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The differences between the reconstructed fields and the reference (model) fields are then analyzed.
With distances we can model fields that satisfy boundary conditions while approximating the governing differential equations to arbitrary precision.
Both the covariance function and noise-to-signal ratio are derived from the analysis of the model fields.
The model is seeded with 450 "virtual" Argo floats, which are then advected by the model fields for 10 years.
Error bars in the plots correspond to the values of the residual root mean square (rms) difference between the observed and model fields for each distance bin.
Using these simulations as representations of the real ocean, the model fields are subsampled in space and time along a typical cruise track.
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A series of shaking table tests of model field were conducted using four shaking tables.
For classical electromagnetism, differential forms are natural objects to model field quantities on manifolds.
In the model field we also include intermittent turbulence, consistent with observations.
Comparison of the T96 model and observations from GOES-8 and GOES-9 shows that if the observed solar wind and IMF parameters are used to compute the model field, the model field is more stretched than the observed field.
We calculate the optical properties of the resulting triode mirror analytically on the basis of a simple model field distribution.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com