Impact of solar background radiation on the accuracy of wind observations of spaceborne Doppler wind lidars based on their orbits and optical parameters

2019 
Due to the quantum properties of light, solar background radiation (SBR) is the main source of noise in daytime wind observations of spaceborne Doppler wind lidars (DWLs). In previous works, the impact of SBR on the observation accuracy of spaceborne lidars was assessed mainly using the default or worst-case scenarios. We assessed the impact of SBR on the observations of spaceborne DWLs using the global distributions of SBR in summer and winter, which were obtained based on their orbit parameters, view geometry and optical parameters. Three experiments illustrate that the uncertainty in wind observations increases with an increase in the quantiles of SBR. The uncertainties of the whole profiles of wind are greater than 2 m s−1 in the troposphere and 3 m s−1 in the stratosphere when the quantile of the SBR is greater than 85% in summer and 95% in winter, which do not satisfy the accuracy expectations of the European Space Agency (ESA) for spaceborne DWLs. The facts indicate that the impact of SBR cannot be negligible for the observations of spaceborne DWLs. Based on the orbit parameters, view geometry, and optical parameters of new spaceborne DWLs, engineers can assess the impact of SBR on the accuracy of wind observations from a global perspective using the method proposed in this paper.
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