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Improve robustness of wind field estimation #174
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The estimated wind field for each time step is a vector sum of two components, the advective field due to the translational motion of the storm and the rotational field. The rotational field intensity is a function of radius from storm eye. Previously, the advective field had no spatial dependence. This meant the entire spatial domain had some sort of background wind field (typically(!) a few m/s). In the event of a fast moving storm (say a decayed cyclone transitting the NA, this speed may be quite significant. For large domains like the USA, this could mean not insignificant background wind speeds many thousands of miles from the storm. I have decided that preventing this is worth the necessary assumptions and extra complexity. We now take the advective wind vector and multiply it by some reduction factor. This factor is the distance to storm eye, normalised by the radius to maximum winds, then tapered to 0 using a hyperbolic tangent function.
Previously, we used distance normalised by radius to maximum winds. Now, fade to 0 at 1,000km radius. Prevents a storm erroneously influencing the other side of a continent.
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