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Rapid modelling of the large scale magnetospheric field from Swarm satellite data

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Figure

Fig. 1. The Swarm L2PS FTMM processing chain. The items feeding into the algorithm from the top are input data and models
Table 1. The primary outputs of the Fast-Track Magnetospheric Model. The outputs will be released in Common Data Format (CDF) that will includebasic meta-data describing the output.
Table 2.Summary of the different models produced to test the FTMM algorithm and their distinguishing parameters
Fig. 2. Time series in nT of (external) q01 coefficient from the FTMM (top) and the TDS-1 reference model (middle) and their difference (FTMM minusTDS-1, bottom)
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