“…New oxygen and hydrogen isotope ratios of secondary silica precipitates in the residual rubble breccia: (1) yield continental palaeotemperature estimates between 17 and 22 °C; and, (2) indicate that meteoric water played a role in the crystallization history of the secondary silica. …”
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“…Low praecaecal digestibility of starch causes a forced microbial fermentation accounting for energy losses and meteorism. To optimise dietetic measures, knowledge of praecaecal digestibility of starch is needed but such information from PEI patients is rare. …”
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“…Monthly meteoric water lines have slopes similar to the Global Meteoric Water Line (∼8) for winter months and more evaporated slopes (∼6) during the summer. …”
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“…One-way analysis of variance for δ(13)C, δ(2)H and δ(18)O showed some significant differences either between crop years or geoclimatic conditions. …”
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“…They homogenize by bubble disappearance at 100–200 °C, whereas the estimated entrapment depth is ~ 3–5.5 km. …”
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“…We analysed major ions, trace elements, tritium activity, (14)C, δ(18)O(H2O), δ(2)H(H2O,) δ(13)C(DIC), gas composition and noble gases in six wells. …”
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“…Kapabacteria genome contained both the sulfate reduction pathway and cytochrome c oxidase. Presumably, the availability of buried organic matter of Mesozoic marine sediments, long-term recharge of the aquifer with meteoric waters and its spatial heterogeneity provided the conditions for the development of microbial communities, taxonomically and functionally more diverse than those found in oligotrophic underground ecosystems.…”
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“…The oldest carbonates (∼31 to >50 kyr) are localized calcite, dolomite, and aragonite veins, formed between 26°C and 43°C and related to focused fluid flow. Subsequent pervasive small amounts of dispersed carbonate precipitated in the last 1,000 years. …”
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“…The water/rock mass ratio of 0.065~0.115 suggests the δ(18)O garnet composition is ~1‰ at temperatures ranging from 250–450 °C. The low oxygen isotopic composition indicates the role of meteoric water in the garnet formation. …”
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“…The δ(18)O had a significant positive correlation with temperature, and the δ(18)O-temperature gradient ranged from 0.28‰/°C to 0.68‰/°C. However, the dependence of δ(18)O on precipitation was unclear; a significant precipitation effect was only observed at the Zhangye and Teheran stations, showing δ(18)O-precipitation gradients of 0.20‰/mm and −0.08‰/mm, respectively. …”
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“…In the immediate postoperative period, the patient started reporting nausea/vomiting, abdominal pain at pressure, moderate meteorism, abdominal distension, hypoactive bowel sounds, and fever. …”
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“….%) hydroxyl (OH) component, interpreted as evidence for secondary hydration by meteoric water. BRIC glasses contain the most depleted hydrogen isotopes yet measured in terrestrial rocks, down to δD = −325 ‰. …”
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“…The obtained results indicated non-existence of paleo recharge; rather all groundwater in the basin were found to be essentially of meteoric origin with intermittent surface water contributions. …”
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“…We also report δ(18)O analyses of phenocrysts and groundmass in samples, δ(18)O-δ(13)C analyses of limestones and limestone xenoliths in the Chegem ignimbrite, and coupled δ(18)O-δD-Δ(17)O analyses of glass and groundmass of rock samples from the Chegem ignimbrites that show abundant evidence of post-emplacement interaction with meteoric waters. …”
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“…The process was once thought to be driven by oxygen delivered to deep petroleum reservoirs by meteoric water. This paradigm has been replaced by a view that the process is anaerobic and frequently associated with methanogenic hydrocarbon degradation. …”
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“…Here we describe a new approach to paleo-latitudinal reconstruction based on simultaneous determination of carbonate formation temperature and δ(18)O of soil carbonates, constrained by the abundances of (13)C-(18)O bonds in palaeosol carbonates. Assuming that the palaeosol carbonates have a strong relationship with the composition of the meteoric water, δ(18)O carbonate of palaeosol can constrain paleo-latitudinal position. …”
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“…A combination of fluid inclusion data and stable δ(18)O value for barite (+ 6.71‰ VSMOW) suggests that low-salinity barite-forming solutions resulted from the mixing of strongly-diluted meteoric waters (enriched in light oxygen isotope) with magmatic-hydrothermal fluids under low-temperature conditions (< 100 °C). …”
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“…Gorman’s Well each winter is the result of rapid infiltration, heating and recirculation of meteoric waters within a structurally controlled hydrothermal circulation system. …”
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“…We show that this observation is best explained with the involvement of heated meteoric  waters during their cooling in the crust. …”
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