A modified sliding spectral method and its application to COSMIC radio occultation data
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In the moist lower troposphere, a limitation of the sliding spectral (SS) method is the restriction of the resolution of bending angle profiles because of the atmospheric multipath effect and noise. A modified sliding spectral (MSS) method is proposed in this paper to improve the inversion resolution of SS method in the moist lower troposphere. Simulation results show that the noise in the signal may cause inversion error in the classical SS method. The MSS method can decrease the influence of the noise to some extent. The SS and MSS methods were used to process COSMIC (Constellation Observing System for Meteorology, Ionosphere, and Climate) atmPhs profiles from DOY (day of year) 71–DOY 100 in 2007. The retrieved refractivity profiles were compared with those from the corresponding ECMWF (European Centre for Medium-Range Weather Forecasts) analysis. The results show that the SS method contains systematic positive biases in the 3–10 km height range and systematic negative biases below 3 km. The MSS method, in comparison to SS method, has decreased the maximum positive bias in the range of 3–10 km height from 0.37% to 0.23% in the northern hemisphere, from 1.3% to 0.25% in the tropics, and from 0.60% to 0.35% in the southern hemisphere. The biases of the MSS method are comparable to those announced for the COSMIC atmPrf profile; the latter is inverted by full spectrum inversion (FSI) method.
KeywordsCOSMIC occultation multipath inversion MSS method
- Anthes R A, Bernhardt P A, Chen Y, Cucurull L, Dymond K F, Ector D, Healy S B, Ho S P, Hunt D C, Kuo Y H, Liu H, Manning K, McCormick C, Meehan T K, Randel W J, Rocken C, Schreiner W S, Sokolovskiy S V, Syndergaard S, Thompson D C, Trenberth K E, Wee T K, Yen N L, and Zeng Z 2008 The COSMIC/FORMOSAT-3 mission: Early results; Bull. Am. Meteor. Soc. 89 (3) 313–333, doi: 10.1175/BAMS-89-3-313.CrossRefGoogle Scholar
- Beyerle G, Hocke K, Wickert J, Schmidt T, Marquardt C, and Reigber C 2002 GPS radio occultations with CHAMP: A radio holographic analysis of GPS signal propagation in the troposphere and surface reflections; J. Geophys. Res. 107(D24) 4802, doi: 10.1029/2001JD001402.
- Fjeldbo G, Kliore A J and Eshleman V R 1971 The neutral atomosphere of Venus as studied with the Mariner V radio occultation experiments; Astron. J. 76(2) 123–140.Google Scholar
- Kursinski E R, Hajj G A, Leroy S S and Herman B 2000 The GPS radio occultation technique; Terr. Atmos. Oceanic Sci. 11 (1) 53–114.Google Scholar
- Lohmann M S, Jensen A S, Benzon H H and Nielsen A S 2003 Radio occultation retrieval of atmospheric absorption based on FSI; Scientific Report 03-20 Danish Meteorological Institute, Copenhagen.Google Scholar