Ea. Parfitt et Jw. Head, BUFFERED AND UNBUFFERED DIKE EMPLACEMENT ON EARTH AND VENUS - IMPLICATIONS FOR MAGMA RESERVOIR SIZE, DEPTH, AND RATE OF MAGMA REPLENISHMENT, Earth, moon, and planets, 61(3), 1993, pp. 249-281
Models of the emplacement of lateral dikes from magma chambers under c
onstant (buffered) driving pressure conditions and declining (unbuffer
ed) driving pressure conditions indicate that the two pressure scenari
os lead to distinctly different styles of dike emplacement. In the unb
uffered case, the lengths and widths of laterally emplaced dikes will
be severely limited and the dike lengths will be highly dependent on c
hamber size; this dependence suggests that average dike length can be
used to infer the dimensions of the source magma reservoir. Probable e
xamples on Earth of the unbuffered case are flanking rift zones on shi
eld volcanoes such as the Hawaiian Kilauea East Rift Zone, in which th
e dikes of average widths of less than a meter extend for several km f
rom the central part of the edifice. In contrast, emplacement of later
al dikes in the constant driving pressure (buffered) case can produce
dikes which have sizes and widths which are very large, and are indepe
ndent of chamber size. For relatively shallow magma chambers, buffered
emplacement is expected to produce graben of relatively fixed length
which are associated with eruptive fissures and long, large volume lav
a flows. A decline in magma supply rate and loss of pressure buffering
during the later stages of such eruptions may give rise to caldera fo
rmation/collapse events. Deeper dikes are not likely to erupt but will
produce surface graben of variable length. Therefore, edifices or dik
e swarms which show an extremely wide variation in fracture or dike le
ngths are likely to have been formed in buffered conditions. On Earth.
the characteristics of many mafic-dike swarms suggest that they were
emplaced in buffered conditions (e.g., the Mackenzie dike swarm in Can
ada and some dikes within the Scottish Tertiary). On Venus. the distin
ctive radial fractures and graben surrounding circular to oval feature
s and edifices on many size scales and extending for hundreds to over
a thousand km are candidates for dike emplacement in buffered conditio
ns.