chapter 3 Flashcards

1
Q

The large scale flow in the atmosphere is nearly

A

geostrophic

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

the large scale flow in the atmosphere is nearly geostrophic

the ………………. and …………………. are …………………..

A

wind and mass fields are virtually in balance

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

the large scale flow in the atmosphere is nearly geostrophic

the wind and mass fields are virtually in balance

In such an atmosphere, the isobars are

A

straight and parallel and the density is a function of pressure alone (barotropic)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

If geostrophy is assumed, there is

A

no vertical motion and there is no change in the spatial patterns of the height of isobaric surfaces.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

If geostrophy is assumed, there is no vertical motion and there is no change in the spatial patterns of the height of isobaric surfaces.

Hence, geostrophy cannot be used to

A

understand the development of weather systems

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Hence, geostrophy cannot be used to understand the development of weather systems, which requires

A

time changes in the spatial patterns of the height of isobaric surfaces

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

………………………………………. can be used to understand the development of weather systems in ……………………………….

A

Quasi-geostrophic theory

a baroclinic atmosphere

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

In a baroclinic atmosphere, the

A

surfaces of constant pressure and density intersect each other forming solenoids that leads to direct circulation and vertical motion.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

In a baroclinic atmosphere, the surfaces of constant pressure and density intersect each other forming solenoids that leads to direct circulation and vertical motion.

In such an atmosphere,

A

the spatial pattern of height field changes with time.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Hence, the slight deviation of geostrophy (quasi-geostrophic) is of great importance to

A

understanding of atmospheric flow and weather systems

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

The Quasi-Geostrophic (QG) Momentum Equations

For this analysis, it is convenient to use the

A

isobaric coordinate system

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

For this analysis, it is convenient to use the isobaric coordinate system because

A
  • meteorological measurements are generally referred to constant pressure surfaces and
  • the dynamical equations are somewhat simpler in isobaric coordinates than in height coordinates.
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

The scalar and vector horizontal momentum equations in (x,y,z) coordinate system can be written as:

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

The scalar and vector horizontal momentum equations in (x,y,z) coordinate system can be written as:

where

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Equation (1) can be transferred to

A

x,y,p coordinates

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Equation (1) can be transferred to (x,y,p) coordinate system as follows:

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

LHS of Eq.(2) can be expanded as follows:

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

The QG Momentum Equations

Consider the momentum equation in vector form (Eq.3)

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

The QG Momentum Equations

after considering the momentum equation in vector form

now you should

A

Split the horizontal wind into geostrophic and ageostrophic components

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

The QG Momentum Equations

after concidering the momentum equation in vector form

plitting the horizontal wind into geostrophic and ageostrophic components:

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

The QG Momentum Equations

  • Consider the momentum equation in vector form (Eq.3):
  • Splitting the horizontal wind into geostrophic and ageostrophic components:

the next step is

A

Substituting (4) in the coriolis term in (3)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

The QG Momentum Equations

  • Consider the momentum equation in vector form (Eq.3):
  • Splitting the horizontal wind into geostrophic and ageostrophic components:

Substituting (4) in the coriolis term in (3):

A
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

Midlatitude ß-plane approximation

A

To retain the dynamical effect of the variation of the Coriolis parameter with latitude, f can be approximated by expanding its latitudinal dependence in a Taylor series about a reference latitude O| o

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

The QG Momentum Equations

  • Consider the momentum equation in vector form (Eq.3):
  • Splitting the horizontal wind into geostrophic and ageostrophic components:
  • Substituting (4) in the coriolis term in (3):

The next step is

A

Now, we replace the Coriolis parameter by f= f0 +ßy , so that the momentum equations (Eq.5) become:

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
25
The QG Momentum Equations * Consider the momentum equation in vector form (Eq.3): * Splitting the horizontal wind into geostrophic and ageostrophic components: * Substituting (4) in the coriolis term in (3): * Now, we replace the Coriolis parameter by f = f0 + ßy , so that the momentum equations (Eq.5) become: the next step is
Expanding the RHS of Eq.(6)
26
The QG Momentum Equations * Consider the momentum equation in vector form (Eq.3): * Splitting the horizontal wind into geostrophic and ageostrophic components: * Substituting (4) in the coriolis term in (3): * Now, we replace the Coriolis parameter by f = f0 + ßy , so that the momentum equations (Eq.5) become: * Expanding the RHS of Eq.(6) the next step is
The last term in (7) is very small, and can be ignored, so we now have:
27
The QG Momentum Equations * Consider the momentum equation in vector form (Eq.3): * Splitting the horizontal wind into geostrophic and ageostrophic components: * Substituting (4) in the coriolis term in (3): * Now, we replace the Coriolis parameter by f = f0 + ßy , so that the momentum equations (Eq.5) become: * Expanding the RHS of Eq.(6) * The last term in (7) is very small, and can be ignored, so we now have but the next step is
By the definition of the geostrophic wind
28
The QG Momentum Equations * Consider the momentum equation in vector form (Eq.3): * Splitting the horizontal wind into geostrophic and ageostrophic components: * Substituting (4) in the coriolis term in (3): * Now, we replace the Coriolis parameter by f = f0 + ßy , so that the momentum equations (Eq.5) become: * Expanding the RHS of Eq.(6) * The last term in (7) is very small, and can be ignored, so we now have * By the definition of the geostrophic wind the next step is
Substituting (9) in (8), the first two terms on the right-hand side of (8) cancel, resulting in
29
The approximate QG horizontal momentum equation thus has the form:
30
The rate of change of momentum following the total motion is approximately equal to
the rate of change of the geostrophic momentum following the geostrophic wind
31
The rate of change of momentum following the total motion is approximately equal to the rate of change of the geostrophic momentum following the geostrophic wind:
32
................................................................................. is approximately equal to the rate of change of the geostrophic momentum following the geostrophic wind
The rate of change of momentum following the total motion
33
As discussed earlier, though the atmosphere is close to being in geostrophic balance, the unbalanced component of the wind (the ageostrophic wind) is very important for
the dynamics of synoptic disturbances
34
Now, we derive an equation for the ageostrophic wind. For this, consider the
simplified horizontal momentum equations
35
Now, we derive an equation for the ageostrophic wind. For this, consider the simplified horizontal momentum equations:
36
Thus, the ageostrophic wind, which is the
deviation of the real wind from the geostrophic wind,
37
Thus, the ageostrophic wind, which is the deviation of the real wind from the geostrophic wind, is mathematically expressed as:
38
The ageostrophic wind is a measure of the
horizontal acceleration
39
As shown in figure, the ageostrophic wind points to the
left of the geostrophic acceleration (in NHS)
40
the ageostrophic wind figure
41
the bold line is representing
the height contour
42
the thin line represents
isotachs
43
the wind barbs represent
the geostrophic wind
44
the figure represents
a typical jet streak
45
ageostrophic wind is to the left of the geostrophic acceleration, the ageostrophic wind will be oriented as
46
the ageostrophic wind is divergent in
the right entrance and left-exit regions of the jet streak
47
the ageostrophic wind is convergent in
the other regions
48
the ageostrophic wind is divergent in the right entrance and left-exit regions of the jet streak, and convergent in the other regions This leads to
upward motion in the right-entrance and left-exit regions and downward motion in the other two regions of the jet streak.
49
The Isallobaric Wind – Vector Form step 1
Expanding the total derivative on the RHS of Eq.12:
50
Thus the forcing of the ageostrophic wind can be divided conveniently into the two parts, the
isallobaric wind and the advective wind.
51
the isallobaric wind is writen as
52
The scalar components of the isallobaric wind can be obtained as:
53
from the equation of isallobaric wind is determined by the
gradient of the isolines of do p/do t
54
what are the isolines
These are the lines connecting the equal amounts of surface pressure change (isallobars)
55
These are the lines connecting the equal amounts of surface pressure change (isallobars). In figure, we have:
56
The direction of the isallobaric wind is
perpendicular to the isallobars
57
The direction of the isallobaric wind is perpendicular to the isallobars, always pointing
towards the falling pressure
58
The direction of the isallobaric wind is perpendicular to the isallobars, always pointing towards the falling pressure (i.e., pointing to
the minimum value where the strongest pressure decrease) in surface pressure is located.
59
the second term on the RHS of is the
advective term
60
The scalar components of the advective wind can be written as:
61
The advective wind arises when
the geostrophic wind is not uniform, as in diffluent or confluent flow pattern.
62
In diffluent flow pattern (fig), the geostrophic wind
decreases in positive x-direction
63
In diffluent flow pattern (fig), the geostrophic wind decreases in positive x-direction due to
the larger spacing between the isobars indicating smaller pressure gradient.
64
In the analogous case of a confluent flow the wind speed will
increase
65
The divergence of the isallobaric wind is:
66
Divergence of the isallobaric wind When heights are falling: the isallobaric wind is ..........................
convergent
67
Divergence of the isallobaric wind When heights are rising: the isallobaric wind is ............................
divergent
68
The divergence of the advective wind can be obtained as: where عg is the ................................ and Vg.\-/عg is the ..................................
where عg is the geostrophic vorticity and Vg.\-/عg is the vorticity advection
69
When there is Positive Vorticity Advection (PVA): the advective wind is ..................
divergent
70
When there is Negative Vorticity Advection (NVA): the advective wind is ..........................
convergent