast

    Table  3  The frequence root-mean-square (RMS) D and probability RMS Q of ensemble forecasts with respect to the expected values

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    • Received : 2005-09-23
    • Accepted : 2006-08-15
    • Published : 2007-02-28

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