weatherTimeSeries
Simulate I/Q signals for weather returns using a Monte Carlo approach
Since R2024a
Syntax
Description
This function generates I/Q signals for monostatic polarimetric weather radar
systems. Each weatherTimeSeries
simulation produces an independent radar return
from a particular resolution volume, or cell, that is modeled as a complex stationary Gaussian
random process using Monte Carlo method (see Algorithms).
Examples
Input Arguments
Output Arguments
Algorithms
weatherTimeSeries
simulates I/Q signals using a numerical Monte Carlo
approach combined with a statistical model that is based on the expected behavior of radar
returns from weather phenomena [2]
[3].
weatherTimeSeries
calculates scattering amplitudes for every time step using
relevant scattering parameters specified as input arguments to generate a time series.
Statistical model assumptions for radar returns from weather phenomena:
I/Q signals follow Gaussian distribution
Signal amplitude follows Rayleigh distribution
Signal phase follows uniform distribution
The first step in the Monte Carlo approach is to specify scattering amplitudes and generate random numbers for particle position and motion. Scattering amplitudes for a given resolution volume are modeled as combinations from random multiple scattering centers. Assume that scatterers within the resolution volume have the same size and a canting angle of zero (which implies that off-diagonal elements of the backscattering matrices have a value of zero). Then we have
where Pr is the received power for horizontal
polarization, N is the number of scatterers in the resolution volume, and
Vhh is the complex voltage for an individual
scatterer for horizontal polarization. At least 20 scatterers (N ≥
20
) are necessary to adequately model Gaussian random signals.
The amplitude of Vhh can be obtained as
Accordingly, the amplitude of the complex voltage for an individual scatterer for vertical polarization can be calculated as
where Zdr is the differential reflectivity on a linear scale.
In addition, the correlation coefficient ρhv is assumed to be reduced by a factor of due to the random scattering phase difference, where σδ is the standard deviation of random scattering phase difference, that is, . Then we have
For simplicity, it is assumed that , where σδh and σδv are standard deviations of the backscattering phase δh for horizontal polarization and the backscattering phase δv for vertical polarization, respectively.
Next, the scattered wave field for each particle is calculated. The amplitudes of complex voltage for an individual scatterer can be expressed as
where is the differential phase.
The final step is to calculate the total scattered wave fields. The total complex voltage of the resolution volume is
where is the incident wave vector and is the random position of each scatterer.
References
[1] Doviak, R. and D. S. Zrnic. Doppler Radar and Weather Observations, 2nd Ed. New York: Dover Publications, 2006.
[2] Zhang, G. Weather Radar Polarimetry. Boca Raton: CRC Press, 2016.
[3] Li, Z, et al. Polarimetric phased array weather radar data quality evaluation through combined analysis, simulation, and measurements. IEEE Geosci. Remote Sens. Lett., vol. 18, no. 6, pp. 1029–1033, Jun. 2021.
Version History
Introduced in R2024a