A theoretical study of combustion in porous media driven by a gravity
induced gas flux is conducted. Filtration of the oxidizer carrying gas
arises in response to heating of the gas due to exothermic conversion
of the solid fuel. Specifically, we consider a reaction front propaga
ting through a porous matrix consisting of reactive (fuel) and inert c
omponents. Gas, consisting of both oxidizer and inert components, filt
ers through the matrix and reacts with the solid fuel. The hot gases i
n the medium rise due to buoyancy, thus drawing in Fresh gas from belo
w. Pie employ approximate analytical methods and numerical simulations
to analyze all the basic combustion phenomena, including self ignitio
n, external ignition, both upward and downward as well as adiabatic an
d nonadiabatic propagating combustion waves. Our simulations also desc
ribe the dynamics of buoyancy driven combustion waves. In conventional
combustion systems the combustion waves are traveling waves, whose wa
ve characteristics, e.g., propagation velocity and shape, are constant
, and the time and length scales for the ignition period are independe
nt of the length L of the sample. In contrast, here the waves are not
traveling waves. Rather, they are quasisteady waves, whose characteris
tics do depend on L. Thus, knowledge of the combustion characteristics
determined From experiments on a specific sample of a given size can
not be generalized to samples of larger size as is the case in convent
ional combustion. We derive estimates for the dependence of various co
mbustion characteristics on L. Finally, suggestions for the experiment
al verification of some of the qualitative results of our analysis are
presented.