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Ignition
Ignition is defined as:
"The process by which a rapid, exothermic reaction is initiated,
which then propagates and causes the material involved to undergo
change, producing temperatures greatly in excess of ambient"
- Drysdale, D. An Introduction to Fire Dynamics, Wiley, 1999
pg193.
There are two types of ignition.
Piloted Ignition (insert a picture of a spark plug sparking
or a small flame) This particular kind of ignition consists of a
spark or a small flame providing the initial energy for a fire to
ignite
Spontaneous Ignition (insert a picture that looks like an
explosion???) This kind of ignition is the result of a flame developing
spontaneously in a flammable mixture of gases.
As you have seen in the Science section,
a flame can release a tremendous amount of energy into the ambient
environment. The key to sustaining and propagating a flame after
ignition is the rate of energy release. If the rate of energy release
is less than or equal to the rate of heat loss by the flammable
mixture to the environment, then the flame will not propagate. If
the rate of heat release is greater than the rate of heat loss,
then the reaction will become unstable and proceed to a higher temperature.
The figure below can be used to qualitatively understand this idea.
When the temperature of the mixture is greater than T2, the heat
release rate is greater than the heat loss. The mixture becomes
unstable and begins to heat up, until the temperature T3 is reached.
T3 is the higher temperature normally associated with combustion.
While this concept is not rigorously valid for spark piloted ignition,
it does provide a useful schematic for thinking about how ignition
is achieved and a flame propagated.
There are two models for finding the critical ignition temperature.
The first was proposed by Semenov. He assumed a uniform temperature
in the reacting mixture and that the heat losses could be described
by the product of a overall heat transfer coefficient and the difference
in temperature between the walls of the reacting vessel and the
mixture. Because this method assumes a lumped model for the reacting
mixture, it is called the “low Biot number model”. To see the equations
for this model, follow this link. (link to equations)
The second model was developed by Frank Kamenetskii
and takes into account the temperature variations across the mixture.
This is known as the “high Biot number” model. To see the equations
for this model, follow this link (link to equations)
The values for the auto-ignition temperatures for several fuels
have been tabulated and some common fuels are shown on a table from
the 1997 NFPA Handbook (link to table 1)
These values for auto-ignition temperature are relevant in that
they represent the temperature that must be achieved in a flammable
mixture at a distance greater than the quench distance above a surface,
whether it be a solid or liquid, for spontaneous ignition to occur.
The flammability of a liquid is related to this through
the flashpoint. The flashpoint of a liquid fuel is the minimum
temperature that is needed to insure a flammable mixture above the
liquid surface. This is found using our knowledge of the lower
flammability limit of the fuel (link to science) and the Clausius-Calpyron
equation to find the partial pressure of the liquid (link to science).
Flashpoints of certain fluids are listed in Table 2 (link).
This idea of a flashpoint is also valid in a solid,
but in this case it refers to the minimum temperature that will
cause the solid to undergo pyrolysis. Unlike the liquids, this involves
a chemical change in the substance of the solid, and so is a destructive
reaction. Part of the solid is decomposed and flammable vapors are
released. In this case, the establishment of a flame is not necessarily
more “difficult” but does require more conditions to be met. First,
a sufficient heat flux is necessary to pyrolize the solid at a high
enough rate to provide a flammable mixture to the atmosphere above
the solid. Second, a pilot ignition source must be near and, third,
the conditions must be suitable for flame propagation. There are
two possibilities for a piloted ignition of a solid, a continuous
heat flux and a discountinous heat flux.
A continuous heat flux is defined as being separate
from the ignition source and of a necessary level that the temperature
of the solid surface is high enough to cause a flow a pyrolized
material to sustain a flame. In this case, the flashpoint temperature
is the temperature that will cause the flow of volatiles in sufficient
amount to sustain a flame. To see the equations for this condition,
click hear.(link)
A discontinuous heat flux is one that is applied and
then removed after the flame becomes self-supporting. In this case,
a flux is applied to a solid until the flow of volatiles is high
enough that the heat release from the flame is sufficient to keep
the pyrolysis going and sustain the flame. To see the equations
for this condition, click here (link).
Spark-piloted ignition: The phenomenon of spark piloted
ignition does not rely on a heat flux from a flame to produce the
heat flux necessary to ignite a flammable mixture of gasses. Instead,
a high energy spark ionizes the materials in the gap the spark jumps
over. This ionization results in the formation of highly reactive
chemical species, or ‘radicals.’ These radicals the attack the fuel
and start the chemical reactions that lead to a flame and flame
propagation.
Semenov Model
Semenov assumes that the gas is at a uniform temperature, T, and
that DT is the temperature difference between the gas and the wall
of the vessel enclosing it. If this is true, then the heat loss
to the walls of this vessel can be described mathematically by:
where h is the coefficient of heat transfer between the gas and
the walls of the vessel and S is the surface area.
The critical ambient temperature, Ta,crit, is defined
as the temperature at which the heat production is equal to the
heat lost. In this situation,
and, taking the derivative with respect to the gas temperature,

The heat released by combustion is expressed by the following formula:
Tus, Equation 2 becomes:

and Equation 3 becomes:
dividing Equation 5 by Equation 6 yields
by assuming EA>>RT, Equation 7 is solved by binomial
expansion for values of the equilibrium gas temperature. This solution,
however, is not very realistic because it assumes a uniform gas
temperature. Thus, Frank-Kaminetskii (link) developed a model that
takes into account the temperature differences in the gas.
Frank-Kaminetskii (presented in Drysdale)Assuming a one-dimensional
container with uniform symmetrical heating, the heat equation becomes:
for this equation, T is the gas temperature, r is the position
inside the gas, Q is the volumetric rate of heat generation, k is
the thermal conductivity, a is the thermal diffusivity and k takes
a different value depending on geometery (0 for an infinite slab,
1 for an infinite cylinder and 2 for a sphere). In addition, the
reaction rate is assumed to be in a single Arrhenius expression.
Also, there is no reactant consumption , the Biot number is large
enough for conduction to determine the rate of heat loss (Bi >
10) and the thermal properties are independent of temperature.
Thus, the boundary conditions are now:
Tro=To at t≤0 (surface) at r=0 and
t≥0 (center)
If a few non-dimensional variables are defined:
and
Assuming e<<1, Equation 8 becomes:
Declaring a new variable, d, such that

Equation 9 becomes:
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