コーパス検索結果 (1語後でソート)
通し番号をクリックするとPubMedの該当ページを表示します
1 atic activity (primary outgassing or contact metamorphism).
2 es in NWA 7983 record a high degree of shock metamorphism.
3 t exist at mantle depths associated with UHP metamorphism.
4 ngite ages reliably record the timing of UHP metamorphism.
5 ted objects subjected to thermal/accretional metamorphism.
6 been reported in association with high-grade metamorphism.
7 ions generated during ultra-high temperature metamorphism.
8 mation resulting from Pb mobilization during metamorphism.
9 ed, but even they have experienced low-grade metamorphism.
10 ying that the Os(i) carrier was destroyed by metamorphism.
11 typically thought to occur during low-grade metamorphism.
12 served within minerals that are resistant to metamorphism.
13 rved as crystalline graphite during prograde metamorphism.
14 at was accreted to the parent asteroid after metamorphism.
16 or providing insight into aspects of organic metamorphism and biochemical evolution, and for clarifyi
17 which porphyroblast minerals nucleate during metamorphism and carry implications for the role that no
20 archive of diagenetic temperatures, despite metamorphism and exposure to meteoric fluids, and show t
21 ring late Archean ca. 2.9 Ga thermal contact metamorphism and not in an early ca. 3.45 Ga subseafloor
22 first continents that formed via high-grade metamorphism and partial melting of hydrated basaltic cr
25 t in relationships between blueschist-facies metamorphism and seismicity, particularly through dehydr
26 the crystallization of magmas, fluid flow in metamorphism and the sealing of open cracks in earthquak
27 perienced high temperature-to-pressure ratio metamorphism and were most likely transported to deep ar
28 rt on an interpretation that eclogite-facies metamorphism and, therefore, collisional orogenesis, occ
29 s, a granoblastic calcite texture (incipient metamorphism), and subsequent hypidioblastic white mica
31 oidal impacts and meteorite craters by shock metamorphism, and in Earth's mantle 1 to 2 billion years
34 n of heat by melt generates granulite facies metamorphism, and widespread andalusite-sillimanite meta
37 ve aqueous alteration and subsequent thermal metamorphism at 570-670 K (300-400 C), suggesting that R
38 intrusions but do not show correlations with metamorphism at intermediate scales (10(0)-10(1) km).
39 mately400°C, it follows that parent body metamorphism cannot explain the absence of 26Mg* in some
40 tening, magmatism, and high thermal gradient metamorphism connected cratons in Australia, East Antarc
41 e Nimrod Complex indicate that high-pressure metamorphism did not occur in the Palaeoproterozoic, but
42 crust--for the localized nature of eclogite metamorphism during Caledonian crustal thickening, as re
43 very from the mantle through zones of active metamorphism eliminates the mass-balance argument for th
45 tered-Fe domains and 1,412+/-56 Ma (tectonic metamorphism) from planar and subgrain boundary structur
46 ral changes due to chemical transport during metamorphism has been previously impossible both in natu
47 lite transition during burial diagenesis and metamorphism, impeding the maturation of organic materia
48 ata that dates the timing of eclogite facies metamorphism in eastern Papua New Guinea at 4.3 +/- 0.4
50 igh monzodioritic proportion and inefficient metamorphism in the Breaksea Orthogneiss resulted in its
51 s constructed to probe the degree of thermal metamorphism in the crust in the effort to recreate the
55 tapped volatile-fertile sediments to contact metamorphism, likely liberating the massive greenhouse g
56 arbonaceous chondrite that experienced shock metamorphism, local melting (with conditions exceeding 5
57 metamorphic belts(5), which is attributed to metamorphism near (low T/P) and away from (high T/P) sub
58 n of CO2 and H2O through the subduction-zone metamorphism of carbonate-bearing marine sediments (whic
60 enozoic orogenesis are flawed, and that some metamorphism of Greater Himalayan rocks may have occurre
61 rom each planet's surface via the burial and metamorphism of hydrated mafic crusts, and calculate min
65 carbon could possibly confirm the effect of metamorphism on original biomass, but this is still unex
66 sure (thermobaric ratio) of granulite facies metamorphism peaked at over 1500 degrees C/GPa during th
67 ~4100 Ma dry melting and subsequent ~4070 Ma metamorphism provide new evidence for the diversity of t
74 both the crystallization age and age of the metamorphism to ~+/-135 Ma, a significant improvement on
77 results indicate that impact-driven thermal metamorphism under low-pressure conditions led to partia
78 ted basalt) during high pressure/temperature metamorphism via phengite crystallization from subductio
79 y large sizes in Tissint indicate that shock metamorphism was widely dispersed in this sample (~25 GP
81 that has experienced ultra-high temperature metamorphism, where ion imaging has revealed submicromet
82 lder than 3,500 Myr have experienced intense metamorphism, which would have obliterated any fragile m
83 reached 550 K, then fluids released by rock metamorphism would have promoted conditions favorable fo