Satellite Microwave Remote Sensing Instrument Performance Estimate Using Monte Carlo Simulation

• Published in: SoutheastCon 2018 pp. 1 - 5
• Main Authors: Hossan, Alamgir, Jacobi, Maria, Jones, W.Linwood
• Format: Conference Proceeding
• Language: English
• Published: IEEE 01.04.2018
• Subjects: AV-H; Extraterrestrial measurements; GMF; Microwave measurement; Microwave radiometry; Ocean wind vector; Oceans; Precipitation Radar; Radar; Sea measurements; TMI; Wind; wind direction retrieval
• ISSN: 1558-058X
• DOI: 10.1109/SECON.2018.8479041

In this paper, we describe a Monte Carlo technique to simulate the active and passive remote sensor observations (normalized ocean radar backscatter, \sigma^{\circ} and brightness temperatures, Tb) and to estimate the resulting wind direction retrieval accuracy. A critical part of the simulation was to calculate the satellite/sensor geometry for each point along the orbital ground track. For this, we used the System Tool Kit (STK) orbital analysis software to determine the antenna pointing geometry and instantaneous-field-of-view (IFOV) locations (latitude, longitude, EIA, and azimuth) versus orbit position. Next, these simulated sensor IFOV's were spatially gridded into 0.25°xO.25° boxes and collocated with numerical weather model "nature-run" outputs, to obtain the desired geophysical parameters, namely wind speed and wind direction. Using existing radar and radiometer geophysical model functions (GMF), which relate ocean σ° and Tb with wind speed, relative wind direction, and earth incidence angle, the radar backscatter measurements and radiometer brightness temperatures (AV-H) were simulated, with realistic values of Gaussian noise added. Finally, a maximum likelihood estimation (MLE) procedure was applied to retrieve the wind directions, which were compared to the nature run WD, and the error statistical results are presented.