The flame spread rates over PMMA sheets are measured throughout the thin an
d the thick regimes with varying oxygen level and pressure in normal-gravit
y. The prediction by Extended Simplified Theory (EST) shows good agreement
with the experimental results in the thermal regime where relatively high o
pposed-flow exists. In micro-gravity, the spread rate over thin PMMA sheets
is measured with varying opposed-flow velocity and oxygen level. When the
opposed-flow velocity is very low, the thermal regime assumption breaks dow
n so that the radiative effect becomes significant. As the radiative effect
appears, the mass diffusion layer grows faster than the thermal layer, and
the flame spread is suppressed due to the shortage of oxygen. On the other
hand, if the oxygen level is high and/or thickness of the fuel is sufficie
ntly thin, the radiative effect is negligible and the steady spread is esta
blished even in a quiescent environment.