There are five different vertical motion options in HYSPLIT, three of
which are currently implemented in HYSPLIT-WEB (model vertical velocity,
isobaric, isentropic). As mentioned previously, the suggested default
is to use the vertical velocity field that is included with most meteorological
data. Other options may be required for special situations such as following
the transport of a balloon on a constant density surface, comparing isobaric
flow fields between data sets, or situations when the meteorological data’s vertical
velocity field may be too noisy compared with the time step at
which the data are available (high spatial resolution simulations).
In the isobaric and isentropic modes, vertical velocities are computed
from the equation,
W = (- ∂q/∂t – u ∂q/∂x – v ∂q/∂y) / (∂q/∂z)
where W is the velocity required for
the trajectory to remain on the q surface (pressure or potential
temperature). Note that the equation results in only
an approximation of the motion and a trajectory may drift from
the desired surface.
Shown below left is
the same trajectory from the previous example using the NAM 12 km vertical
velocity fields. To the right is the same
trajectory computed using the isentropic flow assumption and choosing the
Theta vertical coordinate option from the Display Options
menu. This graphic shows that the potential temperature
varied by only about 1 degree, however by assuming adiabatic flow conditions the
second trajectory ended in northeastern Louisiana after 84 hours instead of
north central Texas. The validity of the adiabatic flow assumption would need to
be assessed for this case.
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