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1 atic activity (primary outgassing or contact metamorphism).
2 ngite ages reliably record the timing of UHP metamorphism.
3 ted objects subjected to thermal/accretional metamorphism.
4 been reported in association with high-grade metamorphism.
5 ions generated during ultra-high temperature metamorphism.
6 ed, but even they have experienced low-grade metamorphism.
7 ying that the Os(i) carrier was destroyed by metamorphism.
8 served within minerals that are resistant to metamorphism.
9 t exist at mantle depths associated with UHP metamorphism.
10 or providing insight into aspects of organic metamorphism and biochemical evolution, and for clarifyi
12 ring late Archean ca. 2.9 Ga thermal contact metamorphism and not in an early ca. 3.45 Ga subseafloor
14 t in relationships between blueschist-facies metamorphism and seismicity, particularly through dehydr
15 the crystallization of magmas, fluid flow in metamorphism and the sealing of open cracks in earthquak
17 oidal impacts and meteorite craters by shock metamorphism, and in Earth's mantle 1 to 2 billion years
18 n of heat by melt generates granulite facies metamorphism, and widespread andalusite-sillimanite meta
20 intrusions but do not show correlations with metamorphism at intermediate scales (10(0)-10(1) km).
21 mately400°C, it follows that parent body metamorphism cannot explain the absence of 26Mg* in some
22 crust--for the localized nature of eclogite metamorphism during Caledonian crustal thickening, as re
23 very from the mantle through zones of active metamorphism eliminates the mass-balance argument for th
24 tered-Fe domains and 1,412+/-56 Ma (tectonic metamorphism) from planar and subgrain boundary structur
25 ral changes due to chemical transport during metamorphism has been previously impossible both in natu
26 ata that dates the timing of eclogite facies metamorphism in eastern Papua New Guinea at 4.3 +/- 0.4
27 igh monzodioritic proportion and inefficient metamorphism in the Breaksea Orthogneiss resulted in its
28 s constructed to probe the degree of thermal metamorphism in the crust in the effort to recreate the
32 tapped volatile-fertile sediments to contact metamorphism, likely liberating the massive greenhouse g
33 arbonaceous chondrite that experienced shock metamorphism, local melting (with conditions exceeding 5
34 n of CO2 and H2O through the subduction-zone metamorphism of carbonate-bearing marine sediments (whic
36 enozoic orogenesis are flawed, and that some metamorphism of Greater Himalayan rocks may have occurre
37 rom each planet's surface via the burial and metamorphism of hydrated mafic crusts, and calculate min
39 ~4100 Ma dry melting and subsequent ~4070 Ma metamorphism provide new evidence for the diversity of t
45 ted basalt) during high pressure/temperature metamorphism via phengite crystallization from subductio
46 y large sizes in Tissint indicate that shock metamorphism was widely dispersed in this sample (~25 GP
47 that has experienced ultra-high temperature metamorphism, where ion imaging has revealed submicromet
48 lder than 3,500 Myr have experienced intense metamorphism, which would have obliterated any fragile m
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