Fig. 10From: Performance assessment of radio occultation data from GeoOptics by comparing with COSMIC dataa Mean, b standard deviation of the fractional bending angle differences \(\left( {\frac{{{\text{BA}}_{{{\text{RO}}}} - {\text{BA}}_{{{\text{ECMWF}}}} }}{{{\text{BA}}_{{{\text{ECMWF}}}} }} \times 100} \right)\) and c counts of observationsBack to article page