857 research outputs found
Global-mean marine δ13C and its uncertainty in a glacial state estimate
Author Posting. © The Author(s), 2015. This is the author's version of the work. It is posted here by permission of Elsevier for personal use, not for redistribution. The definitive version was published in Quaternary Science Reviews 125 (2015): 144-159, doi:10.1016/j.quascirev.2015.08.010.A paleo-data compilation with 492 δ13C and δ18O observations provides the opportunity
to better sample the Last Glacial Maximum (LGM) and infer its global
properties, such as the mean δ13C of dissolved inorganic carbon. Here, the paleocompilation
is used to reconstruct a steady-state water-mass distribution for the
LGM, that in turn is used to map the data onto a 3D global grid. A global-mean
marine δ13C value and a self-consistent uncertainty estimate are derived using the
framework of state estimation (i.e., combining a numerical model and observations).
The LGM global-mean δ13C is estimated to be 0:14h±0:20h at the
two standard error level, giving a glacial-to-modern change of 0:32h±0:20h.
The magnitude of the error bar is attributed to the uncertain glacial ocean circulation
and the lack of observational constraints in the Pacific, Indian, and Southern
Oceans. Observations in the Indian and Pacific Oceans generally have 10 times
the weight of an Atlantic point in the computation of the global mean. To halve
the error bar, roughly four times more observations are needed, although strategic
sampling may reduce this number. If dynamical constraints can be used to better
characterize the LGM circulation, the error bar can also be reduced to 0:05 to 0:1h, emphasizing that knowledge of the circulation is vital to accurately map
δ13CDIC in three dimensions.GG is supported
by NSF grants OIA-1124880 and OCE-1357121, the WHOI Ocean and Climate
Change Institute, and The Joint Initiative Awards Fund from the Andrew W. Mellon Foundation
Unsupervised classification reveals new evolutionary pathways
While we already seem to have a general scenario of the evolution of
different types of galaxies, a complete and satisfactory understanding of the
processes that led to the formation of all the variety of today's galaxy types
is still beyond our reach. To solve this problem, we need both large datasets
reaching high redshifts and novel methodologies for dealing with them. The
VIPERS survey statistical power, which observed galaxies at , and the application of an unsupervised clustering algorithm allowed us to
distinguish 12 galaxy classes. Studies of their environmental dependence
indicate that this classification may actually reflect different galaxy
evolutionary paths. For instance, a class of the most passive red galaxies
gathers galaxies smaller than other red galaxies of a similar
stellar mass, revealing the first sample of red nuggets at intermediate
redshift. On the other end, a class of blue dwarf galaxies is composed mainly
of AGN, challenging commonly used mid-infrared AGN selections.Comment: Accepted for publication in the ML4ASTRO (ICML 2022) proceeding boo
Influence of PbX2 (X = F, Cl, Br) content and thermal treatment on structure and optical properties of lead borate glasses doped with rare earth ions
Oxyhalide lead borate glasses doped with rare earth ions have been studied before and after thermal
treatment. The rare earths as optically active ions were limited to the Er3+ ions. Near-infrared
luminescence due to the main 4I13/2–4I15/2 laser transition of Er3+ was registered. The introduction
of PbX2 to the borate glass results in a reduction of spectral linewidth and an increase of luminescence lifetime of 4I13/2 state of Er3+ ions. The unusual large spectral linewidth for 4I13/2–4I15/2 transition of Er3+ in the oxide glass host was obtained, whereas the luminescence decay from 4I13/2 state is longer for a sample with PbF2 than PbCl2 and PbBr2. Heat treatment introduces transformation from a glass to transparent glass-ceramic (TGC). The coordination sphere around Er3+ ions is changed, giving important contribution to the luminescence characteristics. The spectroscopic consequence of this transformation is the increase of
luminescence lifetime and the narrowing of spectral lines of Er3+
Bayesian model selection for the glacial-interglacial cycle
A prevailing viewpoint in paleoclimate science is that a single paleoclimate record contains insufficient information to discriminate between typical competing explanatory models. Here we show that by using SMC 2 (sequential Monte Carlo squared) combined with novel Brownian bridge type proposals for the state trajectories, it is possible to estimate Bayes factors to sufficient accuracy to be able to select between competing models, even with relatively short time series. The results show that Monte Carlo methodology and computer power have now advanced to the point where a full Bayesian analysis for a wide class of conceptual climate models is now possible. The results also highlight a problem with estimating the chronology of the climate record prior to further statistical analysis, a practice which is common in paleoclimate science. Using two datasets based on the same record but with different estimated chronologies, results in conflicting conclusions about the importance of the astronomical forcing on the glacial cycle, and about the internal dynamics generating the glacial cycle, even though the difference between the two estimated chronologies is consistent with dating uncertainty. This highlights a need for chronology estimation and other inferential questions to be addressed in a joint statistical
procedure
Benthic foraminiferal stable carbon isotope constraints on deglacial ocean circulation and carbon-cycle changes
How does deep-ocean circulation influence atmospheric CO2 across deglacial transitions? Although biogeochemical and physical processes complicate interpretation of foraminiferal stable carbon isotope data, these complications can be addressed with expanded data compilations, multiproxy approaches, and model-data assimilation efforts.Fil: Peterson, Carlye D.. University of California Riverside; Estados UnidosFil: Gebbie, G.. Woods Hole Oceanographic Institution; Estados UnidosFil: Lisiecki, L. E.. University of California Santa Barbara; Estados UnidosFil: Lynch Stieglitz, J.. School of Earth and Atmospheric Sciences; Estados UnidosFil: Oppo, D.. Woods Hole Oceanographic Institution; Estados UnidosFil: Muglia, Juan. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Centro Nacional Patagónico. Centro para el Estudio de Sistemas Marinos; ArgentinaFil: Repschläger, Janne. Max Planck Institute for Chemistry; AlemaniaFil: Schmittner, A.. University of Oregon; Estados Unido
On the state dependency of fast feedback processes in (palaeo) climate sensitivity
Palaeo data have been frequently used to determine the equilibrium (Charney)
climate sensitivity , and - if slow feedback processes (e.g. land
ice-albedo) are adequately taken into account - they indicate a similar range
as estimates based on instrumental data and climate model results. Most studies
implicitly assume the (fast) feedback processes to be independent of the
background climate state, e.g., equally strong during warm and cold periods.
Here we assess the dependency of the fast feedback processes on the background
climate state using data of the last 800 kyr and a conceptual climate model for
interpretation. Applying a new method to account for background state
dependency, we find K(Wm) using the latest LGM
temperature reconstruction and significantly lower climate sensitivity during
glacial climates. Due to uncertainties in reconstructing the LGM temperature
anomaly, is estimated in the range K(Wm).Comment: submitted to Geophysical Research Letter
A persistent Norwegian Atlantic Current through the Pleistocene glacials
Changes in ocean‐circulation regimes in the northern North Atlantic and the Nordic Seas may affect not only the Arctic but potentially hemispheric or even global climate. Therefore, unraveling the long‐term evolution of the North Atlantic Current‐Norwegian Atlantic Current system through the Pleistocene glaciations could yield useful information and climatological context for understanding contemporary changes. In this work, ~50,000 km2 of 3‐D seismic reflection data are used to investigate the Pleistocene stratigraphy for evidence of paleo‐oceanographic regimes on the mid‐Norwegian margin since 2.58 Ma. Across 33 semicontinuous regional paleo‐seafloor surfaces ~17,500 iceberg scours have been mapped. This mapping greatly expands our spatiotemporal understanding of currents and iceberg presence in the eastern Nordic Seas. The scours display a dominant southwest‐northeast trend that complements previous sedimentological and numerical modeling studies that suggest northward‐flowing currents in the Norwegian Sea during the Pleistocene. This paleo‐oceanographic study suggests that through many of the Pleistocene glaciations, the location of surface ocean currents in the Norwegian Sea and, by extension, the eastern North Atlantic, were broadly similar to the present
Broadband near-infrared luminescence in lead germanate glass triply doped with Yb3+/Er3+/Tm3+
This paper deals with broadband near-infrared luminescence properties of lead germanate
glass triply doped with Yb3+/Er3+/Tm3+. Samples were excited at 800 nm and 975 nm. Their
emission intensities and lifetimes depend significantly on Er3+ and Tm3+ concentrations. For samples
excited at 800 nm, broadband emissions corresponding to the overlapped 3H4 ! 3F4 (Tm3+) and
4I13/2 ! 4I15/2 (Er3+) transitions centered at 1.45 m and 1.5 m was identified. Measurements of
decay curves confirm reduction of 3H4 (Tm3+), 2F5/2 (Yb3+) and 4I13/2 (Er3+) luminescence lifetimes
and the presence of energy-transfer processes. The maximal spectral bandwidth equal to 269 nm for
the 3F4 ! 3H6 transition of Tm3+ suggests that our glass co-doped with Yb3+/Er3+/Tm3+ is a good
candidate for broadband near-infrared emission. The energy transfer from 4I13/2 (Er3+) to 3F4 (Tm3+)
and cross-relaxation processes are responsible for the enhancement of broadband luminescence near
1.8 m attributed to the 3F4 !3H6 transition of thulium ions in lead germanate glass under excitation
of Yb3+ ions at 975 nm
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