نتایج جستجو برای: accreted

تعداد نتایج: 1682  

2017
Bethan A. Phillips Andrew C. Kerr Emily K. Mullen Dominique Weis

Article history: Received 11 October 2016 Accepted 5 January 2017 Available online 14 January 2017 The Siletz terrane, a predominantly mafic accreted oceanic terrane, is located in the Cascadia forearc region of Oregon, Washington and Vancouver Island. The terrane represents a late Palaeocene–Eocene large igneous province that consists of pillow lavas, massive flows and intrusive sheets. Previo...

Journal: :Khulna University studies 2022

This research was conducted to observe the constraints of rice cultivation in accreted char land Saint Martin’s Island soils were analyzed and compared with normal reference Batiaghata, Southwest Bangladesh for same variety (BR-11). The soil pH ranged from 7.63 7.74, EC 5.49 dS.m-1 8.24 dS.m-1, CEC 37.87 Cmol(+) kg-1 52.13 , total N 0.086 0.11%, available P 1.6 2.38 µg.g-1 K 149.73 184.93 S 134...

The Khoy Ophiolitic Complex (KOC) as a part of Tethyan, Izmir-Ankara- Erzincan and Bitlis-Zagros sutures of South East (SE) Turkey is broadly exposed around Khoy region (NW Iran). This complex comprises dismembered fragments of mantle lithosphere, obducted oceanic lithosphere and parts of volcanic arc remnants. The Khoy Ophiolitic Complex can be structurally divided into two major eastern and w...

Noghreyan, Mousa, Rezaei, Zahra, Saccani, Emilio,

Sabzevar ophiolitic pillow lavas contain variolitic, porphyritic with microlitic matrix, intersertal and amygdaloidal textures and include plagioclase, clinopyroxene (augite-diopside), olivine, amphibole (magnesiohastingsite) and opaque minerals. The chemical composition of clinopyroxenes show a calc-alkaline magmatic series and a tectonic environment within plate alkaline basalts. Geochemicall...

Journal: :Monthly Notices of the Royal Astronomical Society 2016

Journal: :Monthly Notices of the Royal Astronomical Society 2021

ABSTRACT Galaxy mergers are instrumental in dictating the final mass, structure, stellar populations, and kinematics of galaxies. Cosmological galaxy simulations indicate that most massive galaxies at z = 0 dominated by high fractions ‘ex-situ’ stars, which formed first distinct independent galaxies, then subsequently merged into host galaxy. Using spatially resolved MUSE spectroscopy we quanti...

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