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SIMULATION OF DUST DEVILS

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Title: SIMULATION OF DUST DEVILS


1
SIMULATION OF DUST DEVILS
  • Zhaolin GU, PhD, Professor
  • Xian Jiaotong University
  • October , 2006, CCFD Forum , Tokyo University

2
Background
  • Atmospheric dust has important impacts on global
    and regional climates.
  • Some specific convective wind systems in the
    convective boundary layer (CBL), such as, dust
    storms, dust devils etc., can carry dust into the
    atmosphere.

3
Dust transportation in Northwestern arid area of
China
Dust storm Meso-scale meteorological process
Dust devil Micro-scale meteorological process
4
About dust storms Some pictures
The vision of Lanzhou Train Station at 1600,
April 10, 2004
The vision of Dunhuang Grottoes at 1600, April
10, 2004
The vision of Xian City Wall, April 9, 2006
The destroyed window by the dust storm, April 9,
2006
5
About dust storms Meteorological aspects
  • A Mesoscale meteorological process, composed of
    strong convection cells
  • Height of dust front 300-400 m
  • Length of dust front around 100 km
  • second dust front 10-20 km
  • Horizontal velocity more than 20
    ms-1
  • Vertical velocity more than
    15 ms-1
  • Temperature increment (DT ) 48 K
  • Pressure depression (Dp) 2.03.5 hPa
  • ?T and ?p are departures from ambient values of
    temperature and pressure.

6
About dust devils Meteorological aspects
  • A special case of convective vortex occurring in
    the atmosphere boundary layer.
  • The most common, small-scale dust transmitting
    system.
  • Maybe the primary atmospheric dust-loading
    mechanism in non-storm seasons
  • Mixing grains in dust devils becoming
    tribo-electrified.

7
Typical Observed Dust Devil Physical
Characteristics
  • Diameter Tens to 141 m
  • Height 300660 m
  • Horizontal velocity 5-20 ms-1
  • Vertical velocity 315 ms-1
  • Rotation sense Random
  • Temperature increment (?T ) 28 K
  • Pressure depression (?p) 2.54.5 hPa
  • ?T and ?p are departures from ambient values of
    temperature and pressure.

8
Inducement of dust devilsBackground vorticity
The Benards Convection in atmospheric boundary
layer
9
Inducement of dust devilsBackground vorticity
10
Inducement of dust devils Surface roughness
At h5.2m and h9.4m (V7 and V31 in the figure),
the value of tangential velocities at r50m is
different, where is far from the dust devil
center and maybe the boundary of the dust devil.
(P. C. Sinclair, 1973)
11
Inducement of dust devils Buoyancy
  • Heat radiation from the sun causing the rise of
    surface temperature
  • The temperature difference between the ground
    surface and the near-surface air parcels is over
    20-30K at sunny mid-day in deserts (Li J. F. ,
    Desert Climate, Meteorological Press, Beijing,
    2002)
  • The temperature difference is related to the heat
    flux on the surface.

12
Tool and methods for dust devil study
  • Field observation and test
  • Laboratory experiment, e.g. dry ice simulator in
    Arizona University
  • Numerical simulation
  • gas-solid two-phase flow

13
Numerical simulation
  • C. B.Leovy, Nature, 424 ,2003
  • Promise to be an important tool for interpreting
    laboratory and field observations of dust devils
  • (C. B.Leovy, Nature, 424 ,2003)
  • Getting insights into the dynamics of
    boundary-layer vortices
  • Two scale methods convective boundary layer
    (CBL) scale simulation, and dust devil-scale
    simulation

14
Dust devil-scale simulation method LES-
Lagrangian discrete phase model (LDPM) model
  • LES for the turbulent flow
  • LDPM for the grain movementone way coupling
  • Lifting of dust not actually appearing to be of
    major dynamical importance for the development of
    these vertical vortices ( P. C. Sinclair, J.
    Appl. Meteorol. 8,1969)

15
LES Equations
Continuity equation
Momentum equation
Energy equation
16
Dynamic subgrid scheme
Least-squares approach, Lilly (1992)
17
Dust devil scale LES modelboundary conditions
18
Involution of dust devils
  • a) Weak vortex phase b)
    Single cell phase
  • c) Transition phase of single cell to double
    cell d) Double cell phase .

19
Fine flow structure in the weak vortex phase
The updraft vectors and contours of updraft
velocity
20
Fine flow structure in the single cell phase
The updraft vectors and contours of updraft
velocity
21
Fine structure in transition phase of single cell
to double cell
The updraft vectors and contours of updraft
velocity
22
Fine flow structure in the double cell phase
The updraft vectors and contours of updraft
velocity
23
Daughter vortices in the double cell phase
24
Grain tracks in the mature phase flow
100mm
200mm
300mm
25
Dust lifting patterns in a dust devil
1-track of fine dust grains 2-track of medium
grains 3-track of large grains 4-small vortices
induced by the interaction of different
sized grains 5-general pattern of
interactions.
26
An illustration of the electric dust
devilFarrell et al. J. Geophys. Res., 109,2004
27
Observed near-surface patterns of terrestrial
dust devils
28
Modeled dust devils and typical parameters
29
Simulated near-surface patterns of dust devils
  • Near-surface shapes of dust devils simplified by
    the periphery of the rotating velocity contour of
    their cores.

30
Some problems in the numerical simulation
  • Grain size distribution
  • The influence of electrostatic field on the
    movement the positive-charged or negative-charged
    particles
  • The collision of particles resulting in charge
    neutralization and/or production, and then the
    particle movement

31
Particle population balance modelan example
32
Particle population balance model
  • A method connecting the microcosmic behaviors
    with the macroscopic token of dispersed phase
  • Description for different microcosmic behaviors
    in various process, such as crystal, growth,
    dissolution, breakage, aggregation, erosion,
    sinter and so on
  • Dealing with some process formation or
    transformation of rain, snow and hail, aerosol,
    sand storm, dust devils

33
Particle population balance equation (PPBE)
  • n (L, us, t, x) particle number density
    function
  • us particle velocity
  • L particle properties
  • X dimension
  • T time
  • S(L, us, x, t ) source tem, relating to the
    dispersed phase behaviors
  • F forces acting on the dispersed
    phase.

34
Particle population balance equation (PPBE)
Source term with no reaction
35
Solution of the PPBE
  • Classification method (CM)(N1)-fluid model, one
    fluid corresponding to the gas phase and N fluids
    to the different size dispersed phase
  • Quadrature method of moment (QMOM) (McGraw,
    Aerosol. Sci. Technol., 27, 1997)
  • Direct Quadrature method of moment (DQMOM)
    (Marchisio et al., Chem. Eng. Sci., 58, 2003)
  • Monte Carlo Methods

36
Prospect of CFD coupling with PPBE-1
  • Extending the physical understanding of the
    dispersed phase behaviors and process
  • QMOM and DQMOM, based on the fundamental
    statistical concepts on the microscopic level,
    are the promise to solve the PPBE
  • Reformulation of the coalescence and breakage,
    consistent with QMOM and DQMOM
  • Improving the formulation of the turbulence
    effects, interfacial transfer fluxes
  • Improving the formation of the boundary
    conditions (inlet and outlet conditions, wall
    boundary)

37
Prospect of dust simulation
  • The evaluation of dust flux at a level of dust
    devil on different surface
  • The possibility evaluation of occurring of dust
    devils in the region
  • The evaluation of regional dust flux from dust
    devils

38
Thanks for your attention!
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