Basic Equations of Atmospheric Motion - Lecture 2 Flashcards

1
Q

Eulerian view/derivative

A

consider changes at a fixed point in the fluid
Eulerian derivative: rate of change at a fixed point
∂/∂t

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2
Q

Lagrangian view/derivative

A

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

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3
Q

v

A

v is the 3-dimensional velocity vector (u,v,w)

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4
Q

ρ [rho]

A

density=mass/volume

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5
Q

Coriolis force

A

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.

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6
Q

P.g.f

A

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

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7
Q

g

A

gravity

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8
Q

F (Capitalised)

A

friction acts in opposite direction to velocity

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9
Q

f (lower case)

A

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)

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10
Q

k

A

vertical unit vector

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11
Q

p

A

pressure

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12
Q

hydrostatic balance

A

p.g.f=force of gravity

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13
Q

geostrophic balance/flow

A

p.g.f=Coriolis
the resulting geostrophic flow/wind/fluid is parallel to the isobars

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14
Q

isobars

A

lines on weather map that join places of equal pressure
-think level set

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15
Q

θ

A

potential temperature
usually θ=T(p/1000)^(2/7)
*the exponent is the Poisson constant

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16
Q

T

A

temperature

17
Q

R

A

R is the specific gas constant (e.g. for dry air R = 287 J kg^–1 K^–1)

18
Q

adiabatic

A

heat does not enter or leave the system