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Toward more complete magnetic gradiometry with the Swarm mission

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Figure

Fig. 1 Power spectra ŴhR(0 )n(rh), R(1 )n(rh) and R(2 )n(rh) of the observables (0), Ŵ(1) and Ŵ(2) at the Earth’s surface, h = 0 km, (dashed lines) and at  = 460 km altitude (solid lines) based on MF7 model
Fig. 2 Variance at satellite altitude (their analytical expressions, Eqs. (r = a + 460 km) of the estimated model parameters from each observable a  Ŵ(1), b  Ŵ(2) and c  Ŵ(0), based on 28), (30) and (32), respectively
Fig. 3 spherical distance, Left North–South spherical distance, SNS, i.e., the distance between consecutive positions (along-track) of Swarm Alpha
Fig. 5b. For reference, the radial lithospheric field result-ing from MF7 and CM5 (Sabaka et al
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