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TimeDependent Mountain Waves and Their Interactions with Large Scales

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Follow mountain-wave evolution in a realistic, but simple ... relative vorticity & velocity vector at surface. relative vorticity & velocity vector at surface ... – PowerPoint PPT presentation

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Title: TimeDependent Mountain Waves and Their Interactions with Large Scales


1
Time-Dependent Mountain Waves and Their
Interactions with Large Scales
  • Chen, C.-C., D. Durran and G. Hakim
  • Department of Atmospheric Sciences
  • University of Washington

2
The Goal
  • Follow mountain-wave evolution in a realistic,
    but simple time-varying large-scale flow.
  • Avoid artificial initialization
  • Capture the decaying phase of the waves
  • Examine feedback of the waves on the large-scale
    flow.

3
The Simulations
  • Numerical model
  • Boussinesq (compressible, nonhydrostatic)
  • f-plane
  • Terrain-following coordinates
  • Gravity-wave absorbing upper boundary
  • Parameterized subgrid-scale mixing
  • Multiply nested grids

4
The Nested Grids
?z 150500 m
5
Initial Condition Ingredients
  • Square wave in streamfunction plus a mean flow
  • Doubly periodic
  • ?x ?y2700 km

6
Initial Streamfunction
  • Mean wind 7.5 m/s
  • 0 lt local u lt 15 m/s
  • Period 100 hrs
  • (4 days)
  • Constant N
  • (2/3 lt Nh/u lt ?)

7
w velocity vector _at_ 5km (x-y plane)
8
w velocity vector _at_ 5km (x-y plane)
9
w theta turbulent mixing coefficient (x-z
cross-section)
10
w theta turbulent mixing coefficient (x-z
cross-section)
11
relative vorticity velocity vector at surface
12
relative vorticity velocity vector at surface
13
PV _at_ 295K 2.5km at t 55 hrs
14
PV _at_ 295K
15
PV _at_ 295K
16
PV _at_ 295K, t 0
17
PV _at_ 295K, t 100hrs
18
SummaryNear Mountain Flow
  • Near mountain evolution
  • Flow-around to flow-over to flow-around
  • Low-level blocking
  • Lee vortex generation and shedding
  • Wave breaking
  • Quasi-linear waves
  • Acceleration phase not mirror image of
    deceleration phase (period is 4 days)

19
SummaryScale Interaction
  • Localized dissipation creates PV dipoles in the
    lee of the barrier
  • Adiabatic interactions with the larger scale PV
    creates significant synoptic-scale anomalies
  • More analysis is on the way!
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