From this representation, they construct an unstable
velocity field model.
Not exact matches
He notes that such a
model requires precise knowledge of gas
velocities as well as the strength and tilt of magnetic
fields in the penumbra, data the Swedish team hopes to obtain next year.
We first generate a stellar
field with planetary companions based on radial
velocity discoveries, use a planetary evolution
model assuming a variable fraction of heavy elements to compute the characteristics of transit events, then apply a detection criterion that includes both statistical and red noise sources.
the divergence of the
velocity field is in the first equation in
modeling the sloshing dynamics of ENSO http://contextearth.com/2014/05/02/the-soim-substantiating-the-chandler-wobble-and-tidal-connection-to-enso/
If you really want to consider thermal transport you need a
model of the
velocity field.