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Heat Transfer across Boundary

The surface of a structural member exposed to a fire is subject to heat transfer by convection and radiation. Generally, the radiation is more dominant than the convection after the very early stages of the fire. The thermal actions can be represented by the net heat flux to the surface of the member.

On the fire exposed surfaces, the net heat flux [W/m2] considering heat transfer by convection and radiation can be determined by:

(1)
where
is the net convective heat flux component as given in Eq.(2) ;
is the net radiative heat flux component as given in Eq.(3) .

For non-fire exposed (unexposed) surfaces of members subjected to partial heating conditions, such as the unexposed side of walls and slabs, heat will transfer from the member to the boundary as the member will have a higher temperature. The heat transfer analysis according to Eq.(1) can be applied, considering different boundary conditions. The following modifications in the heat transfer can be considered (Purkiss 1996):

  • For a surface exposed to ambient conditions, the gas temperature is taken to be equal to ambient temperature with both radiation and convection heat transfer considered.
  • Alternatively, for a surface exposed to ambient conditions, a fixed temperature equal to ambient temperature can be imposed on the boundary nodes of the surface.
  • For a surface with insulation, the boundary can be treated as a no heat-flow condition.

It is worth noting that the heat transfer to the boundary has an important effect on the thermal response of the region within the members close to the unexposed surface. The effect is smaller in the region close to the fire exposed surface.

Convection

The net heat flux [W/m2] due to convection is given by:

(2)
where
αc is the coefficient of heat transfer by convection as given in Table 1 [W/m2K];
Θg is the gas temperature in the vicinity of the fire exposed member [°C];
Θm is the surface temperature of the member [°C].

Table 1 Convection coefficients αc according to EN1991-1-2 (2002)
Fire model or exposed condition αc[W/m2K]
Standard fires
25
External fires
25
Hydrocarbon fires
50
Parametric fires
35
Unexposed side of separating members
-withough radiation
4
-with radiation
25

Radiation

The exact formula for the heat flux due to radiation is complicated, in which the parameters involved depend on the type of surface, the type of flame and the temperature. For simplicity, EN1991-1-2 (2002) provides an approximation of the net heat flux [W/m2] due to radiation as follows:

(3)
where
εf is the emissivity of the fire (=1.0);
εm is the surface emissivity of the member (see Table 2);
Φ is the configuration factor (≤ 1.0);
Θr is the effective radiation temperature of the fire environment [°C];
σ is the Stephan Boltzmann constant (=5.67 × 10-8 W/m2K4).

Table 2 Emissivity of materials according to Eurocodes
Material Emissivity εm Reference
Carbon steel
0.7
prEN1993-1-2
stainless steel
0.4
prEN1993-1-2
Concrete
0.7
EN1992-1-2
Others
0.8
EN1991-1-2

The configuration factor Φ takes into account of varying radiative heat flux levels on the fire exposed surface of the members depending on the position and shallow effects. Annex G (informative) of EN1991-1-2 gives the method for calculating the value of Φ, which will be discussed in the next section. Conservatively, Φ can be taken as 1.0.

Configuration Factor

Annex G (informative) of EN1991-1-2 (2002) provides the simple method for calculating the configuration factor Φ for the determination of the thermal actions for external members.

The configuration factor Φ measures the fraction of the total radiative heat leaving a radiating surface that arrives at a receiving surface, depending on the size of the radiating surface and the distance and the orientation between the two surfaces (see Figure 1).

Basically, the value Φ of for a member surface exposed to a fire depends on two effects:

  • Position effect – the position and the size of the fire
  • Shadow effect – the radiation from other parts of the member

The radiative heat transfer to a convex member surface is determined by the position effect, whereas the transfer to a concave surface is determined by both the position and shadow effects.

The assumptions made in the calculation of Φ for an external member include:

  • All radiating surfaces are taken as rectangles in shape, including windows and other openings in fire compartment walls and the equivalent rectangular surfaces of flames.
  • The value of Φ is determined for the mid-point P of each face of a rectangular envelope drawn around the cross-section of the member receiving the radiative heat transfer, as shown in Figure 2. This accounts for the shadow effect in an approximate way.

The calculation procedure Φ of is explained in the following steps:

  1. Choose a point P on the member.
  2. Locate the point X on the radiating surface by drawing a horizontal line perpendicular to the receiving surface from P to the plane containing the radiating surface. The distance s from P to X is the shortest distance from P to the receiving surface.
  3. Divide the receiving surface into different zones by drawing a horizontal and a vertical line through X. Normally, it contains four zones if the whole radiating surface is visible from P as shown in Figure 3(a). It will only contain two zones if the radiating surface is only partially visible as shown in Figure 3(b).
  4. The Φ of the receiving surface is the sum of the contributions from each visible zone on the radiating surface.
  5. If X lies outside the radiating surface, the effective Φ is determined by adding the contributions of the two extending rectangular zones from X to the farther side of the radiating surface, then subtracting the contributions of the two rectangular zones extending from X to the nearer side of the radiating surface.
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