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Himalayan
Geology,
Vol. 30 (2), 2009, pp.103-113 Printed in India
Late Quaternary-Holocene fold and landform generated by
morphogenic earthquakes in Chandigarh anticlinal ridge in Panjab Sub
Himalaya
V.C.
THAKUR, R. JAYANGONDAPERUMAL, N. SURESH
Wadia Institute of Himalayan Geology, Dehra Dun - 248 001,
India
Abstract: The Pinjor dun is an
intermontane valley within the Sub Himalaya of Panjab lying between the
rivers Satluj and Ghaggar. The dun is bounded to south by the Frontal
Siwalik Range (FSR) and to north by the Inner Siwalik Range (ISR). The FSR
is made of an anticlinal ridge, trending northwest - southeast, of folded
upper Siwalik strata. The southern margin of the FSR is marked by an abrupt
topographic and tectonic break against the Panjab alluvial plains along the
Himalayan Frontal Thrust (HFT). The HFT was initiated, south of the Nalagarh
Thrust (NT), representing southward propagation of the decollement referred
as Main Himalayan Thrust (MHT) sometime between 0.5 Ma and 0.1 Ma. The
Chandigarh anticline was formed as a fault-bend fold over the HFT. The
anticline is asymmetric, the forelimb on the southern flank has long
terraced streams and mature compared to the back limb on the northern flank
with deeply incised short streams. The drainage pattern, incision of the
landform and geometry of the structure indicates the presence of a blind
back thrust and a fold scarp on the northern margin of the Chandigarh ridge.
South of the HFT, a 10-15 km wide Piedmont Zone (PZ) has been formed with
coalescing alluvial fans. The PZ has rolling topography with streams incised
by a few meters and active deformation features. The Pinjor dun is
interpreted to represent the continuation of the back limb of the anticline
into the flat synformal depression of a piggy - back type basin. The dun is
covered by post- Siwalik Dun formation consisting of sand, silt, mudstone
and gravel of poorly to unconsolidated and horizontally bedded nature. The
sediments were deposited on alluvial fans sourced from the hinterland
Siwaliks and the Lesser Himalaya. The OSL ages of the Dun formation range
more than 90 Ka to 20 Ka. Earthquakes breaking the surface have been
reported along the HFT scarps in Holocene sediments near Chandigarh on the
basis of palaeoseismological studies. The Chandigarh anticline and its ridge
topography appear to have grown as a result of coseismic cumulative slip
during late Quaternary-Holocene generated by repeated large earthquakes,
with assumed average 5-10 m dip-slip and 1000 years recurrence interval. |