AMTD Atmospheric Measurement Techniques Discussions AMTD Atmos. Meas. Tech. Discuss. 1867-8610 Göttingen, Germany 10.5194/amt-2020-114 The influence of the signal-to-noise ratio upon radio occultation inversion quality Gorbunov Michael 1 2 3 A.M. Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences, Pyzhevsky per. 3, Moscow, 119017, Russia Hydrometcenter of Russia, Bolshoy Predtechensky per. 11-13, Moscow, 123242, Russia Spire Global Inc., 1825 33rd St, Boulder, CO 80301 Russian Foundation for Basic Research 20-05-00189 22 04 2020 2020 1 11 Copyright: © 2020 Michael Gorbunov 2020 This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit https://creativecommons.org/licenses/by/4.0/ This article is available from https://amt.copernicus.org/preprints/amt-2020-114/ The full text article is available as a PDF file from https://amt.copernicus.org/preprints/amt-2020-114/amt-2020-114.pdf

<p>In this paper, we investigate the influence of the signal-to-noise ratio (SNR) upon the radio occultation (RO) retrieval quality. We perform two series of numerical simulations: (1) with artificial RO data and, (2) with real COSMIC observations. We superimpose the simulated white noise with varying magnitudes upon both types of the observation data and evaluate the response in the statistics. The statistics use the reference fields of the analyses of European Centre for Medium-Range Weather Forecasts (ECMWF). Our simulations indicate that the effect of additive white noise has a threshold character: the influence of the noise is very low up to some threshold, but when the threshold is exceeded, the influence increases dramatically. Another conclusion is that, given RO observations of fair quality, the enhancement of the SNR cannot be expected to provide significant improvement in retrieval quality.</p>