2019
DOI: 10.1175/jtech-d-18-0160.1
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On the Importance of Statistical Homogeneity to the Scaling of Rain

Abstract: Scaling studies of rainfall are important for the conversion of observations and numerical model outputs among all the various scales. Two common approaches for determining scaling relations are the Fourier transform of observations and the Fourier transform of a correlation function using the Wiener–Khintchine (WK) theorem. In both methods, the observations must be wide-sense statistically stationary (WSS) in time or wide-sense statistically spatially homogeneous (WSSH) in space so that the correlation functi… Show more

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Cited by 5 publications
(8 citation statements)
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“…In order to be able to fully scale the rain rate, R, for example, in any spatial direction, it is most useful to have access to the radial power spectra that, in the case of statistically homogeneous rain, can also be transformed into the radial correlation function. (e.g., for a discussion see Jameson, 2019). Accomplishing estimates of the rainfall rates at high resolution is a challenging task that is, perhaps, best addressed using vertical pointing Doppler radar data in rain.…”
Section: Basic Considerationsmentioning
confidence: 99%
“…In order to be able to fully scale the rain rate, R, for example, in any spatial direction, it is most useful to have access to the radial power spectra that, in the case of statistically homogeneous rain, can also be transformed into the radial correlation function. (e.g., for a discussion see Jameson, 2019). Accomplishing estimates of the rainfall rates at high resolution is a challenging task that is, perhaps, best addressed using vertical pointing Doppler radar data in rain.…”
Section: Basic Considerationsmentioning
confidence: 99%
“…Thus, correlation functions are usually likely to be of little use when trying to tranform rainfall rate among different time and/or different spatial scales. Nor can they be transformed into power spectra with any general applicability(e.g., see [8]) via the Wiener-Khintchine theorem [16,17]. However, the power spectra of these data fields might still serve a useful albeit more narrow purpose.…”
Section: Convective Variable Rainmentioning
confidence: 99%
“…In particular the correlation function exists only when they are independent of the origin of the calculation in space or time over the spatial-temporal domain of interest. Similarly, power spectra, whether power fits or otherwise, only have generality when the data are wide-spread statistically homogeneous and statistically stationary (WSS) as emphasized for the rainfall rate in [8]).…”
Section: Introductionmentioning
confidence: 99%
“…In particular, the correlation function exists only when they (mean values and variance) are independent of the origin of their calculation in space or time over the spatial-temporal domain of interest. Similarly, power spectra, whether power fits or otherwise, exist but only have generality when the data are widespread, statistically homogeneous, and statistically stationary (WSS), as emphasized for the rainfall rate in [8]. According to the Wiener-Khintchine theorem, only when the data are WSS can one compute the auto-correlation function and proper power laws [1,2] Specifically, then, the first order of business is to see whether or not the temporalvertical MRR observations of rainfall rates are statistically homogeneous.…”
Section: Introductionmentioning
confidence: 99%