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Figure 4 shows the map of the vertical down component of core field at the CMB for the year 2005.
In order to model primarily the core field at each epoch, a maximum number of 10 statistically significant coefficients were used, corresponding to a minimum wavelength of approximately 2200 km.
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Moreover, over the last decade, these models have dramatically improved the core field description at the core-mantle boundary and brought new insights into core dynamics.
At its core, field hockey is similar to soccer and ice hockey.
These magnets obtained core field and field integral uniformities at the parts in 10,000 level.
These dipoles run at two core field ranges, 0.05 T and 0.22 to 0.71 T.
Decomposition of the core field (top) into its constituents at inter-centennial (bottom left), sub-centennial (bottom middle) and inter-decadal (bottom right) time scales in terms of time-averaged energy maps for the period 1630 1950.
They provide a detailed picture of the internal field, of the core field secular variation and secular acceleration at Earth's surface.
We have revealed that the GRIMM and CM4 core field models, when each is truncated at the same degree for both MF and SV models, evidently involve the non-advective SV violating the FF condition and also the non-geostrophic SV violating the FF+TG condition.
Since CM4 has zero core field coefficients above degree 13, we supplement the model with synthetic coefficients at those degrees.
Harvest your core hay fields at optimum stage and plant corn later.
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Justyna Jupowicz-Kozak
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