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Detailed File Information |
Description
This distribution contains the pfm9k geomagnetic field models and datafiles as presented in A. Nilsson, R. Holme, M. Korte, N. Suttie and M. Hill (2014): Reconstructing Holocene geomagnetic field variation: new methods, models and implications. Geophys. J. Int., doi: 10.1093/gji/ggu120. Please see this publication for details on the models
Files:
pfm9kfield.f - Fortran source code to predict time series of declination, inclination and intensity pfm9kcoefs.f - Fortran source code to calculate model Gauss coefficients for a given time
pfm9k.1 - pfm9k.1 model coefficients pfm9k.1a - pfm9k.1a model coefficients pfm9k.1b - pfm9k.1b model coefficients with uncertainties
pfm9k.0_DAT - Initial dataset, before outlier rejection and declination/intensity calibration pfm9k.0a_DAT - Initial timescale adjusted dataset, before outlier rejection and declination/intensity calibration pfm9k.1_DAT - Final dataset used for pfm9k.1 pfm9k.1a_DAT - Final dataset used for pfm9k.1a (adjusted timescales for the sedimentary data) pfm9k.1b_DAT - Final dataset used for pfm9k.1b |
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Instructions Unzip the archive and compile the Fortran code. Keep the model coefficient files in the same directory as the executable to run the programs. |
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Keywords Geomagnetic models, Geomagnetic secular variation, Archaeomagnetism, Palaeointensity, Lake Sediments, Holocene |
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