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Transcript of Chapter 12: Mountain waves & downslope wind storms see also: COMET Mountain Wave PrimerCOMET...
Chapter 12: Mountain waves & downslope wind storms
see also: COMET Mountain Wave Primer
trapped lee waves
Quasi-stationary lenticular clouds result from trapped lee waves
Amsterdam Island,Indian Ocean
MODIS
Try a real-time animation of a cross section of isentropes/winds over the Snowy Range or Sierra Madre (source: NCAR’s WRF runs)
stack of lenticular clouds
12.1.1 linear theory: sinusoidal mountains,
no shear, constant stability, 2D
vertically-propagating waves:
N2 > U2k2 or a > 2pU/N (large-scale terrain)
evanescent waves:
N2 < U2k2 or a < 2pU/N (small-scale terrain)
a
u’<0
u’>0
warm
cold
L
H
u’>0cold
Lu’<0
warm H
Fig. 12.3
𝑑𝑈𝑑𝑧
=0𝑑2𝜃𝑑 𝑧 2=0
12.1.2 linear theory: isolated mountain (k=0), no shear, constant stability,
2D
a=1 km a=100 km
a << U/N or U/a >> N a >> U/N or U/a >> N
evanescent – vertically trapped vertically propagatingFig. 12.4 (Durran 1986)
witch of Agnesimountain
lzlx ~0
12.1.3 linear/steady vs non-linear/unsteady
trapped lee waves
both 2D
Fig. 12.5
linear theory – analytical solution numerical solution
Fig. 12.6
time-independent, i.e. steady
witch of Agnesi mtn, N constant, U increases linearly with height (from Durran (2003)
non-linear flow over 2D mountains
• Linear wave theory assumes that – mountain height h << flow depth, and – that u’<<U (wave pert. wind << mean wind)
– in other words, Fr >>1
• In reality Fr is often close to 1– Fr <1 : blocked flow, Ep>Ek
– Fr >1 : flow over mountain, Ek>Ep
• Non-linear effects caused by– terrain amplitude– large u’ (wave steepening and breaking)– transience
Nh
UFr Froude number
U
Nh
Fr
1non-dimensional mountain height
2D numerical simulations over Agnesi mountainThe lines are isentropes. The ND time Ut/a = 50.4
• Fr ~1.3: – no mtn wave breaking, no upstream
blocking– resemble linear vert. prop. mtn waves
• Fr ~1: – A weakly non-linear, stationary internal
jump forms at the downstream edge of the breaking wave.
– strong downslope winds near the surface
• Fr ~0.7: – jump propagates a bit downstream, and
becomes ~stationary– upstream blocking
• Fr ~0.4:– upstream flow firmly blocked– wave breaking over crest
(Lin and Wang 1996)
Froude #
Dz=
14
km
Dx=256 km
non-linear flow over an isolated 2D mountain:
transient effects Fr
2D numerical simulations over Agnesi mountainThe lines are isentropes. The ND time Ut/a = 50.4
• Fr ~1.3: – no mtn wave breaking, no upstream
blocking– resemble linear vert. prop. mtn waves
• Fr ~1: – A weakly non-linear, stationary internal
jump forms at the downstream edge of the breaking wave.
– strong downslope winds near the surface
• Fr ~0.7: – jump propagates a bit downstream, and
becomes ~stationary– upstream blocking
• Fr ~0.4:– upstream flow firmly blocked– wave breaking over crest
(Lin and Wang 1996)
Froude #
Dz=
14
km
Dx=256 km
non-linear flow over an isolated 2D mountain:
transient effects Fr
linear theoryVP waves (a >> U/N)
heig
ht
(km
)heig
ht
(km
)heig
ht
(km
)heig
ht
(km
)
Froude
num
ber
3.5 hrs 14 hrs 3.5 hrs 14 hrstime(for U=10 m/s
a = 10 km)
no wave breaking aloftno upstream blocking
wave breaking aloftno upstream blocking
wave breaking aloftupstream blocking
wave breaking is first
wave breaking aloftupstream blocking
blocking is first
isentropesearly late early late
wind anomalies
(Lin and Wang 1996)
12.2: flow over isolated peaks (3D): covered in chapter 13 (blocked flow)
wind
12.3 downslope windstorms
example: 18 Feb 2009
12.3 downslope windstorms
example: 18 Feb 2009
12.3 downslope windstormsexample: 18 Feb 2009
12.3 downslope windstormsexample: 18 Feb 2009
12.3downslope windstorms
Fig. 12.8
Fig. 12. 9 & 10
q (K)
u (m/s)
Is this downslope acceleration & lee ascent dynamically the same as a hydraulic jump in water?
Or is it due to wave energy reflection on a self-induced critical level & local resonance?
stable
less stable
Boulder windstorm 11 Jan 1972
2D simulations by Ming Xue, OUmountain halfwidth = 10 km horizontal grid spacing = 1 kminput stability and wind profile
animations of zonal wind u, and potential temperature q:(H=mountain height)1. H= 1 km2. H= 2 km3. H= 3 km
stable
less stable
stable
tropopause
strong wind shear
Grand Junction CO00Z 1972/01/12
This case study has been simulated by Doyle et al. (2000 in Mon. Wea. Rev.)
12.3.1 downslope windstorms: (a) hydraulic jump analogy
downslope windstorms: (a) hydraulic theory: shallow water theory
Fig. 12.12
downslope windstorms: (a) hydraulic theory - dividing streamline (Smith
1985)
Fig. 12.13
Smith 1985
dividing streamline
assumptions: steady (Bernouilli)inviscidhydrostatic & Boussinesq
𝜕2𝛿𝜕 𝑧2 +𝑙
2 𝛿=0
𝑙2=𝑁2
𝑈 2 −1𝑈
𝑑2𝑈𝑑𝑧2
Long’s equation
Scorer parameter (l)
downslope windstorms – hydraulic theory
• Shallow water eqns assume a density discontinuity (free water surface). Results qualitatively similar to a hydraulic jump can be produced in a numerical model with a stability (N) discontinuity
• Durran (1986) does this, using a two layer (Nlow>> Nup) constant wind U environment. Here the mountain height is varied.
hmountain =200 m
hmountain =800 mhmountain =500 m
hmountain =300 m
(numerical simulations by Durran 1986)
trapped lee waves
severe downslope
winds
trapped lee waves
Fig. 12.14
top of stable layer at 3 km in each case
~ subcritical flow
downslope windstorms – hydraulic theory
• Durran (1986) also examines the effect of the depth of the low-level stable layer.
d stable layer = 1000 m
mountain height fixed at 500 m in each case
severe downslope
winds
trapped lee waves
d stable layer = 4000 md stable layer = 3500 m
d stable layer = 2500 m
Fig. 12.15 (numerical simulations by Durran 1986)
~ subcritical flow
plunging flow in Laramie, east of the Laramie
Range
plunging flow + hydraulic jump?
barrier jet ?
downslope windstorms: (b) resonant amplification theory
Clark and Peltier (1984)Scinocca and Peltier (1993)Resonant amplification due to wave energy reflection at the level of wave breaking. The storm is transient, with this evolution according to 2D inviscid simulations:
1. wave steepening & breaking produces a well-mixed layer aloft, above the lee slope
2. This results in a (self-induced) critical level (U=0)
3. Ri<0.25 KH instability develops on top of the surface stable layer, squeezing that layer & increasing the wind speed (Bernouilli)
4. strong wind region expands downstream
shading shows isentropic layers
t=0 min
t=166 mint=160 min
t=96 mint=66 min
t=20 min
downslope windstorms:resonant amplification theory
shaded regions: Ri <0.25
linear
non-linear
Fr=20, Ri=0.1
Fr=20, Ri=0.1
Wang and Lin (1999)
transient flow (4 different times), non-linear
• asymmetric mountain, with gentle upstream slope and steep lee slope
• strong cross-mountain wind (>15 m s-1) at mtn top level
• cross mountain flow is close to normal to the ridge line
• stable layer near mountain top (possibly a frontal surface), less stable air above
• (not always) reverse shear such that the wind aloft is weaker, possibly even in reverse direction ( pre-existing critical level)
downslope windstorms: forecast clues
Note: The Front Range area sees less downslope winds than the Laramie valley in winter in part because of strong lee stratification, due to low-level cold air advected from the Plains states. Thus the strong winds often do not make it down to ground level.
12.4lee
rotorswind
Haimov et al. 2008 (IGARRS)
blue line applies to the 26 Jan 2006 case, shown below
26 Jan
Fig. 12.17
A downslope wind storm in the lee of the Sierra Nevada picks dust in the arid Owens Valley.
rotor cloud
h (s-1)
vorticity sheet
(no-slip BC)
reverseflow
downslopewindstorm