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Title: Workshop Agenda


1
Workshop Agenda
Model Overview Model history and features Computational method Trajectories versus concentration Code installation Model operation Example calculations Updating HYSPLIT Meteorological Data Data requirements Forecast data FTP access Analysis data FTP access Display grid domain Vertical profile Contour data Examples 1-5 Particle Trajectory Methods Trajectory computational method Trajectory example calculation trajectory model configuration Trajectory error Multiple trajectories Terrain height Meteorological analysis along a trajectory Vertical motion options Pollutant Plume Simulations Modeling particles or puffs Concentration prediction equations Turbulence equations Dispersion model configuration Defining multiple sources Simulations using emission grids Concentration and particle display options Converting concentration data to text files Example local scale dispersion calculation Special Topics Automated trajectory calculations Trajectory cluster analysis Concentration ensembles Chemistry conversion modules Pollutant deposition Source attribution using back trajectory analysis Source attribution using source-receptor matrices Source attribution functions GIS Shapefile output KML/KMZ output Customizing map labels Scripting for automated operations Extra Topics Modeling PM10 emissions from dust storms Restarting the model from a particle dump file
82
82
2
Modeling Particle Motion or Particle
Distributions (Puffs)
  • To compute air concentrations its necessary to
    follow all the particles needed to represent the
    pollutant distribution in space and time. This
    can be done explicitly by following the
    trajectory of each particle, where a random
    component is added to the mean velocity (from the
    meteorological model), to define the dispersion
    of the pollutant cloud. 
  • In the horizontal, the computations can be
    represented by the following equations
  • Xfinal(t ?t) Xmean(t ?t) U'(t
    ?t)?t, where, U'(t ?t) R(?t) U'(t) U''(1 -
    R(?t)2)0.5, (horiz. turbulent velocity)
  • R(?t) exp(-?t/TLu), (auto-correlation
    coefficient)
  • TLu is the Lagrangian time scale
  • U'' su?, where ? is a random number with
    mean of 0 and s of 1. 
  • The computations can be simplified, if instead of
    modeling the motion of each particle, we compute
    the trajectory of the mean particle position and
    the particle distribution. The standard deviation
    of the particle distribution can be computed from
    all the particles,
  •        ______ s2  (Xi-Xm)2
  • or it can be computed without following
    individual particles by assuming a distribution
    shape (puff) and relationship to the local
    turbulence.  Many different formulations can be
    found in the literature. dsh/dt v2 su su
    (Ku / TLu)0.5
  • These computations are set in the Advanced /
    Configuration Setup / Concentration menu, which
    modifies the SETUP.CFG file.

83
3
Modeling Particle Motion or Particle
Distributions (Puffs)
  • Below, note the initial differences between the
    simulation using the 3D particle distribution
    (left) and the top-hat puff center position
    method (right). Without the random motion
    component, the top-hat puff positions follow a
    straight line during the initial few hours until
    vertical motions or horizontal divergence begins
    to act on the particles. In this particular case
    the primary reason for the sudden expansion of
    the puff-particles is that they have mixed to
    higher levels and we are seeing the differential
    horizontal advection acting upon the particles.

3D Particle Distribution
Top-hat Puff Center Positions
84
4
Modeling Particle Motion or Particle
Distributions (Puffs)
  • The previous example showed a snapshot of the
    particle or puff center positions after 12
    hours.  Air concentrations are computed by
    summing each particles mass as it passes over
    the concentration grid.
  • In the particle model mode, the concentration
    grid is treated as a matrix of cells, each with a
    volume defined by the grid dimensions.  Therefore
    the concentration is just the particle mass
    divided by the cell volume
  • 3D Particle      ?C q(?x ?y
    ?z)-1 Top-Hat           ?C q(? r2
    ?z)-1 Gaussian        ?C q(2? sh2 ?z)-1 e-
    0.5x2/sh2
  • In the puff model mode, the concentration grid is
    considered as a matrix of sampling points, such
    that the puff only contributes to the
    concentration if it passes over the sampling
    point.  In the puff calculation mode it is
    possible for a puff to pass between points and
    not be shown on the display
  • Top-Hat           ?C q(? r2
    ?zp)-1 Gaussian        ?C q(2? sh2 ?zp)-1 e-
    0.5x2/sh2

85
5
Modeling Particle Motion or Particle
Distributions (Puffs)
  • Shown below are the concentration patterns
    associated with the particle (left) and puff
    (right) distributions from the previous example. 
    Note that the puff distribution is smoother but
    also initially somewhat broader.  In this
    particular case, the horizontal puff growth
    equations give larger values than the particle
    expansion. The noisy particle distribution
    indicates that more particles than 5000 used are
    needed to better represent the horizontal
    distribution.

3D Particle Distribution
Top-hat Puff Center Positions
86
6
Turbulence Equations
The method by which the meteorological data are
evaluated to determine the turbulent velocities,
used in either the puff or particle computation,
is set in the Advanced / Configuration Setup /
Concentration menu (below-left). Clicking on the
Configure the TURBULENCE method button produces
the menu given below-right.
87
7
Turbulence Equations
  • Turbulence Computation Methods
  • Standard velocity deformation - The default
    standard method computes the mixing using a
    diffusivity approach based upon vertical
    stability estimates and the horizontal wind field
    deformation
  • Kz k wh z (1 - z/Zi)2
  • Kh 2- 0.5(c ?)2 ?u/?y ?v/?x
  • Short-range similarity (fluxes/profile) - In
    shorter range dispersion simulations (lt 100 km)
    the deformation parameterization used in
    conjunction with larger scale meteorological
    fields will not reflect the diurnal variations in
    horizontal turbulence. In these situations its
    desirable to use the short-range
    parameterizations in which the turbulent
    velocities are computed directly from the
    stability parameters, heat and momentum fluxes,
    if available, or derived from the wind and
    temperature profiles.  The user has the option of
    forcing the use of the profile to compute
    stability rather than the fluxes. This may be
    desirable, especially if the fluxes represent
    averages rather than instantaneous values. The
    boundary layer velocity variances are defined as
    a function of u, w, and Zi.  This method does
    not use the diffusivity and no assumptions are
    required about turbulent scales. For instance, in
    the stable/neutral boundary layer
  • w'2 3.0 u2 (1 z/zi)3/2
  • u'2  4.0 u2 (1 z/zi)3/2
  • v'2   4.5 u2 (1 z/zi)3/2

88
8
Turbulence Equations
  • Turbulence Computation Methods (Cont.)
  • Input meteorological model TKE - If the turbulent
    kinetic energy (TKE) field is available from the
    meteorological model, then the velocity variances
    can be computed from its definition and the
    previous velocity variance equations to yield
    relationships with TKE
  • E 0.5 (u2 v2 w2)
  • w2 0.32 E,  u2 0.74 E,  v2 0.85 E
  • u2   v2 0.36 w2
  • TKE and mixed layer defined TKE The TKE can be
    used with the mixed layer depth as estimated from
    the TKE profile.
  • Turbulence velocity variance - Some
    meteorological data sets may already contain the
    3-dimensional component velocity variances.  This
    would normally be the case for data that have
    been generated from local measurement programs.

The Puff Growth Computation Method section is
used to define either the Linear or Square Root
with time dispersion equation for the horizontal
growth rate of puffs. This option does not affect
particle dispersion. The user also has the
ability to set ratios of the vertical to the
horizontal turbulence for daytime and nighttime
in the Turbulence Aniosotropy Factors section
(click the Help button for more details).
89
9
Dispersion Model Configuration
  • The control file (CONTROL) for dispersion
    simulations is configured from the Concentration
    / Concentration Setup menu tab.  The
    concentration setup layout is identical to the
    trajectory menu with the exception of an
    additional button to set the emissions,
    deposition, and concentration grid (top right).
  • The Pollutant, Deposition and Grids setup button
    will bring up a submenu (lower right) with three
    options (Pollutant, Grids, Deposition).
  • To make modifications, enter the number of
    pollutants to define in the Num box and then
    click on the Specie or Grid to access the
    next menu.
  • The pollutant emission rate and deposition must
    be set for each pollutant. 
  • Several independent concentration grids may be
    defined for each simulation. However, they may be
    nested in space or time, if desired. 
    Concentrations for each pollutant species are
    output on all grids.

90
10
Dispersion Model Configuration
  • Definition of Pollutant
  • An arbitrary 4-character field identifies each
    pollutant.
  • The Emission rate is mass units per hour. The
    actual mass unit is not specified, so for
    instance, if the units are kg, then concentration
    output will be in kg/m3.  Any unit is acceptable,
    however some chemical conversion modules require
    specific units.
  • The Hours of emission may be defined in
    fractional hours.
  • The pollutant Release start can be set to any
    time at or after the start of the simulation.  As
    is true for all time units, zeros default to the
    simulation start time in the main menu.  Zero for
    the month and non-zero values for day and hour
    cause those values to be treated as relative to
    the simulation start time.

91
11
Dispersion Model Configuration
  • Definition of Concentration Grid
  • Each concentration grid must be defined. 
  • Zeros for the grid center default to the source
    location. 
  • The grid spacing is especially important in
    concentration computations in determining the
    cell size (particles) or sampling resolution
    (puffs). 
  • When multiple levels are defined, each height
    represents the top of the cell (particles) or
    actual height (puffs). 
  • The averaging time (Avg) starts at the sampling
    start time for the hours/minutes specified in the
    output interval. 
  • Snapshot concentrations (Now) are defined as the
    average over one time-step at the time interval
    specified. Max will save the maximum
    concentration at each grid point over the
    duration of the output interval.

92
12
Example Dispersion Calculation
  • Run the dispersion model using these settings
  • Source 28.50N, 80.70W _at_ 10.0 m
  • Meteorology NAM 12 km
  • Emission 12 hrs beginning 1200 UTC on 19 Dec
    2005
  • Output Snapshot after 12 hrs between the ground
    and 100 m-agl
  • Top-hat-horizontal, particle-vertical
  • 5000 particles
  • Run Standard Model

93
13
Example Dispersion Calculation
  • Results
  • Change the map background file from arlmap to
    floridamap in the Concentration Display menu and
    display the results.
  • The resulting graphic should be the same as that
    shown (right).

The floridamap file and other high resolution map
backgrounds can be downloaded from the NOAA ARL
website at http//www.arl.noaa.gov/ready/hysp_uti
l.html
94
14
Example Dispersion Calculation
  • All HYSPLIT simulations generate a text MESSAGE
    file, which contains diagnostic information about
    the calculation.  Use the View MESSAGES link from
    the Advanced menu tab to view the last MESSAGE
    file. In this case (below), at the end of the
    simulation, 12.00014 units of mass were still on
    the domain. The vertical mass distribution showed
    more than 80 of the mass to be within 1000 m of
    the ground.  The vertical mass distribution is
    computed independently of the vertical
    concentration grid.

95
15
Defining Multiple Sources
  • Now run the dispersion model for 2 sources
    using these settings
  • Source1 28.50N, 80.70W _at_ 10.0 m
  • Source 2 28.0N, -80.0W _at_ 10.0 m
  • Meteorology NAM 12 km
  • Emission 6 hrs beginning 1200 UTC on 19 Dec 2005
  • Output 6 hr average concentration between the
    ground and 100 m-agl
  • Top-hat-horizontal, particle-vertical
  • 5000 particles
  • Run Standard Model

96
16
Defining Multiple Sources
  • A second source added at location 28.0N and 80.0W
    results in two adjacent, almost identical
    plumes. 
  • Note that the emission rate of 1 unit per hour is
    applied to each source individually.

97
17
Defining Multiple Sources
  • The emission rate can be set for each source by
    including that information after the release
    height in the Starting Location Setup menu. (A
    fifth field can be added that sets an initial
    plume area in square-meters, but is only valid
    for puff simulations.)
  • In the example shown here (top right), the
    emission rate of the second source has been
    increased to 10 units/hr
  • The concentrations in the second plume (right)
    have increased by the same amount as the emission
    increase (10).
  • To display the same concentration levels as the
    last graphic, change the output contour levels in
    UserSet to 1.0E-091.0E-101.0E-111.0E-12

98
18
Simulations using Emissions Grids
  • Option 1 Matrix Approach
  • An emission matrix is defined using three
    locations the first two represent the lower left
    and upper right grid corners, respectively, and
    the third represents the grid spacing.
  • Example to run  Start sources every 0.5 degrees
    between the grid corners (27.0, -82.0) and (30.0,
    -79.0). Leave all other parameters the same as
    the last Florida example, however increase the
    maximum number of particles to at least 50,000 in
    the Advanced / Configuration Setup /
    Concentration menu.
  • Run the model from the Concentration / Special
    Simulations / Run Matrix menu option.
  • Prior to running the model, the CONTROL file is
    redefined with 49 starting locations (right).

99
19
Simulations using Emissions Grids
  • The result (top right) shows 49 plumes over a
    uniform 0.5 degree grid.
  • To make the graphic less noisy, from the
    Concentration Display menu, turn off the source
    location labeling and remove the black contour
    lines from the graphic by setting the contour
    outlines to none
  • Execute the display to create a considerably
    simplified graphic (below right).

100
20
Simulations using Emissions Grids
  • Option 2 Emissions File Approach
  • Another approach is to define an emissions file,
    which tabulates hourly emission rates by
    location. 
  • An emission.txt file defines the grid to which
    those emissions data will be accumulated and is
    located in the working directory. 
  • A simulation using this approach for the same
    case (right) is almost identical to the previous
    matrix run. 
  • The CONTROL file must define the lower left and
    upper right corners of the desired emission
    domain, which may be larger or smaller than the
    data available. 
  • Due to the continuous emissions at many
    locations, these simulations may require the
    maximum number of particles be increased from the
    default value as was done for the matrix run.
  • Information on the format of the emissions file
    and the emission text file can be found in the
    HYSPLIT User's Guide under Advanced / Special
    Topics (S441).

101
21
Concentration and Particle Display Options
Now, we will look at the particle distributions
for the Florida case for various source terms.
  • Setup the following run
  • Delete the emission.txt and emission.asc files
    from the working directory if used previously.
  • Source1 28.50N, 80.70W _at_ 10.0 m
  • Meteorology NAM 12 km
  • Emission 6 hrs beginning 1200 UTC on 19 Dec 2005
  • Output snapshot at 6 hours between the ground
    and 100 m-agl
  • 3D particle horizontal and vertical
  • 500 particles
  • Dump the particles after 6 hours (right)
  • Run Standard Model

102
22
Concentration and Particle Display Options
  • Results
  • Turn back on source labeling and color contour
    outlines in the Concentration Display menu and
    execute the display.
  • The resulting graphic should be the same as that
    shown (right).
  • The concentration output clearly shows a noisy
    pattern indicating too few particles were defined
    to adequately represent the plume.

103
23
Concentration and Particle Display Options
  • Setup the following runs
  • Rerun the last case, but use 5,000 and 50,000
    particles.
  • Make sure the maximum number of particles is
    greater than 50,000.
  • The particles are beginning to better define the
    plume, but at the expense of longer computational
    time.

5,000 Particles
50,000 Particles
104
24
Concentration and Particle Display Options
  • Results
  • To speed up the run without loosing the plume
    structure, change the type of run from a 3D
    particle to a top-hat-horizontal
    particle-vertical and reduce the number of
    particles to 2500 (500 is still not enough to
    resolve the plume.
  • The resulting plume (right) covers a similar
    footprint as the 50,000 3D particle run.

105
25
Concentration and Particle Display Options
  • Particle Display
  • In addition to the standard display of particle
    concentrations, individual particle positions can
    also be displayed on a map.
  • The Concentration / Display Options / Particle
    menu (right) has options to show snapshot
    particle distributions, assuming that the
    particle dump option was set in the Advanced /
    Configuration Setup / Concentration menu before
    running the particle simulation.
  • Horizontal, vertical, and cross-sectional views
    are available.
  • Other options include color-coding the particles
    by mass size (Mass Sizing), by height (Color
    Scale) or output as a shapefile (GIS).

26
Concentration and Particle Display Options
  • Particle Display
  • Rerun the 50,000 3D particle simulation to
    produce a PARDUMP particle dump file.
  • Then choose the particle vertical cross-section
    with the color Scale option checked.
  • As seen in the graphic (right), the center line
    of the cross-section is drawn automatically based
    upon the particle distribution.
  • The particles toward the west are at a higher
    level than those to the east.

27
Concentration and Particle Display Options
  • Pointer Select Concentration Display
  • Another display option is to view the
    concentration values directly on the grid without
    any interpolation through the Concentration /
    Display Options / Pointer Select tab.
  • This option will draw the entire concentration
    domain as defined in the concentration grid setup
    menu. The grid span may need to be reduced to
    zoom in on the area of interest.
  • Click on the initial map domain image with the
    right mouse button to display the concentrations
    (right). In this case the full 30 x 30 degree
    concentration grid defined previously covers an
    area much larger than the plume.

28
Converting Concentration Data to Text Files
  • The concentration output file is in a binary
    format, however there are several options
    available through the Concentration / Utility
    Programs menu that can be used to convert the
    concentration data to other formats.
  • First, prepare a multi-time period output file by
    setting up a simulation as in the previous
    example, but with the following changes
  • Top-hat-horizontal particle-vertical,
  • No particle dump interval (0),
  • 12 hour simulation,
  • 12 hour continuous release,
  • 500 particles, and
  • 1 hour average concentrations.
  • Check the Fix-Exp box in the Display menu to keep
    the contours constant and you may need to change
    the name of the output file from partplot to
    concplot.
  • After displaying the Postscript output, create an
    animated gif image by using the Concentration /
    Utility Programs / Convert Postscript menu by
    checking the animate box in the Postscript
    Conversion menu.
  • The continuous emission plume moves southwest and
    then more to the south near the end of the
    simulation.

29
Converting Concentration Data to Text Files
  • Time Series Data Extraction
  • Next, select the Concentration / Utility Programs
    / Grid to Station menu (right).
  • Select a point downwind in the plume (27.7N,
    81.0W),
  • Give it a unique Integer ID (2781),
  • Set the Concentration Multiplier to 1.0,
  • and choose a Log Ordinate scale.
  • Click Extract Data and an ASCII con2stn.txt file
    will be created with the concentration values
    interpolated to that location.  (An input file
    with the station locations must be created for
    multiple locations).
  • Selecting the Display Time Series Yes button
    results in the creation of a time series plot
    (right). In this case the peak concentration
    occurred at 1600 UTC on 19 December 2005.

30
Converting Concentration Data to Text Files
  • The Concentration / Utility Programs / Convert to
    ASCII menu will convert every non-zero grid point
    value to its ASCII equivalent, writing the output
    to one file per time period unless you specify
    Single File.
  • Files are labeled according to the name of the
    binary file, Julian day, and hour of the sampling
    period.
  • See the contents of this file for the output from
    the first time period.
  • This file can useful when importing the data into
    other mapping applications.

31
Example Local Scale Dispersion Calculation
  • HYSPLIT can be configured for applications such
    as emergency response, when the scale of the
    simulation is on the order of 10-30 km.
  • For this example, set up the run as shown below
    for Washington, D.C.
  • 38.880N 77.027W _at_10m and 100m,
  • 1200 UTC 19 December 2005,
  • NAM 12 km forecast data,
  • 1-hr emission and simulation,
  • 1-hr average concentration after 1 hr,
  • Lat/lon Grid Resolution of 0.001 degrees, and
  • Grid Span of 1.0 degrees lat/lon.
  • Using the Advanced / Configuration Setup /
    Concentration menu, set
  • 3-D particle horizontal and vertical method,
  • 1000 particles,
  • 10000 maximum number of particles, and
  • Short-range similarity (fluxes) method for the
    turbulence computation.
  • Run Standard Model

32
Example Local Scale Dispersion Calculation
  • After running the model, set the Concentration
    Display menu to the following (right)
  • Output File concplot
  • Number of rings to 4 every 10 km
  • Map background to countymap
  • Zoom to 100
  • Dyn-Exp contours
  • Turn on the contour outlines 
  • Turn on the Google Earth option

33
Example Local Scale Dispersion Calculation
  • The resulting plume (below left) produces a very
    narrow plume moving southeast into Maryland over
    the 1 hour period.
  • As will be discussed later, the Google Earth file
    (HYSPLITconc.kmz) was created and allows the
    emergency manager to overlay the plume with other
    geographic features (below right). This file can
    be provided directly to the emergency manager.

34
Example Local Scale Dispersion Calculation
  • Now assume the release was very small and only
    lasted 15 minutes. Use the Concentration setup /
    Pollutant, Deposition and Grids setup menu
    (right) to define a 15 minute (0.25h) release of
    one unit of mass. Note that since the release
    rate required is per hour, you will need to
    multiply the mass by 4 in this case.
  • Also, change the averaging period to 10 minutes
    over the 1 hour simulation, which can be defined
    in the Concentration Grid Setup menu.
  • Run the model and create an animated GIF (right).
    To keep the contours from changing as the
    concentrations decrease, you may want to fix the
    contours by checking Fix-Exp box in the
    Concentration Display menu.
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