00000cab a22000003a 4500 UP-99796217609333297 Buklod 20231007234443.0 m |o d | ta 100616s xx d | ||r ||||| || DENGII eng Celandroni, N. Modeling Ka-band scintillation as a fractal process. pp. 164-172 We propose a model that describes the signal fading process due to scintillation in the presence of rain. We analyzed a data set of uplink (30 GHz) and downlink (20 GHz) attenuation values averaged over 1 s intervals. The data are samples relative to ten significant events, for a total of 180 000 s recorded at the Spino d'Adda (North of Italy) station using the Olympus satellite. Our analysis is based on the fact that the plot of attenuation versus time recalls the behavior of a self-similar process. We then make various considerations, and propose, a fractional Brownian motion model for the scintillation process. We describe the model in detail, with pictures showing the apparent self-similarity of the measured data. We then show that the Hurst parameter of the process is a simple function of the rain fade. We describe a method for producing random data that interpolate the measured samples, while preserving some of their interesting statistical properties. This method can be used for simulating fade countermeasure systems. As a possible application of the model, we show how to optimize fade measurement times for fade countermeasure systems 20 GHz. 30 GHz. Hurst parameter. Ka-band scintillation modelling. Olympus satellite. SHF. Spino d'Adda. Attenuation measurements. Downlink. Fade countermeasure systems. Fade measurement times optimization. Fractal process. Fractional Brownian motion model. Measured data. Measured samples interpolation. Rain. Rain fade. Random data. Self-similar process. Signal fading. Statistical properties. Uplink. IEEE Journal on selected areas in communications 17, 2 (1999). FO UPD DENG-II Article