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10 results for “archean”

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zenodo40/100

Geochemical evidence for high volatile fluxes from the mantle at the end of the Archean: Sample data

<p>This file describes the origin of samples and gives the original xenon data published in refs. 4, 5 and 8. The slopes of the fractionation lines are given in refs. 8 (Table S1), 5 (Tables 1 and S1) and 4 (Table S1). For the barite sample (Ref. 6, Table 1), Xe data were normalized to 132Xe since 130Xe could have been contributed by radioactivity products. In this case &Delta;129Xe was computed from 128Xe and 131,132Xe data. The&nbsp;&Delta;129Xe values were computed from the difference&nbsp;between the isotope fractionation slope (&permil;/u) and the 129Xe/130Xe values in deviation permil (&permil;) relative to the corresponding atmospheric isotope composition.</p>

opencc-by-4.0Aug 2019View details →
zenodo36/100

Metasomatic reactions between Archean dunite and trondhjemite at the Seqi Olivine Mine in Greenland

<p>Supplementary materials relating to the paper: Metasomatic reactions between Archean dunite and trondhjemite at the Seqi Olivine Mine in Greenland by Wyatt et al.</p>

opencc-by-4.0Nov 2019View details →
zenodo36/100

Supplementary material for manuscript *Building Archean cratonic roots*

<p>Scripts and raw data used to plot Figures 1 and 6 of the manuscript &quot;Building Archean cratonic roots&quot; submitted to the Research Topic: &quot;Interior Dynamics and Chemistry of Earth and Other Rocky Planets: Past and Present&quot; at the journal &quot;Frontiers in Earth Science: Solid Earth&quot;</p>

opencc-by-4.0Jun 2022View details →
zenodo36/100

Geochemical evidence for high volatile fluxes from the mantle at the end of the Archean: matlab code

<p>This is the matlab code used to compute past fluxes of mantle-derived Xe to account for the isotopic evolution of atmospheric Xe.&nbsp;</p>

opencc-by-4.0Aug 2019View details →
zenodo36/100

3D simulations of the Archean Earth including photochemical haze profiles [dataset]

<p>Dataset of 3D simulations of the Archean Earth including photochemical haze profiles</p> <p>We present results from 3D simulations of the Archean Earth including a prescribed spherical haze generated through a 1D photochemical model. Our simulations suggest that a thin haze layer, formed when CH4/CO2 = 0.1, leads to global warming of ~10.6K due to the change of water vapour and cloud feedback, compared to the simulation without any haze. However, a thicker haze layer, formed when CH4/CO2 &gt; 0.1, leads to global cooling of up to ~65K as the scattering and absorption of shortwave radiation from the haze reduces the radiation from reaching the planetary surface. A thermal inversion is formed with a lower tropopause as the CH4/CO2 ratio increases. The haze reaches an optical threshold thickness when CH4/CO2 ~ 0.175 beyond which the atmospheric structure and the global surface temperature do not vary much.</p> <p>&nbsp;</p> <p>The IRIS python package developed by the Met Office is needed to analyse the data.</p>

opencc-by-4.0Jul 2023View details →
zenodo32/100

Can Archean Impact Structures be Discovered? A Case Study from Earth's Largest, Most Deeply Eroded Impact Structure. Additional Data.

<p>Modeling inputs: Input files for iSALE.&nbsp;</p> <p>Code: Files for Matlab.&nbsp;</p> <p>Out: Graphs and tabulated results.&nbsp;</p>

opencc-by-4.0May 2023View details →
dryad32/100

Data from: The Archean origin of oxygenic photosynthesis and extant cyanobacterial lineages

Open the record for dataset details and reuse information.

publicOct 2021View details →
zenodo28/100

Two metamorphic gold mineralization events confirmed by Lu-Hf isotope dating of garnet in the Late Archean Storø Au deposit, Nuuk region of SW Greenland

<p><strong>Supplementary material</strong></p> <p><strong>Table A1.</strong> LA-ICP-MS data for a profile through a representative garnet from sample KSZ 21.</p> <p>&nbsp;</p> <p><strong>Table A2.</strong> Lu-Hf isotope data for garnet separates. The samples are described in Szilas et al. (2014).</p> <p>&nbsp;</p> <p><strong>Table A3.</strong> Lu-Hf isotope data for bulk-rock samples. The samples are described in Szilas et al. (2016).</p>

opencc-by-4.0Mar 2020View details →
zenodo28/100

Extended Data Tables for "Geological evidence for high H2 production from komatiites in the Archean"

<p>Extended Data Tables for &quot;Geological evidence for high H2 production from komatiites in the Archean&quot;, including a subset of the global chemistry database of Gard et al. (2019), for komatiites and komatiitic basalts.</p>

opencc-by-4.0Sep 2023View details →
zenodo24/100

Archean crust and metallogenic zones in the Amazonian Craton sensed by satellite gravity data

<p>This is the geochronology data inventory for the published paper &#39;Archean crust and metallogenic zones in the Amazonian Craton sensed by satellite gravity data&#39; on Scientific Reports.</p> <p>As it reads in the Methods section of the publication: &#39; Geochronological data.To constrain our interpretations over the physical structure of the terranes regard-ing feasible geological evolution, we evaluated their age relationships from a compiled geochronology data set. We examined the TDM model and crystallization ages to unveil the relationships of parent material to a common ancestor reservoir, and crystallization of igneous and protoliths rocks, respectively. Evaluation of &epsilon;Nd determi-nations provide clues for the derivation of crustal material during crystallization and reworking episodes. The compiled data set comprises 414 age determinations from various minerals and methods (Sm-Nd, U-Pb, Pb-Pb, K-Ar, Ar-Ar isotopic systems). The target ages were model (n = 142) and crystallization (n = 272) ages. A total of 99 simultaneous determinations of Sm and Nd isotopic composition and crystallization ages with &epsilon;Nd calcula-tions were compiled to evaluate crustal evolution. Data come from more than 50 publications, most of them cited in papers14&ndash;18,21,22,26,28,30,31,33&ndash;35,42,50 and references therein. We are aware that the geochronology data set is deficient in some aspects, such as the existence of geographical gaps (e.g., western Caraj&aacute;s, southern Bacaj&aacute;), sample collec-tion bias, and preservation of the geochronology record, or even incomplete inspection of the record&#39;.</p>

opencc-by-4.0Feb 2019View details →

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