Medial moraines form striking dark. stripes that widen non-linearly, steepe
n laterally and increase in relief down-glacier from the equilibrium line.
Coalescence of these low-ablation-rate features can feed back strongly on t
he mass balance of a glacier snout. Ablation-dominated medial moraines orig
inate from debris delivered to glacier margins, producing a debris-rich sep
tum between tributary streams of ice below their confluence. Emergence of t
his ice below the equilibrium line delivers debris to the glacier surface,
which then moves down local slopes of evolving morainal topography. A quant
itative description of moraine evolution requires specification of the debr
is concentration field within the glacier, treatment of the melt-rate depen
dence on debris thickness, and characterization of processes that transport
debris once it emerges onto the ice surface. Debris concentration at glaci
er tributary junctions scales with the erosion rates and the lengths of the
tributary-valley walls, and inversely with the tributary ice speeds. Melt
rate is damped exponentially by debris, with a similar to 10 cm decay scale
. Debris flux across the glacier surface scales with die product of debris
thickness and local slope. Analytical and numerical results show that media
l moraines should develop cross-glacier profiles with parabolic crests and
linear slopes, and should widen with age and hence distance down-glacier. D
ebris should be both thin and uniform over the moraine. Observed faster-tha
n-linear growth of moraine widths with distance reflects the increasing abl
ation rate down-glacier. Increase in medial moraine cover reduces the local
average ablation rate, allowing the glacier to extend further down-valley
than meteorology alone would suggest. This feedback is especially effective
when moraines merge.