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Tectonics of the Himalaya **damaged stock**

Product code: SP412D

Print publication date: 22/09/2015

Geological Society of London, GSL Special Publications, Reduced while stocks last

Type: Book (Hardback)

Binding: Hardback

ISBN: 9781862397033

Author/Edited by: Edited by S. Mukherjee, R. Carosi, P.A. van der Beek, B.K. Mukherjee and D.M. Robinson

Weight: 0.95kg

Number of pages: 323

Online publication date: 17/08/2015

Lyell Collection URL: http://sp.lyellcollection.org/content/412/1

£70.00

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Full Description

Product Code:SP412D

Edited by S. Mukherjee, R. Carosi, P.A. van der Beek, B.K. Mukherjee and D.M. Robinson

Special Publication 412

*** Reduced price for copies damaged in transit.

Books have damaged covers (on spine, corners and edges) - interior pages are all OK.

Regular prices:
List price: £100.00
Fellow's price: £50.00
Other member societies price: £60.00


The Himalayan mountain belt, which developed during the India–Asia collision starting about 55 Ma ago, is a dramatically active orogen and it is regarded as the classic collisional orogen. It is characterized by an impressively continuous 2500 km of tectonic units, thrusts and normal faults, as well as large volumes of high-grade metamorphic rocks and granites exposed at the surface. This constitutes an invaluable field laboratory, where amazing crustal sections can be observed directly in very deep gorges. It is possible to unravel the tectonic and metamorphic evolution of litho-units, to observe the mechanisms of exhumation of deep-seated rocks and the propagation of the deformation.  Himalayan tectonics has been the target of many studies from numerous international researchers over the years. In the last 15 years there has been an explosion of data and theories from both geological and geophysical perspectives.

This book presents the results of integrated multidisciplinary studies, including geology, petrology, magmatism, geochemistry, geochronology and geophysics, of the structures and processes affecting the continental lithosphere. These processes and their spatial and temporal evolution have major consequences on the geometry and kinematics of the India–Eurasia collision zone.