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Título de Acceso Abierto

Geophysical Research Letters

Resumen/Descripción – provisto por la editorial en inglés
Publishes high-impact, innovative, and timely communications-length articles on major advances spanning all of the major geoscience disciplines.
Palabras clave – provistas por la editorial

encias de la tierra (general) u2013 Geociencias; Geología; Geofísi

Disponibilidad
Institución detectada Período Navegá Descargá Solicitá
No requiere desde ene. 1974 / hasta sep. 2024 Wiley Online Library acceso abierto
open-access-logo  Esta publicación es de Acceso Abierto y no aplica cargos a los/as autores/as.

Información

Tipo de recurso:

revistas

ISSN impreso

0094-8276

ISSN electrónico

1944-8007

Editor responsable

American Geophysical Union (AGU)

País de edición

Estados Unidos

Fecha de publicación

Información sobre derechos de publicación

© 2021 American Geophysical Union

Tabla de contenidos

Two‐Dimensional Hybrid Simulation of the Second‐Harmonic Generation of EMIC Waves in the Inner Magnetosphere

Zuxiang XueORCID; Zhigang YuanORCID; Xiongdong YuORCID; Dan DengORCID

<jats:title>Abstract</jats:title><jats:p>Two‐dimensional (2‐D) hybrid model is developed to investigate the second harmonic (SH) generation of electromagnetic ion cyclotron (EMIC) waves. Applying the singular value decomposition method to simulated fields, we show that the SH exhibits wave properties analogous to typical EMIC waves generated by ion cyclotron instabilities, that is, left‐hand polarization and small wave normal angle. However, the bicoherence index inferred from simulated fields reflects a strong phase coupling between the fundamental wave (FW) and the SH, illustrating the nonlinear generation of the SH by the FW. The necessary conditions, especially for the wave vector relation, are further verified from a 2‐D perspective. The simulated amplitude ratios well meet the theoretical results only in the SH saturation stage, while the necessary conditions remain satisfied almost throughout the simulation. This study provides a comprehensive analysis of the SH excitation in a 2‐D simulation domain, contributing to a deeper understanding of EMIC wave nonlinear generation.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Quantifying the Relative Contributions of the Global Oceans to ENSO Predictability With Deep Learning

Tang LiORCID; Youmin TangORCID; Tao LianORCID; Anfeng Hu

<jats:title>Abstract</jats:title><jats:p>We propose a unified statistical method based on deep learning and analysis to quantify the relative contributions of the global oceans to El Niño–Southern Oscillation (ENSO) predictability. By incorporating subsurface signals in the Indian Ocean and Atlantic, the forecast lead can be skillfully extended by about one season. This skill enhancement mainly originates from the tropical Indian Ocean, presumably related to signals of the Indian Ocean Dipole passing to the tropical Pacific through the Indonesian Throughflow. The sea surface temperature anomaly (SSTA) in the Indian Ocean accounts for nearly 50% of surface contributions to both El Niño and La Niña predictions at a 15‐month lead. The north tropical Atlantic SSTA has a moderate impact on La Niña at a 9‐month lead. The Pacific Meridional Mode plays a significant role in both ENSO phases at a 12‐month lead. Thus, our study suggests that trans‐basin effects for ENSO are more vigorous than previously thought.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Summer Deep Depressions Increase Over the Eastern North Atlantic

Fabio D'AndreaORCID; Jean‐Philippe Duvel; Gwendal Rivière; Robert VautardORCID; Christophe Cassou; Julien CattiauxORCID; Dim CoumouORCID; Davide Faranda; Tamara HappéORCID; Aglaé Jézéquel; Aurelien RibesORCID; Pascal YiouORCID

<jats:title>Abstract</jats:title><jats:p>Mid‐tropospheric deep depressions in summer over the North Atlantic are shown to have strongly increased in the eastern and strongly decreased in the western North Atlantic region. This evolution is linked to a change in baroclinicity in the west of the North Atlantic ocean and over the North American coast, likely due to the increased surface temperature there. Deep depressions in the Eastern North Atlantic are linked to a temperature pattern typical of extreme heat events in the region. The same analysis is applied to a sample of CMIP6 model outputs, and no such trends are found. This study suggests a link between the observed increase of summer extreme heat events in the region and the increase of the number of Atlantic depressions. The failure of CMIP6 models to reproduce these events can consequently also reside in an incorrect reproduction of this specific feature of midlatitude atmospheric dynamics.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Resonant Plasma Acceleration at Jupiter Driven by Satellite‐Magnetosphere Interactions

Y. SarkangoORCID; J. R. SzalayORCID; A. H. SulaimanORCID; P. A. DamianoORCID; D. J. McComasORCID; J. RabiaORCID; P. A. DelamereORCID; J. SaurORCID; G. ClarkORCID; R. W. EbertORCID; F. AllegriniORCID

<jats:title>Abstract</jats:title><jats:p>The Juno spacecraft had previously observed intense high frequency wave emission, broadband electron and energetic proton energy distributions within magnetic flux tubes connected to Io, Europa, Ganymede, and their wakes. In this work, we report consistent enhancements in &lt;46 keV energy proton fluxes during these satellite flux tube transit intervals. We find enhanced fluxes at discrete energies linearly separated in velocity for proton distributions within Io wake flux tubes, and both proton and electron distributions within Europa and Ganymede wake flux tubes. We propose these discrete enhancements to be a result of resonances between particles' bounce motion with standing Alfvén waves generated by the satellite‐magnetosphere interaction. We corroborate this hypothesis by comparing the bounce and field‐line resonance periods expected at the satellites' orbits. Hence, we find bounce‐resonant acceleration is a fundamental process that can accelerate particles in Jupiter's inner magnetosphere and other astrophysical plasmas.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Thermal Conductivity of MgSiO3‐H2O System Determined by Machine Learning Potentials

Yihang PengORCID; Jie DengORCID

<jats:title>Abstract</jats:title><jats:p>Thermal conductivity plays a pivotal role in understanding the dynamics and evolution of Earth's interior. The Earth's lower mantle is dominated by MgSiO<jats:sub>3</jats:sub> polymorphs which may incorporate trace amounts of water. However, the thermal conductivity of MgSiO<jats:sub>3</jats:sub>‐H<jats:sub>2</jats:sub>O binary system remains poorly understood. Here, we calculate the thermal conductivity of water‐free and water‐bearing bridgmanite, post‐perovskite, and MgSiO<jats:sub>3</jats:sub> melt, using a combination of Green‐Kubo method with molecular dynamics simulations based on a machine learning potential of ab initio quality. The thermal conductivities of water‐free bridgmanite and post‐perovskite overall agree well with previous theoretical and experimental studies. The presence of water mildly reduces the thermal conductivity of the host minerals, significantly weakens the temperature dependence of the thermal conductivity, and reduces the thermal anisotropy of post‐perovskite. Overall, water reduces the thermal conductivity difference between bridgmanite and post‐perovskite, and thus may attenuate lateral heterogeneities of the core‐mantle boundary heat flux.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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The Impact of Rotation on Tropical Climate, the Hydrologic Cycle, and Climate Sensitivity

Levi G. SilversORCID; Alyssa M. StansfieldORCID; Kevin A. ReedORCID

<jats:title>Abstract</jats:title><jats:p>This work explores the impact of rotation on tropical convection and climate. As our starting point, we use the RCEMIP experiments as control simulations and run additional simulations with rotation. Compared to radiative convective equilibrium (RCE) experiments, rotating RCE (RRCE) experiments have a more stable and humid atmosphere with higher precipitation rates. The intensity of the overturning circulation decreases, water vapor is cycled through the troposphere at a slower rate, the subsidence fraction decreases, and the climate sensitivity increases. Several of these changes can be attributed to an increased flux of latent and sensible heat that results from an increase of near‐surface wind speed with rotation shortly after model initialization. The increased climate sensitivity results from changes of both the longwave cloud radiative effect and the longwave clear‐sky radiative fluxes. This work demonstrates the sensitivity of atmospheric humidity and surface fluxes of moisture and temperature to rotation.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Geophysical Responses to an Environmentally‐Boosted Volcanic Unrest

L. De SienaORCID; A. AmorusoORCID; S. PetrosinoORCID; L. CrescentiniORCID

<jats:title>Abstract</jats:title><jats:p>The spatiotemporal relationship between geophysical, environmental, and geochemical responses during volcanic unrest is essentially unknown, making their joint use and interpretation for eruption forecasting challenging. Here, Empirical Orthogonal Functions analysis applied to GPS data allows the separation of the dominant deep‐sourced inflation from environmentally controlled signals associated with extension at Campi Flegrei caldera. This separation bridges the gap between deformation, seismic and geochemical responses, clarifying the processes underlying the ongoing volcanic unrest. Persistent meteoric forcing during the 2017–2018 hydrological year changed the decadal trend of seismic energy and secondary deformation components, pairing their spatial patterns. The result was a block in the carbon dioxide released in 2018 at Solfatara, the primary stress‐release valve at the caldera. The subsequent overpressure weakened the fractured eastern caldera, opening pathways for deep, hot materials to reach the surface. Our results give insight into how environmental forcing can favor volcanic unrest in pressurized calderas.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Spring Irrigation Reduces the Frequency and Intensity of Summer Extreme Heat Events in the North China Plain

Guoshuai Liu; Weiguang WangORCID; Hui Xu

<jats:title>Abstract</jats:title><jats:p>Irrigation has distinct impacts on extreme temperatures. Due to the carryover effect of soil moisture into other seasons, temperature impacts of irrigation are not limited to irrigated seasons. Focusing on the North China Plain, where irrigation occurs in both spring (March‐April‐May) and summer (June‐July‐August), with a higher proportion of irrigation water applied during spring, we investigate the impact of spring irrigation on summer extreme heat events. Based on partial correlation analysis of data products, we find positive correlations between spring and summer soil moisture, suggesting that spring irrigation‐induced water surplus persists into the following summer and affects regional climate by impacting surface energy partitioning. Regional climate simulations confirm cross‐seasonal climatic effects and show that spring irrigation reduces the frequency and intensity of summer extreme heat events by approximately −2.5 days and −0.29°C, respectively. Our results highlight the importance of the cross‐seasonal climatic effect of irrigation in mitigating climate extremes.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Day‐To‐Day Variability of the Neutral Wind Dynamo Observed by ICON: First Results From Conjugate Observations

Brian J. HardingORCID; Thomas J. ImmelORCID; Stephen B. MendeORCID; Yen‐Jung J. WuORCID; Astrid MauteORCID; Scott L. EnglandORCID; Roderick A. HeelisORCID; Jeffrey M. ForbesORCID; Christoph R. EnglertORCID; Kenneth D. MarrORCID; John M. HarlanderORCID; Jonathan J. MakelaORCID; Sabine Frey

<jats:title>Abstract</jats:title><jats:p>First results are presented from the conjugate maneuvers performed by NASA's Ionospheric Connection Explorer (ICON) spacecraft. During each several‐minute maneuver, ICON crosses the magnetic equator, measuring the plasma drift at the ∼600‐km apex of a magnetic field line and the neutral wind profiles (∼90–300 km altitude) along both ends of that field line. The analysis utilizes 149 pairs of maneuvers separated by ∼24 hr but at nearly the same location and local time. Principal component regression reveals that 39 ± 7% and 24 ± 9% of the day‐to‐day variance in the daytime vertical and zonal drift, respectively, is attributable to conjugate neutral winds. The remaining variance is likely driven by external potentials from non‐conjugate winds and geomagnetic activity (median <jats:italic>Kp</jats:italic> 2−). Zonal winds at 100–113 km and &gt;120 km altitude are the primary drivers of conjugate vertical and zonal drift variance, respectively. These observations can test vertical‐coupling mechanisms in whole‐atmosphere models.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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Influence of Subsurface Critical Zone Structure on Hydrological Partitioning in Mountainous Headwater Catchments

Hang ChenORCID; Qifei NiuORCID; James P. McNamaraORCID; Alejandro N. FloresORCID

<jats:title>Abstract</jats:title><jats:p>Headwater catchments play a vital role in regional water supply and ecohydrology, and a quantitative understanding of the hydrological partitioning in these catchments is critically needed, particularly under a changing climate. Recent studies have highlighted the importance of subsurface critical zone (CZ) structure in modulating the partitioning of precipitation in mountainous catchments; however, few existing studies have explicitly taken into account the 3D subsurface CZ structure. In this study, we designed realistic synthetic catchment models based on seismic velocity‐estimated 3D subsurface CZ structures. Integrated hydrologic modeling is then used to study the effects of the shape of the weathered bedrock and the associated storage capacity on various hydrologic fluxes and storages in mountainous headwater catchments. Numerical results show that the weathered bedrock affects not only the magnitude but also the peak time of both streamflow and subsurface dynamic storage.</jats:p>

Palabras clave: General Earth and Planetary Sciences; Geophysics.

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