C. Lowe et Jf. Cassidy, GEOPHYSICAL EVIDENCE FOR CRUSTAL THICKNESS VARIATIONS BETWEEN THE DENALI AND TINTINA FAULT SYSTEMS IN WEST-CENTRAL YUKON, Tectonics, 14(4), 1995, pp. 909-917
Analyses of receiver functions recorded at two broadband seismic stati
ons in the northern Cordillera indicate that the crust is thinner bene
ath Dawson (similar to 35 km) than Whitehorse (similar to 39 km). A si
mple two-dimensional gravity model, constrained by the seismic results
, shows that this change in crustal thickness occurs at about 63 degre
es N, in a zone approximately 35 km wide, where the Moho dips at simil
ar to 8 degrees to the south. The Bouguer anomaly high associated with
the thinner crust can be traced westward into east-central Alaska whe
re crustal thinning and extension are well documented; therefore we pr
opose that west-central Yukon (north of 63 degrees N) has been extende
d also. On the basis of geological and other geophysical data we exami
ne three likely time windows, in the Cretaceous, early Tertiary, and P
resent. We discuss data which indicate that early Tertiary and younger
extension may be related to the transfer of motion from the Denali Fa
ult System inboard to the Tintina Fault System. Earlier Cretaceous ext
ension has been variously attributed to collision related back are ext
ension, syncollisional processes, or gravitational collapse of an over
thickened crustal section. The relative importance of extension in the
se periods remains nebulus; however, the correspondence between the tr
ansition in crustal thickness determined in this study and a mapped bo
undary between ''lower'' plate and ''upper'' plate rocks suggests mid-
Cretaceous extension exerted a significant influence on current Moho d
epths.