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It was tested with synthetic data in the Swarm Level-1b format.
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Only data from the Swarm A satellite are used in this study.
In a similar way, modelers can select Swarm L1b data using the Swarm L2-IBI product.
This is a safe assumption given the fact that the gravity field models produced from GRACE take advantage of the much more accurate KBR data, in comparison with the hl-SST data used in producing the Swarm models.
This difference in the data quality among the Swarm satellites is lost after the data correction.
In this paper we give an overview of the Swarm Level 2 Ionospheric Bubble Index (IBI), which is a standard scientific data of the Swarm mission.
Regarding the Swarm data, we used the Swarm Level-1b data product Mag-L, taking the latest available baseline 0408/09 data files in March 2016, for more than 28 months from 26 November 2013 to 30 March 2016.
This suggests the offset in the Swarm data needs to be independently determined for the along-track and cross-track directions.
Convection reversals were also identified in the CS10 statistical model at the same MLT location as those identified in the Swarm data.
Fictitious periods of one day and harmonics are possible due to inaccurate a priori models used to isolate the magnetospheric signal in the Swarm data.
During this period the CS10 statistical model for B z < 0, B y < 0, E sw = [1.20, 1.70] mV/m, and β > 10° is used to determine the offset in the Swarm data.
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