Copula-based downscaling of spatial rainfall: A proof of concept

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Abstract

Fine-scale rainfall data is important for many hydrological applications. However, often the only data available is at a coarse scale. To bridge this gap in resolution, stochastic disaggregation methods can be used. Such methods generally assume that the distribution of the field is stationary, i.e. the distribution for the entire (fine-scale) field is the same as the distribution of a smaller region within the field. This assumption is generally incorrect and we provide a proof of concept of a method to estimate the distribution of a smaller region. In this method, a copula is used to construct a bivariate distribution describing the relation between the scales. This distribution is then used to estimate the distribution of the fine-scale rainfall within a single coarse-scale pixel, by conditioning on the coarse-scale rainfall depth. © Author(s) 2011.

Figures

  • Fig. 1. A coarse-scale image of the rainfall depth (mm) (a), and its corresponding sub-pixel standard deviation (b).
  • Table 1. The seven events for which data was available, together with the number of rainy hours on that day, the average depth (mm) for all active pixels. The ratio expresses the proportion of dry to wet pixels within the radar image.
  • Fig. 2. A graphical representation of the framework used to retrieve the sub-pixel distribution. In the lower left, the copula is depicted, and in the top left, a slice of the copula representing P(U ≤ u,V ≤ v). Starting at the coarse-scale distribution, one obtains the probability (rank) of the value used for conditioning. This value is used in the copula to find the conditional probability of the fine-scale ranks, which are then ’projected’ using the fine-scale distribution to find the conditional probability of the sub-pixel rainfall depths.
  • Fig. 4. The fraction of zero rainfall cells at fine scale compared to the coarse-scale value.
  • Fig. 3. The coarse-scale empirical marginal distribution and the fitted coarse-scale marginal distribution.
  • Fig. 5. Regression analysis between log10(r) and log10( µλ′ µλ ), where µλ=E [0(k,θλ)] .
  • Fig. 6. Three copula densities, constructed from the same image, but using different scale steps r .
  • Fig. 7. An illustration of the EMD. The difference between the functions is shown as mass bars. These bars, or parts of them, need to be moved around in such a way that the dark gray bars (surplus) fill all the light gray bars (deficit). The distance they need to be moved is taken into account when calculating the EMD.

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CITATION STYLE

APA

Van Den Berg, M. J., Vandenberghe, S., De Baets, B., & Verhoest, N. E. C. (2011). Copula-based downscaling of spatial rainfall: A proof of concept. Hydrology and Earth System Sciences, 15(5), 1445–1457. https://doi.org/10.5194/hess-15-1445-2011

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