We present a kinematic, self-adaptive, numerical model to describe the down
-now thermal and rheological evolution of channel-contained lava. As our co
ntrol volume of lava advances down a channel it cools and crystallizes, an
increasingly thick and extensive surface crust grows, and its heat budget a
nd rheology evolve. By estimating down-flow heat and velocity loss, our mod
el calculates the point at which the control volume becomes stationary, giv
ing the maximum distance lava flowing in the channel can extend. Modeled ef
fusion rates, velocities, widths, surface crust parameters, heat budget, co
oling, temperature, crystallinity, viscosity, and yield strength all compar
e well with field data collected during eruptions at Mauna Loa, Kilauea, an
d Etna. Modeled lengths of 25-27, 2.5-5.7, and 0.59-0.83 km compare with me
asured lengths of 25-27, 4, and 0.75 km for the three flows, respectively.
Over proximal flow portions we calculate cooling, crystallization, viscosit
y, and yield strength of 1-10 degreesC km(-1): 0.001-0.01 volume fraction k
m(-1), 10(3)-10(4) Pa s, and 10(-3)-10(2) Pa, respectively. At the flow fro
nt, cooling, crystallization, viscosity, and yield strength increase to >10
0 degreesC km(-1), 0.1 volume fraction km(-1), 10(6)-10(7) Pa s, and 10(3)-
10(4) Pa, respectively, all of which combine to cause the lava to stop Bowi
ng. Our model presents a means of (a) analyzing lava flow thermo-rheologica
l relationships; (b) identifying important factors in determining how far a
channel-fed flow can extend; (c) assessing lava flow hazard; and (d) recon
structing flow regimes at prehistoric, unobserved, or remote flows.