Abstract

Abstract. Global Navigation Satellite System Radio Occultation (GNSS-RO) refractivity climatologies for the stratosphere can be obtained from the Abel inversion of monthly average bending-angle profiles. The averaging of large numbers of profiles suppresses random noise and this, in combination with simple exponential extrapolation above an altitude of 80 km, circumvents the need for a "statistical optimization" step in the processing. Using data from the US–Taiwanese COSMIC mission, which provides ~1500–2000 occultations per day, it has been shown that this average-profile inversion (API) technique provides a robust method for generating stratospheric refractivity climatologies. Prior to the launch of COSMIC in mid-2006, the data records rely on data from the CHAMP (CHAllenging Mini-satellite Payload) mission. In order to exploit the full range of available RO data, the usage of CHAMP data is also required. CHAMP only provided ~200 profiles per day, and the measurements were noisier than COSMIC. As a consequence, the main research question in this study was to see if the average bending-angle approach is also applicable to CHAMP data. Different methods for the suppression of random noise – statistical and through data quality prescreening – were tested. The API retrievals were compared with the more conventional approach of averaging individual refractivity profiles, produced with the implementation of statistical optimization used in the EUMETSAT (European Organisation for the Exploitation of Meteorological Satellites) Radio Occultation Meteorology Satellite Application Facility (ROM SAF) operational processing. In this study it is demonstrated that the API retrieval technique works well for CHAMP data, enabling the generation of long-term stratospheric RO climate data records from August 2001 and onward. The resulting CHAMP refractivity climatologies are found to be practically identical to the standard retrieval at the DMI (Danish Meteorological Institute) below altitudes of 35 km. Between 35 and 50 km, the differences between the two retrieval methods started to increase, showing largest differences at high latitudes and high altitudes. Furthermore, in the winter hemisphere high-latitude region, the biases relative to ECMWF (European Centre for Medium-range Weather Forecasts) were generally smaller for the new approach than for the standard retrieval.

Highlights

  • Global Navigation Satellite System Radio Occultation (GNSS-RO) receivers onboard low-Earth-orbit (LEO) satellites have provided a nearly continuous global data record on the state of the atmosphere since the launch of the German CHAMP (CHAllenging Mini-satellite Payload) satellite in 2001

  • For the CHAMP satellite, we usually find between about 4000 up to 5000 profiles per month after applying the initial quality control used at the DMI

  • We studied the relative differences of mean–median combinations to the colocated ECMWF reference profiles, using a transition region between 50 to 60 km in a first attempt and comparing mean– median combinations where additional quality control was applied to combinations without additional quality control

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Summary

Introduction

Global Navigation Satellite System Radio Occultation (GNSS-RO) receivers onboard low-Earth-orbit (LEO) satellites have provided a nearly continuous global data record on the state of the atmosphere since the launch of the German CHAMP (CHAllenging Mini-satellite Payload) satellite in 2001. Ao et al (2012) and Gleisner and Healy (2013) independently described the use of averaged bending angles instead of individual profiles In this averageprofile inversion (API) technique, the required suppression of random noise is obtained through averaging a large number of profiles rather than smoothing and merging with a background. The feasibility of this approach was demonstrated with COSMIC data, which provides 1500–2000 profiles per day.

Data sets
Method
CHAMP bending-angle averages
Bending-angle quality control
Detailed comparison of new inversion to standard inversion
Findings
Discussion and conclusions
Full Text
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