SEISMIC OVERVIEW OF MAKRAN OFFSHORE

Welcome to DSpace BU Repository

Welcome to the Bahria University DSpace digital repository. DSpace is a digital service that collects, preserves, and distributes digital material. Repositories are important tools for preserving an organization's legacy; they facilitate digital preservation and scholarly communication.

Show simple item record

dc.contributor.author Khan, Abdul Rehman
dc.date.accessioned 2018-08-06T06:54:35Z
dc.date.available 2018-08-06T06:54:35Z
dc.date.issued 2015
dc.identifier.uri http://hdl.handle.net/123456789/7103
dc.description.abstract The Makran accretionary prism developed has a kuge potential of kydrocarbons in form of gas consequence of tke subduction of tkekydrates in tke north-western part of tke Indian Ocean as a Arabian Sea since Late Cretaceous times. Tk Makran accretionary prism results from tke nortkward ic crust (Wkite and Klitgord, 1976; Wkite, 1983; Minskull et aL, 1992), with an average speed of 3 cm/year at present. Large kistoric eartkquakes, suck as tke magnitude 8.2 recorded in November 1945 (Packeco and Sykes, 1992; Byrne et aL, 1992), are clearly related to tke skallow dipping inter-plate mega-tkrust. Tkis subduction has caused a tremendous change in tke subsurface Fairly sizable sources and reserves are found. Tke complexity of tke structures is a barrier to the appropriation o/tke data collected. en_US
dc.language.iso en_US en_US
dc.publisher Bahria University Karachi Campus en_US
dc.title SEISMIC OVERVIEW OF MAKRAN OFFSHORE en_US
dc.type Thesis en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Advanced Search

Browse

My Account