A global scavenging and circulation ocean model of thorium-230 and protactinium-231 with realistic particle dynamics (ProThorP 0.1)
A global scavenging and circulation ocean model of thorium-230 and protactinium-231 with realistic particle dynamics (ProThorP 0.1)
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具有真实粒子动力学的钍 230 和镤 231 的全球清除和循环海洋模型 (ProThorP 0.1)
DOI:
10.5194/gmd-11-3537-2018
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发表时间:
2017
期刊:
影响因子:
--
通讯作者:
M. Roy‐Barman
中科院分区:
文献类型:
--
作者:
M. V. Hulten;J. Dutay;M. Roy‐Barman
Abstract. In this paper we set forth a 3-D
ocean model of the radioactive trace isotopes 230Th
and 231Pa. The interest arises from the fact that these isotopes
are extensively used for investigating particle transport in the ocean and
reconstructing past ocean circulation. The tracers are reversibly scavenged
by biogenic and lithogenic particles. Our simulations of 230Th and 231Pa are based on the
NEMO–PISCES ocean biogeochemistry general circulation model, which includes
biogenic particles, namely small and big particulate organic carbon, calcium
carbonate and biogenic silica. Small and big lithogenic particles from dust
deposition are included in our model as well. Their distributions generally
compare well with the small and big lithogenic particle concentrations from
recent observations from the GEOTRACES programme, except for boundary
nepheloid layers for which, as of today, there are no non-trivial
prognostic models available on a global scale. Our simulations reproduce
230Th and 231Pa dissolved concentrations: they compare
well with recent GEOTRACES observations in many parts of the ocean.
Particulate 230Th and 231Pa concentrations are
significantly improved compared to previous studies, but they are still too
low because of missing particles from nepheloid layers. Our simulation
reproduces the main characteristics of the 231Pa∕230Th ratio
observed in the sediments and supports a moderate affinity of
231Pa to biogenic silica as suggested by recent observations
relative to 230Th. Future model development may further improve understanding, especially when
this will include a more complete representation of all particles, including
different size classes, manganese hydroxides and nepheloid layers. This can
be done based on our model as its
source code is readily available.
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影响因子:
5.2
作者:
Burckel, Pierre;Waelbroeck, Claire;Thil, Francois
通讯作者:
Thil, Francois
影响因子:
5.3
作者:
Deng, Feifei;Thomas, Alex L.;Henderson, Gideon M.
通讯作者:
Henderson, Gideon M.
影响因子:
64.8
作者:
Boehm, E.;Lippold, J.;Deininger, M.
通讯作者:
Deininger, M.
影响因子:
4.1
作者:
Sinha B
通讯作者:
Sinha B