Originally published as: Wardinski, I., Lesur, V. (2012): An extended version of the C3FM geomagnetic field model: application of a continuous frozen-flux constraint. - Geophysical Journal International, 189, 3, pp. 1409—1429. DOI: http://doi.org/10.1111/j.1365-246X.2012.05384.x Geophysical Journal International Geophys. J. Int. (2012) 189, 1409–1429 doi: 10.1111/j.1365-246X.2012.05384.x An extended version of the C3FM geomagnetic field model: application of a continuous frozen-flux constraint Ingo Wardinski and Vincent Lesur Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Section 2.3: Earth’s Magnetic Field, Germany. E-mail:
[email protected] Accepted 2012 January 11. Received 2012 January 11; in original form 2011 May 3 SUMMARY A recently developed method of constructing core field models that satisfies a frozen-flux constraint is used to built a field model covering 1957–2008. Like the previous model C3FM, we invert observatory secular variation data and adopt satellite-based field models to constrain the field morphology in 1980 and 2004. To derive a frozen-flux field model, we start from a field model that has been derived using ‘classical’ techniques, which is spatially and temporally smooth. This is achieved by using order six B-splines as basis functions for the temporal evolution of the Gauss coefficients and requiring that the model minimizes the integral of the third-time derivative of the field taken over the core surface. That guarantees a robust estimate of the secular acceleration. Comparisons between the ‘classical’ and the frozen-flux field models are given, and we describe to what extend the frozen-flux constraint is adhered.