id ftdatacite:10.1594/pangaea.881943
record_format openpolar
spelling ftdatacite:10.1594/pangaea.881943 2023-05-15T16:39:28+02:00 epsilon-p and pCO2 estimations for ODP Hole 138-846B Mejía, Luz María Mendez-Vicente, Ana Abrevaya, Lorena Lawrence, Kira T Ladlow, Caroline Bolton, Clara T Cacho, Isabel Stoll, Heather M 2017 text/tab-separated-values https://dx.doi.org/10.1594/pangaea.881943 https://doi.pangaea.de/10.1594/PANGAEA.881943 en eng PANGAEA - Data Publisher for Earth & Environmental Science https://dx.doi.org/10.1594/pangaea.881946 https://dx.doi.org/10.1038/ngeo2813 https://dx.doi.org/10.1126/science.1120395 https://dx.doi.org/10.1016/j.epsl.2017.08.034 Creative Commons Attribution 3.0 Unported https://creativecommons.org/licenses/by/3.0/legalcode cc-by-3.0 CC-BY AGE Diatoms, pennales purity Diatoms, biomass as carbon δ13C, diatom-bound organic matter Isotopic fractionation, during photosynthis Neogloboquadrina sp., δ13C Neogloboquadrina sp., δ18O Globigerinoides sacculifer, δ13C Globigerinoides sacculifer, δ18O Coccoliths, Sr/Ca ratio Alkenone Sea surface temperature, annual mean Coefficient Carbon dioxide, partial pressure Comment Drilling/drill rig Calculated from UK'37 Müller et al, 1998 Leg138 Joides Resolution Ocean Drilling Program ODP dataset Dataset 2017 ftdatacite https://doi.org/10.1594/pangaea.881943 https://doi.org/10.1594/pangaea.881946 https://doi.org/10.1038/ngeo2813 https://doi.org/10.1126/science.1120395 https://doi.org/10.1016/j.epsl.2017.08.034 2022-02-08T16:24:46Z In the publication Mejía et al. (2017), for the calculation of diatom epsilon-p and pCO2 at 0.82 and 3.99 Ma we used the Uk'37 SST from the study of Lawrence et al. (2006), which used the Prahl et al. (1988) calibration. For the rest of the record, epsilon p and pCO2 data were calculated using the Uk'37 SST record calibrated using Müller et al. (1998) from the study of Herbert et al. (2016) and adapted to our age model (Shackleton et al., 1995).For all samples, including those at 0.82 and 3.99 Ma, the epsilon p and pCO2 data shown here are calculated using the Uk'37 SST calibration of Müller et al. (1998) from the study of Herbert et al. (2016), adapted to our age model (Shackleton et al., 1995). Changing the calibration used for the first two samples from Prahl et al. (1988) to Müller et al. (1998) (SST values taken from Herbert et al., (2016)), results in pCO2 estimates of up to 5.1 ppm higher than that reported in Mejía et al. (2017). The use of the Müller et al. (1998) calibration for the Uk'37 SST of the youngest sample would entail insignificant changes in the b* required to obtain a pCO2 of 229 ppmv (from 97, pCO2 of 233 ppmv to 95.5, pCO2 of 229 ppmv). This is not propagated through the remaining calculations because the reproducibility of the ice core pCO2 records is within this range of pCO2 variation (±3 ppmv). Data of the post 5 Ma alkenone concentrations were taken from the study of Lawrence et al. (2006). Data of Pre 5 Ma alkenone concentrations shown here are adapted to the age model of our diatom samples (Shackleton et al., 1995). The full record can be found in spreadsheet "Pre 5Ma alkenone and SST record". Dataset ice core DataCite Metadata Store (German National Library of Science and Technology) Shackleton
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
topic AGE
Diatoms, pennales purity
Diatoms, biomass as carbon
δ13C, diatom-bound organic matter
Isotopic fractionation, during photosynthis
Neogloboquadrina sp., δ13C
Neogloboquadrina sp., δ18O
Globigerinoides sacculifer, δ13C
Globigerinoides sacculifer, δ18O
Coccoliths, Sr/Ca ratio
Alkenone
Sea surface temperature, annual mean
Coefficient
Carbon dioxide, partial pressure
Comment
Drilling/drill rig
Calculated from UK'37 Müller et al, 1998
Leg138
Joides Resolution
Ocean Drilling Program ODP
spellingShingle AGE
Diatoms, pennales purity
Diatoms, biomass as carbon
δ13C, diatom-bound organic matter
Isotopic fractionation, during photosynthis
Neogloboquadrina sp., δ13C
Neogloboquadrina sp., δ18O
Globigerinoides sacculifer, δ13C
Globigerinoides sacculifer, δ18O
Coccoliths, Sr/Ca ratio
Alkenone
Sea surface temperature, annual mean
Coefficient
Carbon dioxide, partial pressure
Comment
Drilling/drill rig
Calculated from UK'37 Müller et al, 1998
Leg138
Joides Resolution
Ocean Drilling Program ODP
Mejía, Luz María
Mendez-Vicente, Ana
Abrevaya, Lorena
Lawrence, Kira T
Ladlow, Caroline
Bolton, Clara T
Cacho, Isabel
Stoll, Heather M
epsilon-p and pCO2 estimations for ODP Hole 138-846B
topic_facet AGE
Diatoms, pennales purity
Diatoms, biomass as carbon
δ13C, diatom-bound organic matter
Isotopic fractionation, during photosynthis
Neogloboquadrina sp., δ13C
Neogloboquadrina sp., δ18O
Globigerinoides sacculifer, δ13C
Globigerinoides sacculifer, δ18O
Coccoliths, Sr/Ca ratio
Alkenone
Sea surface temperature, annual mean
Coefficient
Carbon dioxide, partial pressure
Comment
Drilling/drill rig
Calculated from UK'37 Müller et al, 1998
Leg138
Joides Resolution
Ocean Drilling Program ODP
description In the publication Mejía et al. (2017), for the calculation of diatom epsilon-p and pCO2 at 0.82 and 3.99 Ma we used the Uk'37 SST from the study of Lawrence et al. (2006), which used the Prahl et al. (1988) calibration. For the rest of the record, epsilon p and pCO2 data were calculated using the Uk'37 SST record calibrated using Müller et al. (1998) from the study of Herbert et al. (2016) and adapted to our age model (Shackleton et al., 1995).For all samples, including those at 0.82 and 3.99 Ma, the epsilon p and pCO2 data shown here are calculated using the Uk'37 SST calibration of Müller et al. (1998) from the study of Herbert et al. (2016), adapted to our age model (Shackleton et al., 1995). Changing the calibration used for the first two samples from Prahl et al. (1988) to Müller et al. (1998) (SST values taken from Herbert et al., (2016)), results in pCO2 estimates of up to 5.1 ppm higher than that reported in Mejía et al. (2017). The use of the Müller et al. (1998) calibration for the Uk'37 SST of the youngest sample would entail insignificant changes in the b* required to obtain a pCO2 of 229 ppmv (from 97, pCO2 of 233 ppmv to 95.5, pCO2 of 229 ppmv). This is not propagated through the remaining calculations because the reproducibility of the ice core pCO2 records is within this range of pCO2 variation (±3 ppmv). Data of the post 5 Ma alkenone concentrations were taken from the study of Lawrence et al. (2006). Data of Pre 5 Ma alkenone concentrations shown here are adapted to the age model of our diatom samples (Shackleton et al., 1995). The full record can be found in spreadsheet "Pre 5Ma alkenone and SST record".
format Dataset
author Mejía, Luz María
Mendez-Vicente, Ana
Abrevaya, Lorena
Lawrence, Kira T
Ladlow, Caroline
Bolton, Clara T
Cacho, Isabel
Stoll, Heather M
author_facet Mejía, Luz María
Mendez-Vicente, Ana
Abrevaya, Lorena
Lawrence, Kira T
Ladlow, Caroline
Bolton, Clara T
Cacho, Isabel
Stoll, Heather M
author_sort Mejía, Luz María
title epsilon-p and pCO2 estimations for ODP Hole 138-846B
title_short epsilon-p and pCO2 estimations for ODP Hole 138-846B
title_full epsilon-p and pCO2 estimations for ODP Hole 138-846B
title_fullStr epsilon-p and pCO2 estimations for ODP Hole 138-846B
title_full_unstemmed epsilon-p and pCO2 estimations for ODP Hole 138-846B
title_sort epsilon-p and pco2 estimations for odp hole 138-846b
publisher PANGAEA - Data Publisher for Earth & Environmental Science
publishDate 2017
url https://dx.doi.org/10.1594/pangaea.881943
https://doi.pangaea.de/10.1594/PANGAEA.881943
geographic Shackleton
geographic_facet Shackleton
genre ice core
genre_facet ice core
op_relation https://dx.doi.org/10.1594/pangaea.881946
https://dx.doi.org/10.1038/ngeo2813
https://dx.doi.org/10.1126/science.1120395
https://dx.doi.org/10.1016/j.epsl.2017.08.034
op_rights Creative Commons Attribution 3.0 Unported
https://creativecommons.org/licenses/by/3.0/legalcode
cc-by-3.0
op_rightsnorm CC-BY
op_doi https://doi.org/10.1594/pangaea.881943
https://doi.org/10.1594/pangaea.881946
https://doi.org/10.1038/ngeo2813
https://doi.org/10.1126/science.1120395
https://doi.org/10.1016/j.epsl.2017.08.034
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