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  • 1
    Publication Date: 2023-01-19
    Description: Detailed imaging of accretionary wedges reveals splay fault networks that could pose a significant tsunami hazard. However, the dynamics of multiple splay fault activation during megathrust earthquakes and the consequent effects on tsunami generation are not well understood. We use a 2‐D dynamic rupture model with complex topo‐bathymetry and six curved splay fault geometries constrained from realistic tectonic loading modeled by a geodynamic seismic cycle model with consistent initial stress and strength conditions. We find that all splay faults rupture coseismically. While the largest splay fault slips due to a complex rupture branching process from the megathrust, all other splay faults are activated either top down or bottom up by dynamic stress transfer induced by trapped seismic waves. We ascribe these differences to local non‐optimal fault orientations and variable along‐dip strength excess. Generally, rupture on splay faults is facilitated by their favorable stress orientations and low strength excess as a result of high pore‐fluid pressures. The ensuing tsunami modeled with non‐linear 1‐D shallow water equations consists of one high‐amplitude crest related to rupture on the longest splay fault and a second broader wave packet resulting from slip on the other faults. This results in two episodes of flooding and a larger run‐up distance than the single long‐wavelength (300 km) tsunami sourced by the megathrust‐only rupture. Since splay fault activation is determined by both variable stress and strength conditions and dynamic activation, considering both tectonic and earthquake processes is relevant for understanding tsunamigenesis.
    Description: Plain Language Summary: In subduction zones, where one tectonic plate moves beneath another, earthquakes can occur on many different faults. Splay faults are relatively steep faults that branch off the largest fault (the megathrust) in a subduction zone. As they are steeper than the megathrust, the same amount of movement on them could result in more vertical displacement of the seafloor. Therefore, splay faults are thought to play an important role in the generation of tsunamis. Here, we use computer simulations to study if an earthquake can break multiple splay faults at once and how this affects the resulting tsunami. We find that multiple splay faults can indeed fail during a single earthquake due to the stress changes from trapped seismic waves, which promote rupture on splay faults. Rupture on splay faults results in larger seafloor displacements with smaller wavelengths, so the ensuing tsunami is bigger and results in two main flooding episodes at the coast. Our results show that it is important to consider rupture on splay faults when assessing tsunami hazard.
    Description: Key Points: Multiple splay faults can be activated during a single earthquake by megathrust slip and dynamic stress transfer due to trapped waves. Splay fault activation is facilitated by their favorable orientation with respect to the local stress field and their closeness to failure. Long‐term geodynamic stresses and fault geometries affect dynamic splay fault rupture and the subsequent tsunami.
    Description: Volkswagen Foundation (VolkswagenStiftung) http://dx.doi.org/10.13039/501100001663
    Description: Royal Society (The Royal Society) http://dx.doi.org/10.13039/501100000288
    Description: EC | H2020 | H2020 Priority Excellent Science | H2020 European Research Council (ERC) http://dx.doi.org/10.13039/100010663
    Description: Deutsche Forschungsgemeinschaft (DFG) http://dx.doi.org/10.13039/501100001659
    Description: National Science Foundation (NSF) http://dx.doi.org/10.13039/100000001
    Description: https://github.com/TUM-I5/SWE
    Description: https://doi.org/10.5281/zenodo.6969455
    Keywords: ddc:551 ; earthquake ; tsunami ; subduction zone ; dynamic rupture ; splay fault ; numerical modeling
    Language: English
    Type: doc-type:article
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  • 2
    Publication Date: 2023-11-15
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Chemical processing of reactive nitrogen species, especially of NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 (= NO + NO〈sub〉2〈/sub〉) and nitrous acid (HONO), determines the photochemical ozone production and oxidation capacity in the troposphere. However, sources of HONO and NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 in the remote marine atmosphere are still poorly understood. In this work, the multiphase chemistry mechanism CAPRAM in the model framework SPACCIM was used to study HONO formation at Cape Verde (CVAO) in October 2017, adopted with the input of current parameterizations for various HONO sources. Three simulations were performed that adequately reproduced ambient HONO levels and its diurnal pattern. The model performance for NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 and O〈sub〉3〈/sub〉 improves significantly when considering dust‐surface‐photocatalytic conversions of reactive nitrogen compounds with high correlation coefficients up to 0.93, 0.56, and 0.89 for NO, NO〈sub〉2〈/sub〉, and O〈sub〉3〈/sub〉, respectively. Photocatalytic conversion of the adsorbed HNO〈sub〉3〈/sub〉 on dust is modeled to be the predominant contributor for daytime HONO at CVAO, that is, accounting for about 62% of the chemical formation rate at noontime. In contrast, the ocean‐surface‐mediated conversion of NO〈sub〉2〈/sub〉 to HONO and other discussed pathways are less important. The average OH levels at midday (9:00–16:00) modeled for cluster trajectory 1, 2, and 3 are 5.2, 5.1, and 5.2 × 10〈sup〉6〈/sup〉 molecules cm〈sup〉−3〈/sup〉, respectively. Main OH formation is driven by O〈sub〉3〈/sub〉 photolysis with a contribution of 74.6% to the total source rate, while HONO photolysis is negligible (∼1.8%). In summary, this study highlights the key role of dust aerosols for HONO formation and NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 cycling at CVAO and possibly in other dust‐affected regions, urgently calling for further investigations using field and model studies.〈/p〉
    Description: Plain Language Summary: Chemical processing of NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 (= NO + NO〈sub〉2〈/sub〉) and nitrous acid (HONO) is important for the tropospheric O〈sub〉3〈/sub〉 budget and oxidation capacity. However, the sources of HONO and cycling of NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 in the remote marine atmosphere are still poorly explored. A detailed multiphase chemistry model simulation showed a better performance of HONO, NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 and O〈sub〉3〈/sub〉 when considering dust‐surface‐photocatalytic conversions of reactive nitrogen compounds, especially the photocatalytic conversion of the adsorbed HNO〈sub〉3〈/sub〉 on dust. The simulations demonstrated that OH formation is mainly driven by the O〈sub〉3〈/sub〉 photolysis, while HONO photolysis is a negligible OH radical source due to its low concentration levels at Cape Verde. The study highlights the key role of dust aerosols for HONO and NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 chemistry in the remote marine boundary layer.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉The sources of HONO and NO〈sub〉〈italic〉x〈/italic〉〈/sub〉 at Cape Verde are well modeled with CAPRAM〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Photocatalytic conversion of adsorbed HNO〈sub〉3〈/sub〉 on dust is the predominant contributor for daytime HONO〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Photolysis of O〈sub〉3〈/sub〉 is the prevailing source of OH radical at Cape Verde, while HONO photolysis is a negligible OH radical source〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Leibniz Association SAW
    Description: Horizon 2020 Framework Programme http://dx.doi.org/10.13039/100010661
    Description: National Key Research and Development Program of China http://dx.doi.org/10.13039/501100012166
    Description: National Natural Science Foundation of China http://dx.doi.org/10.13039/501100001809
    Description: https://doi.org/10.5281/zenodo.8070265
    Description: http://mcm.york.ac.uk/
    Description: https://capram.tropos.de/
    Description: https://ebas.nilu.no/
    Description: https://www.ready.noaa.gov/HYSPLIT_traj.php
    Keywords: ddc:551 ; HONO ; NOx ; CAPRAM ; heterogenous chemistry ; mineral dust ; OH radical ; marine boundary layer
    Language: English
    Type: doc-type:article
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  • 3
    Publication Date: 2022-12-06
    Description: Molecular‐biological data and omics tools have increasingly been used to characterize microorganisms responsible for the turnover of reactive compounds in the environment, such as reactive‐nitrogen species in groundwater. While transcripts of functional genes and enzymes are used as measures of microbial activity, it is not yet clear how they are quantitatively related to actual turnover rates under variable environmental conditions. As an example application, we consider the interface between rivers and groundwater which has been identified as a key driver for the turnover of reactive‐nitrogen compounds, that cause eutrophication of rivers and endanger drinking water production from groundwater. In the absence of measured data, we developed a reactive‐transport model for denitrification that simultaneously predicts the distributions of functional‐gene transcripts, enzymes, and reaction rates. Applying the model, we evaluate the response of transcripts and enzymes at the river‐groundwater interface to stable and dynamic hydrogeochemical regimes. While functional‐gene transcripts respond to short‐term (diurnal) fluctuations of substrate availability and oxygen concentrations, enzyme concentrations are stable over such time scales. The presence of functional‐gene transcripts and enzymes globally coincides with the zones of active denitrification. However, transcript and enzyme concentrations do not directly translate into denitrification rates in a quantitative way because of nonlinear effects and hysteresis caused by variable substrate availability and oxygen inhibition. Based on our simulations, we suggest that molecular‐biological data should be combined with aqueous geochemical data, which can typically be obtained at higher spatial and temporal resolution, to parameterize and calibrate reactive‐transport models.
    Description: Plain Language Summary: Molecular‐biological tools can detect how many enzymes, functional genes, and gene transcripts (i.e., precursors of enzyme production) associated with a microbial reaction exist in a sample from the environment. Although these measurements contain valuable information about the number of bacteria and how active they are, they do not directly say how quickly a contaminant like nitrate disappears. Nitrate, from agriculture and other sources, threatens groundwater quality and drinking water production. In the process of denitrification, bacteria can remove nitrate by converting it into harmless nitrogen gas using specialized enzymes. The interface between rivers and groundwater is known as a place where denitrification takes place. In this study, we use a computational model to simulate the coupled dynamics of denitrification, bacteria, transcripts, and enzymes when nitrate‐rich groundwater interacts with a nearby river. The simulations yield complex and nonunique relationships between the denitrification rates and the molecular‐biological variables. While functional‐gene transcripts respond to daily fluctuations of environmental conditions, enzyme concentrations and genes are stable over such time scales. High levels of functional‐gene transcripts therefore provide a good qualitative indicator of reactive zones. Quantitative predictions of nitrate turnover, however, will require high‐resolution measurements of the reacting compounds, genes, and transcripts.
    Description: Key Points: We simulate the distributions of functional‐gene transcripts and enzymes related to denitrification at the river‐groundwater interface. Functional‐gene transcripts respond quickly to diurnal fluctuations of substrate and oxygen concentrations. Substrate limitation and oxygen inhibition impede the direct prediction of denitrification rates from transcript or enzyme concentrations.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://doi.org/10.5281/zenodo.6584591
    Description: https://gitlab.com/astoeriko/nitrogene
    Description: https://doi.org/10.5281/zenodo.6584641
    Description: https://gitlab.com/astoeriko/adrpy
    Description: https://doi.org/10.5281/zenodo.5213947
    Description: https://github.com/aseyboldt/sunode
    Keywords: ddc:551 ; reactive‐transport modeling ; denitrification ; groundwater‐river interface ; functional genes ; transcripts ; molecular biology
    Language: English
    Type: doc-type:article
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  • 4
    Publication Date: 2023-11-18
    Description: Cyclostratigraphy and astrochronology are now at the forefront of geologic timekeeping. While this technique heavily relies on the accuracy of astronomical calculations, solar system chaos limits how far back astronomical calculations can be performed with confidence. High‐resolution paleoclimate records with Milankovitch imprints now allow reversing the traditional cyclostratigraphic approach: Middle Eocene drift sediments from Newfoundland Ridge are well‐suited for this purpose, due to high sedimentation rates and distinct lithological cycles. Per contra, the stratigraphies of Integrated Ocean Drilling Program Sites U1408–U1410 are highly complex with several hiatuses. Here, we built a two‐site composite and constructed a conservative age‐depth model to provide a reliable chronology for this rhythmic, highly resolved (〈1 kyr) sedimentary archive. Astronomical components (g‐terms and precession constant) are extracted from proxy time‐series using two different techniques, producing consistent results. We find astronomical frequencies up to 4% lower than reported in astronomical solution La04. This solution, however, was smoothed over 20‐Myr intervals, and our results therefore provide constraints on g‐term variability on shorter, million‐year timescales. We also report first evidence that the g〈sub〉4〈/sub〉–g〈sub〉3〈/sub〉 “grand eccentricity cycle” may have had a 1.2‐Myr period around 41 Ma, contrary to its 2.4‐Myr periodicity today. Our median precession constant estimate (51.28 ± 0.56″/year) confirms earlier indicators of a relatively low rate of tidal dissipation in the Paleogene. Newfoundland Ridge drift sediments thus enable a reliable reconstruction of astronomical components at the limit of validity of current astronomical calculations, extracted from geologic data, providing a new target for the next generation of astronomical calculations.
    Description: Plain Language Summary: The traditional cyclostratigraphic approach is to align and correlate a geologic depth‐series with an astronomical solution. However, the chaotic nature of the Solar System prevents astronomers from precisely calculating planetary motions beyond 40–50 million years ago. This in turn limits the options for geologists to use the resulting oscillations in Earth's climate system as a metronome for determining geologic time. In this study, we reversed the cyclostratigraphic approach and used the highly rhythmical sedimentary deposits from Newfoundland Ridge (North Atlantic) to back‐calculate planetary motions at ∼41 million years ago. The superior quality of the Newfoundland Ridge geoarchive originates from the combination of relatively high sedimentation rates (∼4 cm/kyr) and the time‐continuous character of our two‐site composite record between 39.5 and 42.8 million years ago. In this work, we had to first overcome considerable challenges in reconstructing the timing of sediment deposition, which we did with highly resolved geochemical measurements from two sites. We then were able to extract information on the Earth's planetary motion and on the Earth‐Moon interactions. These astronomical reconstructions based on geological data can now be used by astronomers to describe the evolution of the solar system further back in time than was previously possible.
    Description: Key Points: A new precession‐based cyclostratigraphy for the middle Eocene intervals of IODP Sites U1408 and U1410. Variability in astronomical fundamental frequencies (g‐terms) on million‐year timescales is larger than previously assumed. Our precession constant estimate for 41 Ma (51.28 ± 0.56″/year) confirms earlier indicators of slower tidal dissipation in the Paleogene.
    Description: National Science Foundation http://dx.doi.org/10.13039/100000001
    Description: University of California http://dx.doi.org/10.13039/100005595
    Description: Belgian American Educational Foundation http://dx.doi.org/10.13039/100001491
    Description: https://paloz.marum.de/AstroComputation/index.html
    Description: https://paloz.marum.de/confluence/display/ESPUBLIC/NAFF
    Keywords: ddc:551 ; North Atlantic ; Eocene ; cyclostratigraphy ; astrochronology
    Language: English
    Type: doc-type:article
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