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What Is a Numerical Weather Prediction Model?

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The precipitation rate P=PL PC is known once HL and HC are known. ... become aware of these limitations in order to make 'Intelligent Use of Model Guidance' ... – PowerPoint PPT presentation

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Title: What Is a Numerical Weather Prediction Model?


1
What Is a Numerical Weather Prediction Model?
  • Seek relationships (equations) between variables
    you want to know (e.g. - v, T, p, z, q) and the
    forcing mechanisms that cause changes in these
    variables.
  • Example

Presented by Fred Carr COMAP Symposium 00-2
2
  • In meteorology, we solve for Du/Dt
  • (1)

3
  • Or
  • or
  • Example of a prognostic equation

4
  • Example of a diagnostic equation
  • Just consider vertical component of (1)
  • rhs balances perfectly for large-scale flow
  • Hydrostatic eq. - used to deduce Z from T

5
  • Thus, the essential components of an NWP model
    are
  • 1. Physical Processes - RHS of equations (e.g.,
    PGF, friction, adiabatic diabatic heating
    (advection terms are also on rhs unless have
    Lagrangian model)

6
  • 2. Numerical Procedures
  • approximations used to estimate each RHS term
    (especially imp. for advection terms)
  • approximations used to integrate model forward
    in time
  • grid used over model domain (resolution)
  • boundary conditions
  • Note Quality and quantity of observations
    (initial conditions) equally vital to NWP system
  • Need to observe prognostic variables

7
Primitive Equation Models
  • A. Primitive Equations
  • It was recognized early in the history of NWP
    (Charney, 1955) that the primitive equations of
    motion would be best suited for development of
    comprehensive dynamical-physical models of the
    atmosphere. Although the problems of
    initialization and numerical integration of the
    primitive equations are still areas of research,
    stable forecasts from these equations have been
    produced for over 35 years.

8
  • We will present the primitive equations in x-y-p
    coordinates and discuss some general properties
    of this system. These equations are equally
    appropriate for global as well as limited-area
    models.
  • A set of governing equations that describe
    large-scale atmospheric motions can be derived
    from conservation laws governing momentum, mass,
    energy, and moisture (see Holton, 1979 - Chap.
    2). These are called the primitive

9
  • equations, not because they are crude or
    simplistic but because they are fundamental or
    basic. Using the Eulerian framework in x-y-p
    coordinates, they can be written as follows
  • (1)
  • (2)
  • (3)
  • (4)
  • (5)
  • (6)

10
  • Eqs. (1) and (2) are the horizontal momentum
    equations for the u- and v- components of the
    wind, respectively. Note that (via scale
    analysis), the curvature terms and the 2??cos?
    Coriolis term have been neglected. Eq. (3) is
    the vertical momentum equation under the
    assumption of hydrostatic balance (diagnoses z).
    The continuity equation (4) expresses the
    conservation of mass (diagnoses w). The First
    Law of Thermodynamics yields an energy equation
    for temperature (5). Eq. (6) is the conservation
    of moisture equation where q is specific
    humidity.

11
  • The dependent variables in this set of equations
    are u, v, ?, ?, T, and q which are assumed to be
    continuous functions of the independent variables
    x, y, p, and t. Eqs. (1), (2), (5), and (6) are
    prognostic equations (involve a time derivative)
    and thus require initial conditions. Initial
    conditions are derived from observations or the
    use of some balance relationship (e.g. -
    obtaining u and v from ? by assuming geostrophic
    balance). Eqs. (3) and (4) are diagnostic
    equations and can be computed once the initial
    conditions are provided. Thus, (1) to (6)
    constitute a set of 6 equations in 6 unknowns

12
  • and we can say we have a closed system if
  • i) we can find expressions for Fx, Fy, H, E,
    and P in terms of the known dependent
    variables
  • ii) we have suitable initial conditions over
    the domain
  • iii) suitable lateral boundary conditions for
    the dependent variables are formulated (for
    regional models) all models need boundary
    conditions at the top and bottom levels

13
  • The first category above encompasses the whole
    subject of adding physics to the primitive
    equations. Fx and Fy are friction terms which
    modify the momentum equations via surface drag
    (skin friction) and horizontal and vertical
    transport of momentum by turbulent eddies of
    various sizes (generally called diffusion in
    large-scale models). The diabatic heating term H
    also consists of several effects which can be
    written
  • H HL HC HR HS (7)

14
  • where HL is due to latent heat of condensation
    caused by the large-scale dynamic ascent of
    stably-stratified, saturated air (grid-scale
    precipitation), HC is the latent heat rate due to
    convection (cumulus parameterization), HR is the
    radiative heating rate and HS represents sensible
    heat flux from the surface of the earth. One
    of the most difficult problems in NWP is how to
    formulate proper expressions for the net effects
    of HC, HR, and HS (which are generally
    subgrid-scale processes) in terms of the
    large-scale dependent variables (the
    parameterization problem). The precipitation
    rate PPLPC is known once HL and HC are known.

15
  • Evaporation E can be due to moisture flux from
    the surface and evaporation of precipitation.
    The effect of mountains also has to be included
    in the model via the lower boundary condition and
    choice of vertical coordinate .
  • Once conditions (i) to (iii) are suitably met
    (the fact that they are never perfectly met
    accounts for a large part of the total forecast
    error), the equations (1) to (6) can, in
    principle, be solved in the following
    straightforward manner

16
  • 1. Obtain observations of the prognostic
    variables u, v, T, and q over the domain
  • 2. Compute ? from (3) and ? from (4)
  • 3. Compute Fx, Fy, H, E, P and the other
    terms on the right-hand sides of (1), (2), (5),
    and (6)
  • 4. Integrate the four prognostic equations
    forward in time to obtain new values of u, v,
    T, and q
  • 5. Repeat steps 2 to 4 until complete the
    forecast

17
  • Since there are nearly an infinite number of ways
    to formulate the physics and many numerical
    procedures are available for the solution of the
    equations, no two numerical models are alike.
    Thus each model may have systematic errors or
    biases peculiar to itself. However, some errors,
    such as those arising from insufficient
    resolution, are common to all models. It is
    important for forecasters to become aware of
    these limitations in order to make Intelligent
    Use of Model Guidance.
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