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    International Journal on Architectural Science, Volume 1, Number 2, p.68-79, 2000

    68

    THE CONVECTIVE-DIFFUSION EQUATION AND ITS USE IN BUILDING

    PHYSICS

    Z. SvobodaFaculty of Civil Engineering, Czech Technical University, Thakurova 7, 166 29 Prague 6, Czech Republic

    ABSTRACT

    The convective-diffusion equation is the governing equation of many important transport phenomena in

    building physics. The paper deals in its first part with the general formulation of the convective-diffusion

    equation and with the numerical solution of this equation by means of the finite element method. The second

    part of the paper contains the analysis of one typical combined transport problem the combined heat transfer

    through the building constructions caused by conduction and convection. The finite element solution of this

    problem is presented in the paper together with the numerical stability analysis and one practical example of the

    numerical analysis of a model lightweight building construction. The results of the model analysis demonstrate

    that the lightweight constructions insulated with permeable mineral wool are very sensitive to the convective

    heat transfer.

    1. INTRODUCTION

    Combined transport of a substance through a

    porous medium caused by diffusion and convection

    is a relatively frequent problem in building physics.

    Characteristic examples are the heat transfer

    through a permeable medium, the transport of a

    pollutant through the atmosphere or the transport

    of a fluid through the porous medium.

    The governing equations of such building physics

    problems are generally called the convective-

    diffusion equations. Such equations are the centre

    of many recent investigations [e.g. 1-6] not only

    due to their importance to building physics

    analyses, but also due to some problems with

    numerical stability in their solution.

    2. THE CONVECTIVE - DIFFUSIONEQUATION

    The complex steady-state transport of a substance

    through the porous medium caused by diffusion

    and convection is described by the partial

    differential equation:

    02

    2

    2

    2

    2

    2

    =+

    +

    +

    +

    +

    Q

    z

    Uw

    y

    Uv

    x

    Uu

    z

    U

    y

    U

    x

    U

    (1)

    Boundary conditions for equation (1), which are

    the most useful for building physics problems, are

    usually of Dirichlet type defined as:

    UU = (2)

    or of Newton type defined as:

    ( ) ( )UUUUvn

    Un =+

    (3)

    The Newton type boundary condition (3) is the

    most frequently used boundary condition for

    common problems such as heat transfer. This type

    of condition could also be easily converted within

    the computer programs to Dirichlet type byassigning a large number to the boundary transfer

    coefficient. The Newton type condition will

    therefore be chosen as the basic boundary

    condition in the following derivations.

    In this paper, the following assumptions were taken

    to obtain the numerical solution of equation (1)

    with the boundary condition (3):

    convection of fluid through the porousmedium is caused only by a pressure

    difference

    the moving fluid is incompressible the fluid flow is linear according to Darcys

    Law

    Pk

    v =r

    r

    (4)

    Equation (4) could be used only if the fluid

    flow is laminar. That could be reached

    according to W. Nazaroff [2,3] if the

    Reynolds number defined for fluid flow in

    the porous medium as:

    vdRe = (5)

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    does not exceed the value of 4. This condition

    could be satisfied for most building materials

    with permeability lower than 10-8

    m2

    when

    the operating pressure gradient is not higher

    then 5 Pa [7,8].

    pressure distribution is governed by Laplaceequation:02 = Pk (6)

    the pressure losses of cracks are considered inthe model in a simplified way by means of an

    equivalent permeability of the air in the

    crack, which is defined as:

    3

    2b

    ka = (7)

    Equation (7) was derived from the equality of

    the air flow velocity defined by Darcys Law

    and the mean velocity of the laminar air flow

    in the crack defined as:

    3

    2b

    L

    Pvm

    = (8)

    3. NUMERICAL SOLUTION OF THECONVECTIVE - DIFFUSION

    EQUATION

    The search for the numerical solution of the

    convective-diffusion equation is always more

    complicated than the search for the solution of the

    related diffusion equation. The main cause is the

    convective transport term - second term in equation

    (1) - which can introduce under certain conditions

    instabilities in the numerical solution.

    The finite element method was used in this paper to

    find the solution of equation (1). The general finite

    element formulation was derived by means of the

    Petrov-Galerkin process. As the Petrov-Galerkinprocess is one of the weighted residuals methods,

    the derivation of the finite element formulation

    starts with the following equation:

    02

    2

    2

    2

    2

    2

    =

    +

    +

    +

    +

    +

    dW

    Qz

    Uw

    y

    Uv

    x

    Uu

    z

    U

    y

    U

    x

    U

    )e(

    i

    The Petrov-Galerkin approach, which is also

    known as streamline balancing diffusion orstreamline Petrov-Galerkin process, is based on the

    special selection of the weighting functions

    different from the interpolation functions. The

    identity of the weighting and interpolation

    functions is characteristic for the standard Galerkin

    method which is the most commonly used method

    in the finite element solution of the field problems.

    Unfortunately, this method cannot be applied toequation (1), because it leads to the numerical

    oscillations mentioned above, as was already

    shown by several researchers (Zienkiewicz [9],

    Huebner [1]).

    Equation (9) is a mathematical expression of the

    requirement that the residual of the numerical

    solution of equation (1) must be orthogonal to the

    weighting functions Wi.

    The unknown function Uin equation (9) is taken as

    an approximation:

    iT

    i UNU= (10)

    The interpolation functionsNi are known functions

    closely connected to the type of the chosen finite

    elements.

    The definition of the weighting functions Wi is very

    important in this case. The approach recommended

    by Zienkiewicz [9] takes the weighting functions as:

    u

    z

    N

    wy

    N

    vx

    N

    uhNW

    iii

    ii

    +

    +

    +=2

    (11)

    Now, if the value of is chosen as:

    PePecoth

    1= (12)

    and Peclet numberPe as:

    2

    huPe

    = (13)

    then according to Zienkiewicz [9] numerical

    oscillations will not arise for any possible rate

    between convective and conductive transport.

    The weighting functions defined in equation (11)

    are constructed to be different from zero only in the

    direction of the velocity vector. This fact is the

    reason why the terms streamline Petrov-Galerkin

    process or streamline balancing diffusion are

    used as synonyms for Petrov-Galerkin method.

    Equations (10) and (11) can be substituted intoequation (9). Integration by parts can be then

    applied to the first term in equation (9) and

    (9)

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    subsequently the boundary conditions (3) can be

    introduced into the equation. The general finite

    element formulation which was derived by means

    of this approach can be finally written as:

    ( ) Qiv qqUKKK +=++ (14)

    The conductance matrixK is defined as:

    dz

    N

    z

    W

    y

    N

    y

    W

    x

    N

    x

    WK

    )e(

    Tii

    Tii

    Tii

    +

    +

    =

    (15)

    the convective transport matrixKv as:

    dz

    NwW

    y

    NvW

    x

    NuWK

    )e(

    Ti

    i

    Ti

    i

    Ti

    iv

    +

    +

    =

    (16)

    the boundary conditions matrixKas:

    ( )

    dNWvK)e(

    Tiin = (17)

    the boundary conditions vectorq as:

    ( )

    dUWvq)e(

    in = (18)

    and the substance generation rate vectorqQ as:

    dQWq)e(

    iQ = (19)

    Note that the convective transport matrix Kv is

    asymmetrical, which is caused by the fact that the

    differential operator in equation (1) is not self-

    adjoint. This leads to the asymmetrical matrix of

    the system of linear equations for unknown nodal

    values Ui.

    4. COMBINED HEAT TRANSFERCAUSED BY CONDUCTION AND

    CONVECTION

    Several building physics problems governed by the

    convective-diffusion equation have been

    mentioned already in the introduction of this paper.

    The architects and building engineers usually pay

    the greatest attention to two important combined

    transport phenomena taking place in the building

    constructions, which are the radon transport caused

    by diffusion and convection and the heat transferdue to conduction and convection. The first

    transport problem mentioned has been discussed in

    detail in several papers [10-12]. The second

    problem - the combined heat transfer caused by

    conduction and convection - is currently actively

    discussed in the building physics field [2,4-6,13].

    This type of heat transfer appears in building

    constructions loaded by the temperature and the

    pressure gradient between the interior and theexterior.

    The importance of the convective-conductive heat

    transfer depends mainly on the type of the

    construction and on its tightness against the air

    flow. Typical construction for which the

    convective part of the heat transfer is of high

    importance is a modern lightweight construction

    with permeable thermal insulation, such as mineral

    wool, covered by thin layers of plasterboards.

    Traditional constructions, such as brick walls, are

    not so sensitive to the convective heat transfer and

    the convective component of the total heat loss isusually negligible in comparison with the

    conductive component.

    5. GOVERNING EQUATION OF THECONVECTIVE - CONDUCTIVE

    HEAT TRANSFER AND ITS

    NUMERICAL SOLUTION

    The analysis of many combined convective-

    conductive heat transfer problems could be based

    on the partial differential equation for the two-dimensional steady-state heat transport in a porous

    medium, which is a member of convective-

    diffusion equations family. This equation could be

    expressed as:

    02

    2

    2

    2

    =

    +

    +

    y

    Tv

    x

    Tuc

    y

    T

    x

    Taa (20)

    The Newton type boundary condition connected to

    equation (20) is defined as:

    ( ) ( )TThTTcvnT aan =+

    (21)

    Note that equation (20) is a subtype of the general

    convective-diffusion equation (1) and the boundary

    condition (21) is of the same type as condition (3).

    The numerical solution of equation (20) could be

    derived using the same assumptions and the same

    method as was already shown for the general

    convective-diffusion equation. The finite element

    solution of equation (20) could be reached by

    means of Petrov-Galerkin process with weighting

    functions Widefined for this two dimensional caseas:

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    u

    y

    Nv

    x

    Nu

    hNW

    ii

    ii

    +

    +=2

    (22)

    and the Peclet number defined as:

    2

    hucPe

    aa = (23)

    The derived general finite element solution of the

    equation (20) could be finally written as:

    ( ) qTKKK iv =++ (24)

    The conductance matrixK is defined as:

    dy

    N

    y

    W

    x

    N

    x

    WK

    )e(

    T

    ii

    T

    ii

    +

    = (25)

    the convective transport matrixKv as:

    dy

    NvW

    x

    NuWcK

    )e(

    Ti

    i

    Ti

    iaav

    +

    = (26)

    the boundary conditions matrixKas:

    ( )

    dNWcvhK

    )e(

    Tiiaan = (27)

    and the boundary conditions vectorq as:

    ( )

    dTWcvhq)e(

    iaan = (28)

    Equation (24) is the basis for the computer

    program called WIND developed by Z. Svoboda.

    This program calculates the pressure field within

    the porous building construction, the air flow

    velocity field, the temperature field and the heat

    flow rate due to conduction and due to convection.This calculation tool uses the simple triangular

    finite elements with three nodes (Fig. 1) and with

    the linear interpolation functions defined as:

    ( )ycxbaA

    N iiii ++=2

    1i = 1, 2, 3 (29)

    where the values a, b and c are expressed as:

    jkkji yxyxa =

    kji yyb =

    jki xxc =

    with the indices i,j, ktaken as 1, 2, 3 in a cycle.

    The weighting functions derived from equation (22)

    could be written for this simple finite element with

    the linear interpolation as:

    ( )

    +

    +++= iiiiii vcub

    u

    hycxba

    AW

    22

    1

    i = 1, 2, 3 (30)

    1

    2

    3

    L3

    L1

    L2

    Fig. 1: Triangular finite element with 3 nodes

    and linear interpolation

    Now, if the interpolation and weighting functions

    are defined in the way as shown in equations (29)

    and (30), it is possible to derive analytical

    expressions for all matrixes and vectors in the

    finite element formulation (24).

    The analytical expression for the conductance

    matrixKis:

    +

    ++

    +++

    =2

    32

    3

    32322

    22

    2

    313121212

    12

    1

    4cbsymm.

    ccbbcb

    ccbbccbbcb

    AK

    (31)

    For the convective transport matrixKvis:

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    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +

    +++

    +++

    +++

    =

    23

    2

    33

    2

    3

    232

    2

    32

    32

    322

    22

    2

    22

    22

    2

    312

    31

    31

    312

    212

    21

    21

    212

    21

    2

    11

    21

    2

    3

    3

    2

    2

    1

    1

    3

    3

    2

    2

    1

    1

    3

    3

    2

    2

    1

    1

    2

    2

    2

    8

    6

    cv

    cuvbbu

    symm.

    ccv

    cuvb

    buvc

    bbu

    cv

    cuvb

    bu

    ccv

    cuvb

    buvc

    bbu

    ccv

    cuvb

    buvc

    bbu

    cv

    cuvb

    bu

    uA

    ch

    vc

    ub

    vc

    ub

    vc

    ub

    vc

    ub

    vc

    ub

    vc

    ub

    vc

    ub

    vc

    ub

    vc

    ub

    cK

    aa

    aav

    (32)

    and for the boundary conditions matrixK is:

    +

    +

    +

    +

    +

    +

    +

    =

    4

    44

    444

    3

    63

    663

    21

    131

    2332

    21

    131

    2332

    BBsymm.

    BBB

    BBBB

    BBsymm.

    BBB

    BBBB

    K

    (33)

    with Bi defined as ( iaai,nii LcvhB = and i=1,2, 3, where i is the number of the triangular finite

    element boundary (side of the triangle). The

    definition of the sides of the triangular finite

    element is shown in Fig. 1. If no boundary

    condition is defined at the finite element boundary,

    all terms corresponding to that boundary in

    equation (33) are taken as 0.

    The boundary conditions matrix K could also be

    defined in a way different from equation (33). If

    the interpolation functions on the finite element

    boundaryLi are taken as partly continuous (Fig. 2),

    which is acceptable according to Zienkiewicz [9]

    as far as there are no derivatives of interpolation

    functions Ni in equation (27), the resulting

    boundary conditions matrixKcan be defined as:

    +

    +

    +

    +

    +

    +

    +

    =

    2

    02

    002

    2

    02

    002

    21

    31

    32

    21

    31

    32

    BBsymm.

    BB

    BB

    BBsymm.

    BB

    BB

    K

    (34)

    with ( iaai,nii LcvhB = and index i rangingfrom 1 to 3.

    1

    23

    LL

    L1

    3

    2

    N N23

    x

    1

    1

    23

    LL

    L1

    3

    2

    N N23

    x

    a) b)

    The use of the boundary conditions matrix defined

    in equation (34) leads to higher numerical stability

    of the calculation results, especially in the parts of

    the construction where two boundary conditions

    are in connection (e.g. at the external surface of the

    wallecorners .

    (a) (b)

    Fig. 2: (a) Linear and (b) partly continuous interpolation functions on the element boundary L 1

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    The last term in equation (24) is the boundary

    conditions vector q which could be analytically

    expressed as:

    +

    +

    +

    +

    +

    +

    +

    =

    2

    2

    2

    2

    2

    2

    2211

    3311

    3322

    2211

    3311

    3322

    TBTB

    TBTB

    TBTB

    TBTB

    TBTB

    TBTB

    q (35)

    with ( iaai,nii LcvhB = and index i rangingfrom 1 to 3.

    6. NUMERICAL STABILITYANALYSIS

    The analysis of the numerical stability of the

    solution obtained by the computer program

    WIND could be realised in two ways. The first

    method is to calculate the exact analytical solution

    of a simple one dimensional problem and to

    compare it with the numerical solution obtained by

    the program. The second method of the numerical

    stability analysis could be based on the evaluation

    of the functional corresponding to the governing

    equation (20).

    The first method of the numerical stability analysis

    was studied based on a simple one dimensionalproblem:

    02

    2

    =dx

    dTuc

    dx

    Tdaa (36)

    with boundary conditions:

    10 =)(T , 01 =)(T (37)

    The analytical solution of the equation (36) is:

    B

    BBx

    e

    ee)x(T

    =

    1(38)

    with the value ofB defined as:

    ucB aa= (39)

    The numerical solution of equation (36) forB = 4

    and for various number of the finite elements in

    comparison with the exact solution could be seen

    in Table 1. The analysis shows clearly that the

    results of the numerical solution converge to theexact solution with increasing number of the finite

    elements covering the solved area.

    Table 1: Results of the exact and the numerical

    solution

    Distance Temperature

    exact

    solution

    numerical

    solution

    x (m) T (K) T1 (K) T2 (K) T3 (K)0,0 1,000 1,000 1,000 1,000

    0,2 0,977 0,978 0,977 0,977

    0,4 0,926 0,928 0,927 0,926

    0,6 0,813 0,815 0,814 0,813

    0,8 0,561 0,564 0,562 0,561

    1,0 0,000 0,000 0,000 0,000

    No. of

    elements

    --- 20 40 80

    The second method of the numerical stability

    analysis - the evaluation of the functional

    corresponding to equation (20) - is more

    complicated but it is more appropriate for theanalysis of the two or three dimensional problems.

    The basic idea of this approach is based on the fact

    that the finite element method is one of the

    variation methods which means that the exact

    solution of the equation (20) obtained by the finite

    element method must minimise the functional

    corresponding to the equation (20). The functional

    connected with the equation (20) could be derived

    by means of the Guymon process cited by

    Zienkiewicz [9]. The first step in this process is to

    adjust the linear differential operatorA in equation

    (20):

    yvc

    xuc

    yxA aaaa

    +

    =

    2

    2

    2

    2

    (40)

    which is not self-adjoint, in a special way so that

    the self-adjointness is achieved without altering the

    equation (20). Let us expect that q(x,y) is a general

    function and let us multiply both sides of equation

    (20) with this function. Equation (20) could be

    rewritten after this operation as:

    0=TqA (41)

    The test for symmetry of the operatorqA could be

    expressed for any two functions and as:

    ( ) ( )

    dqAdqA = (42)

    Now, if we take the operatorqA from equation (41),

    substitute it into equation (42) and integrate the

    result by parts, we could obtain following equation

    (b.t. denoting boundary terms):

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    b.t.d

    y

    qvqc

    y

    xquqc

    xyq

    yxq

    x

    b.t.d

    y

    qvqc

    y

    x

    quqc

    xyq

    yxq

    x

    aa

    aa

    aa

    aa

    +

    +

    +

    =+

    +

    +

    The operator qA will be symmetric and therefore

    self-adjoint if the equations:

    0

    0

    =

    +

    =

    +

    y

    qvqc

    ,x

    quqc

    aa

    aa

    (43)

    are fulfilled. The solution of equations (43), which

    is the function q we search for, could be found as:

    ( )vyuxcaa

    eq+

    =

    (44)

    If we take the function q defined according to

    equation (44) and multiply equation (20) with it,

    we finally obtain the symmetric operator qA.

    Subsequently, we could use a well-known

    expression:

    ( )

    dTqATF21 = (45)

    for the derivation of the functionalFcorresponding

    to equation (20). The resulting functional

    connected to equation (20) could be obtained after

    some derivations in the following form:

    ( )( )

    dTTTcvhq

    dy

    Tq

    x

    TqF

    aan

    +

    =

    2

    21

    22

    21

    (46)

    where the function q is defined in equation (44).

    The building construction shown in Fig. 3 was

    analysed from the point of view of the numerical

    stability using the functional evaluation. The

    characteristics of the materials involved are shown

    in Table 2. The boundary conditions were taken as

    follows:

    interior: temperature 20 C, pressure 0 Pa exterior: temperature -15 C, pressure 10 Pa

    The initial mesh system with 580 finite elements is

    shown in Fig. 4. The mesh system was refined

    twice and each time the functional (46) was

    calculated by means of the Gauss numerical

    integration. The results of the analysis are

    presented in Fig. 5. It could be clearly seen that the

    values of the functional decrease with theincreasing number of finite elements. This shows

    that the calculated results of equation (20)

    converge to the exact solution and the numerical

    stability is reached.

    plasterboard 13 mm

    mineral wool 120 mm

    plasterboard 13 mm 1 mm wide crack

    1 m

    Fig. 3: The model building construction for

    the functional analysis

    Table 2: Used material characteristics

    Material Permeability(m

    2)

    Thermalconductivity

    (Wm-1

    K-1

    )

    Plasterboard 1.10-12 0.220

    Mineral wool 1.10-9

    0.040

    7. ANALYSIS OF A MODEL

    CONSTRUCTION

    The use of the program WIND for the purposes

    of the heat transfer calculations could be

    demonstrated on the analysis of a typical building

    slope roof construction. A cross-sectional view of

    the analysed construction and the boundary

    conditions are shown in Fig. 6. The material

    characteristics are recapitulated in Table 2.

    The calculation has been performed several times

    for various widths of the crack in the internal

    plasterboard cladding, including perfectly tight

    construction with no cracks. For each width of the

    crack and for each loading pressure gradient, the

    air pressure field, the air flow velocity field and the

    temperature field have been calculated.

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    Fig. 4: The initial mesh system with 580 elements

    0,00040

    0,00045

    0,00050

    0,00055

    0,00060

    0,00065

    580 1160 2320

    Number of elements

    Functionalvalues

    Fig. 5: The calculated functional values

    1000 mm

    mineral wool 160 mm

    closed air layer 40 mm

    plasterboard 12 mm

    exterior side:

    temperature -15 C air pressure from 0 to 10 Pa

    interior side:

    temperature 20 C air pressure 0 Pa

    crack of

    various

    width

    roof tiles

    ventilated air layer

    (300 mm to 800 mm)

    inlet

    outlet

    Fig. 6: Cross-section of the analysed construction

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    The influence of the convective heat transport

    through the crack has been expressed for each

    analysed case by means of the convective linear

    thermal transmittance according to the following

    equation:

    ccei

    p,v lUtt

    = (47)

    The linear thermal transmittance is used in ISO and

    European standards as a value showing the

    influence of a thermal bridge on the heat loss. In

    this paper, the crack is taken as a convective

    bridge and the convective linear thermal

    transmittance is used to show the influence of the

    air flow through the convective bridge on the

    heat loss, which can be finally expressed as:

    += tltUAQ p,vvT (48)

    The convective linear thermal transmittance is

    always related to the length of the crack and to the

    operating pressure difference.

    The results of the convective linear thermal

    transmittance calculation for various pressure

    differences and various widths of the crack in theplasterboard are shown in Table 3 and Fig. 7.

    Another interesting calculation result is the

    temperature distribution in the analysed

    construction. Fig. 8 shows the temperature fields in

    the construction with 1 mm wide crack in the

    plasterboard for pressure differences 0 and 10 Pa.

    Note the deformation of the temperature field

    caused by the air flow through the permeable

    thermal insulation not covered by any air-tight

    layer and through the crack in the plasterboard in

    the case of pressure gradient of 10 Pa.

    Table 3: The results of the convective linear thermal transmittance analysis

    Operating Width of the crack

    pressure difference no crack 1 mm 2 mm 3 mm

    0 Pa 0.000 Wm-1

    K-1

    0.000 Wm-1

    K-1

    0.000 Wm-1

    K-1

    0.000 Wm-1

    K-1

    1 Pa 0.003 Wm-1K-1 0.188 Wm-1K-1 0.231 Wm-1K-1 0.247 Wm-1K-1

    5 Pa 0.015 Wm-1

    K-1

    1.296 Wm-1

    K-1

    1.565 Wm-1

    K-1

    1.628 Wm-1

    K-1

    10 Pa 0.031 Wm-1

    K-1

    2.748 Wm-1

    K-1

    3.203 Wm-1

    K-1

    3.385 Wm-1

    K-1

    0,00

    0,50

    1,00

    1,50

    2,00

    2,50

    3,00

    3,50

    0 2 4 6 8 10

    The operating pressure difference [Pa]

    Theconvectivelinearthermaltransmittance[W/mK]

    no crack

    1 mm wide crack

    2 mm wide crack

    3 mm wide crack

    Fig. 7: The convective linear thermal transmittance for various widths of the crack

    Convectivelinear

    thermaltransmittance(Wm-1K-1)

    Operating pressure difference (Pa)

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    Fig. 9 demonstrates three temperature distributions

    in the cross-section of the construction. The first

    distribution, which was calculated for no operating

    pressure difference, is a typical temperature profile

    in the construction exposed to the heat transfer

    caused exclusively by conduction. The second

    distribution calculated for the pressure differenceof 10 Pa shows clearly how the air flow from the

    exterior side changes the temperature profile in the

    construction, even if the analysed construction has

    no crack in the plasterboard covering. The last

    temperature distribution shows the extraordinary

    influence of the crack in the plasterboard. This

    temperature profile is calculated for the pressure

    gradient of 5 Pa and is taken from the cross-sectionleading through the centre of the 1 mm wide crack.

    exterior side:

    temperature -15 C air pressure 0 Pa

    interior side:

    temperature 20 C air pressure 0 Pa

    exterior side:

    temperature -15 C air pressure 10 Pa

    interior side:

    temperature 20 C air pressure 0 Pa

    Fig. 8: The temperature distribution in the construction with 1 mm wide crack in the plasterboard

    -15

    -10

    -5

    0

    5

    10

    15

    20

    0 53 106 159 212

    Cross-section of the construction [mm]

    Tem

    perature[C]

    no crack, 0 Pa

    no crack, 10 Pa

    1 mm wide crack, 5 Pa

    mineral woolair layerplasterboard

    Fig. 9: The temperature distribution in the cross-section of the analysed construction

    Cross-section of the construction (mm)

    Temperature(oC)

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    The results of the model analysis show these major

    conclusions:

    The modern constructions containing permeable

    thermal insulation, such as mineral wool, are very

    sensitive to the convective component of the heat

    transfer. Any crack in the covering of a lightweightconstruction filled with permeable thermal

    insulation could cause air flow into the thermal

    insulation and consequently modifications to the

    temperature distribution. The result of such

    temperature field deformation is a considerable

    increase in the heat loss through the construction.

    ACKNOWLEDGEMENT

    This paper was supported by the research program

    VZ CEZ J04/98:210000001.

    NOMENCLATURE

    A area of a triangular finite element, m2

    b one half of the width of the crack, m

    ca thermal capacity of the air, 1010 Jkg-1

    K-1

    d characteristic diameter of the pore in the

    porous medium, m

    h size of a finite element in the velocity

    direction, m

    h heat transfer coefficient, Wm-2K-1

    k permeability of the porous medium, m2K conductance matrix

    Kv convective transport matrix

    K boundary conditions matrix

    lc width associated with the U value, m

    lv length of the crack associated with the

    convective linear thermal transmittance, m

    L length of the crack in the direction of the air

    flow, m

    Li length of a triangular finite element side, m

    Ni vector of the interpolation functions

    P pressure of the fluid in the porous medium,

    Pa

    P pressure difference between the inlet and the

    outlet of the crack, Pa

    q boundary conditions vector

    T unknown temperature, K

    Ti vector of unknown nodal temperature values,

    K

    T known temperature in the environment in the

    connection with the element boundary, K

    ti interior temperature, K

    te exterior temperature, K

    t temperature difference, K

    u, v, w velocity vector components in the x-axis,

    y-axis and z-axis direction respectively, ms-1u velocity vector magnitude, ms-1

    U unknown concentration of a substance in the

    medium

    Ui vector of unknown nodal concentrations of

    the substance

    Uc U value, thermal transmittance coefficient,

    Wm-2

    K-1

    U known concentration of the substance at partof the boundary

    U known concentration of the substance in theenvironment neighbouring with the boundary

    vn velocity component normal to the boundary,

    ms-1

    v fluid flow velocity in the porous medium,ms-1Q amount of the internal source of the substance

    QT transmission heat loss, W

    Wi vector of the weighting functions

    x, y co-ordinates of the mesh node

    boundary transfer coefficient of the substanceat the discussed boundary

    heat flow rate, Wm-1

    parameter describing the convective

    properties of the medium

    e boundary of a finite element

    parameter describing the diffusive properties

    of the medium

    thermal conductivity, Wm-1K-1

    viscosity of the fluid (for air = 1.7 x 10-5Pas),

    kinematic viscosity of the fluid (for air =

    1.4 x 10-5

    m2s

    -1),

    e area of a finite element, m2

    a density of the air, 1.2 kgm

    -3

    v,p convective linear thermal transmittance at a

    given pressure difference, Wm-1

    K-1

    n derivative in the direction of the external

    normal to the boundary

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