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NARROW
GeoRef Subject
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all geography including DSDP/ODP Sites and Legs
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Asia
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Far East
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China
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Fujian China (1)
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elements, isotopes
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isotope ratios (1)
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isotopes
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radioactive isotopes
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U-238/U-235 (1)
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metals
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actinides
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uranium
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U-238/U-235 (1)
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alkaline earth metals
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calcium (1)
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cobalt (1)
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iron
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ferrous iron (1)
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zinc (1)
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geochronology methods
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igneous rocks
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igneous rocks
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meteorites
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meteorites
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achondrites
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silicates
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pyroxene group
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orthopyroxene
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enstatite (2)
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framework silicates
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feldspar group
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plagioclase (2)
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orthosilicates
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nesosilicates
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zircon group
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zircon (1)
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Primary terms
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Asia
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Far East
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China
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asteroids (1)
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data processing (1)
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volcanic rocks
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basalts (1)
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mantle (3)
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metals
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actinides
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uranium
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alkaline earth metals
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calcium (1)
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cobalt (1)
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iron
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ferrous iron (1)
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zinc (1)
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metamorphism (1)
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meteorites
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iron meteorites (1)
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stony irons (1)
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stony meteorites
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achondrites
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eucrite (1)
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lunar meteorites (1)
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mineralogy (1)
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Moon (1)
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Serra de Mage Meteorite
Orthopyroxene from the Serra de Mage Meteorite; a structure-refinement procedure for a Pbca phase coexisting with a C2/c exsolved phase
Orthopyroxene from the Serra de Magé Meteorite: Structure refinement and estimation of C 2/ c pyroxene contributions to apparent Pbca diffraction violations
Orientation of exsolution lamellae in mantle xenolith pyroxenes and implications for calculating exsolution pressures
Ordering state in orthopyroxene as determined by precession electron diffraction
The effect of Ca substitution on the elastic and structural behavior of orthoenstatite
High-pressure phase transitions of Fe-bearing orthopyroxene revealed by Raman spectroscopy
Crystal structure of Guinier-Preston zones in orthopyroxene: Z-contrast imaging and ab inito study
The induced thermoluminescence and thermal history of plagioclase feldspars
Solid solutions and phase transitions in (Ca,M 2+ )M 2+ Si 2 O 6 pyroxenes (M 2+ = Co, Fe, Mg)
Ca-Zn solid solutions in C 2/ c pyroxenes: Synthesis, crystal structure, and implications for Zn geochemistry
The meteorite collection of the National Museum of Natural History in Paris, France
Abstract The French national meteorite collection of the Muséum National d'Histoire Naturelle (MNHN) represents one of the richest collections in the world in terms of its historical heritage and scientific value, particularly for samples of observed falls (512). In fact, early meteoritic research was dominated by French 18th and 19th century scientists such as René Just Haüy, Auguste Daubrée, Stanislas Meunier and Alfred Lacroix. They all contributed, along with Jean Orcel and Paul Pellas in the last 80 years, to form this exceptional collection. The fall at L'Aigle in 1803 led to the recognition of the nature of meteorites and the promotion of the science of meteoritics by Jean-Baptiste Biot. The first catalogue of the meteorite collection elaborated by Cordier in 1837 contained 43 specimens. The collection now contains about 3385 specimens representing 1343 distinct meteorites, to which can be added at least 3000 tektites and numerous specimens of impactites, casts, artificial samples and thin sections. France has the greatest number of meteorite falls by surface unit and by number of inhabitants, with 70 distinct meteorite falls recovered. The collection offers a diverse range of meteorites such as those containing rare presolar grains, the famous carbonaceous chondrite Orgueil (fall, 14 May 1864), the first martian meteorite, Chassigny (fall, 3 October 1815) and Ensisheim (fall, 7 November 1492), which is one of the two oldest observed and documented meteorites and the first meteorite to be registered in the catalogue. The MNHN collection represents a resource that is particularly appreciated by the scientific community.
Carryover of Sampling Errors and Other Problems in Far-Infrared to Far-Ultraviolet Spectra to Associated Applications
An evolutionary system of mineralogy, Part IV: Planetesimal differentiation and impact mineralization (4566 to 4560 Ma)
History of the American Museum of Natural History meteorite collection
Abstract The core meteorite collection of the American Museum of Natural History (AMNH), New York, including the massive Cape York and Willamette irons, dates from the three decades ending in 1905. Acquisition of new meteorites was steady into the 1970s, and accelerated in the latter 20th century. Institutional and philanthropic support, coupled with the focus, energy and vision of a succession of curators, have been central to building the collection, exhibiting meteorites, educating the public and participating at the cutting edge of meteoritical science. Efforts to describe and classify, characteristic of the pre-war period, evolved into detailed chemical investigations. Recent science seeks to find underlying processes unifying disparate meteorite groups in a coherent story of the early solar system and planet formation.