Basic Equations of Atmospheric Motion - Lecture 2 Flashcards
Eulerian view/derivative
consider changes at a fixed point in the fluid
Eulerian derivative: rate of change at a fixed point
∂/∂t
Lagrangian view/derivative
consider changes as you follow a particle (or parcel) of fluid
Lagrangian (or material) derivative: rate of change moving with a fluid parcel
D/Dt
v
v is the 3-dimensional velocity vector (u,v,w)
ρ [rho]
density=mass/volume
Coriolis force
f(k X v)
acts at right angles to the velocity
Because the Earth rotates on its axis, circulating air is deflected toward the right in the Northern Hemisphere and toward the left in the Southern Hemisphere.
P.g.f
pressure gradient force (p.g.f.) goes from high to low pressure
(1/density) *(grad pressure)
the rate at which the pressure increases divided by the density
g
gravity
F (Capitalised)
friction acts in opposite direction to velocity
f (lower case)
Coriolis parameter
f = 2Ω sin φ with Ω rate of Earth’s rotation ≈ 7.3x10-5 rad s-1 and φ is the latitude (north is positive)
k
vertical unit vector
p
pressure
hydrostatic balance
p.g.f=force of gravity
geostrophic balance/flow
p.g.f=Coriolis
the resulting geostrophic flow/wind/fluid is parallel to the isobars
isobars
lines on weather map that join places of equal pressure
-think level set
θ
potential temperature
usually θ=T(p/1000)^(2/7)
*the exponent is the Poisson constant