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Distinct Energy Budgets of Mars and Earth
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-12-19 DOI: 10.1029/2024AV001389
Larry Guan, Liming Li, Ellen C. Creecy, Xun Jiang, Xinyue Wang, Germán Martínez, Anthony D. Toigo, Mark I. Richardson, Agustín Sánchez-Lavega, Yeon Joo Lee

The radiant energy budget (REB) is a fundamental physical parameter for planetary bodies, though studies constraining the REB for bodies beyond Earth are relatively limited. We generate the first meridional profiles of Mars' REB at seasonal and annual timescales through measurements based on long term multi-instrument observations from spacecraft orbiting Mars. Then, we compare our findings to Earth's REB using contemporary satellite data sets. Each planet exhibits remarkably distinct seasonal REB distributions due to differences in their orbital, atmospheric, and surface properties. Annually, Earth's REB exhibits a tropical energy surplus and a deficit at the poles. In contrast, Mars' annual REB displays an inverted meridional distribution with significant hemispheric asymmetry. Additionally, global dust storms significantly modify the Martian REB. Our observations are employable in future studies to improve models on Mars' general circulation, meteorology, and polar ice cap evolution.

辐射能量预算(REB)是行星天体的一个基本物理参数,但对地球以外天体的辐射能量预算进行约束的研究相对有限。我们根据绕火星轨道运行的航天器的长期多仪器观测数据,首次生成了火星辐射能量预算在季节和年度时间尺度上的子午剖面图。然后,我们利用当代卫星数据集将我们的发现与地球的 REB 进行比较。由于轨道、大气和地表特性的不同,每颗行星都表现出明显不同的季节性可变资本分布。每年,地球的 REB 在热带表现出能量过剩,而在两极则表现出能量不足。与此相反,火星的年度 REB 呈倒经向分布,具有显著的半球不对称性。此外,全球沙尘暴极大地改变了火星的 REB。我们的观测结果可用于未来的研究,以改进火星的大气环流、气象学和极地冰盖演变模型。
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引用次数: 0
Effects of Mesoscale Eddies on Southern Ocean Biogeochemistry
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-30 DOI: 10.1029/2024AV001355
Lydia Keppler, Yassir A. Eddebbar, Sarah T. Gille, Nicola Guisewhite, Matthew R. Mazloff, Veronica Tamsitt, Ariane Verdy, Lynne D. Talley
<p>The Southern Ocean is rich in highly dynamic mesoscale eddies and substantially modulates global biogeochemical cycles. However, the overall surface and subsurface effects of eddies on the Southern Ocean biogeochemistry have not been quantified observationally at a large scale. Here, we co-locate eddies, identified in the Meta3.2DT satellite altimeter-based product, with biogeochemical Argo floats to determine the effects of eddies on the dissolved inorganic carbon (DIC), nitrate, and dissolved oxygen concentrations in the upper 1,500 m of the ice-free Southern Ocean, as well as the eddy effects on the carbon fluxes in this region. DIC and nitrate concentrations are lower in anticyclonic eddies (AEs) and increased in cyclonic eddies (CEs), while dissolved oxygen anomalies switch signs above (CEs: positive, AEs: negative) and below the mixed layer (CEs: negative, AEs: positive). We attribute these anomalies primarily to eddy pumping (isopycnal heave), as well as eddy trapping for oxygen. Maximum anomalies in all tracers occur at greater depths in the subduction zone north of the Antarctic Circumpolar Current (ACC) compared to the upwelling region in the ACC, reflecting differences in background vertical structures. Eddy effects on air–sea <span></span><math> <semantics> <mrow> <msub> <mtext>CO</mtext> <mn>2</mn> </msub> </mrow> <annotation> ${text{CO}}_{2}$</annotation> </semantics></math> exchange have significant seasonal variability, with additional outgassing in CEs in fall (physical process) and additional oceanic uptake in AEs and CEs in spring (biological and physical process). Integrated over the Southern Ocean, AEs contribute <span></span><math> <semantics> <mrow> <mo>∼</mo> <mn>0.03</mn> <mo>±</mo> </mrow> <annotation> ${sim} 0.03pm $</annotation> </semantics></math> 0.01 Pg C <span></span><math> <semantics> <mrow> <msup> <mtext>yr</mtext> <mrow> <mo>−</mo> <mn>1</mn> </mrow> </msup> </mrow> <annotation> ${text{yr}}^{-1}$</annotation> </semantics></math> (7 <span></span><math> <semantics> <mrow> <mo>±</mo> <mn>2</mn> <mi>%</mi> </mrow> <annotation> $pm 2%$</annotation> </semantics></math>) to the Southern Ocean carbon uptake, and CEs offset this by <span></span><math> <semantics> <mrow>
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引用次数: 0
The Petrology and Geochemistry of the 2021 Fagradalsfjall Eruption, Iceland: An Eruption Sourced From Multiple, Compositionally Diverse, Near-Moho Sills 冰岛 2021 年 Fagradalsfjall 火山喷发的岩石学和地球化学:源自多个成分多样的近莫霍山的喷发
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-27 DOI: 10.1029/2024AV001310
E. W. Marshall, A. Caracciolo, E. Bali, S. A. Halldórsson, S. Matthews, E. Ranta, M. B. Rasmussen, J. G. Robin, G. H. Guðfinnson, J. Maclennan, C. Bosq, D. Auclair, O. Sigmarsson, H. Merrill, B. Gísladóttir, S. Johnson, N. Löw, A. Stracke, F. Genske

Magmatic processes at the crust-mantle boundary (i.e., Moho) are commonly studied post facto at fossil ophiolites, oceanic core complexes, or inferred from the compositions of crystals or melt inclusions. The 2021 eruption at Fagradalsfjall on the Reykjanes Peninsula, Iceland, was supplied from magma bodies near the Moho and offers a unique opportunity to study the timescales, structure, and syn-eruptive processes of near-Moho magmatic systems at ∼15 km depth. Here, we present a comprehensive petrological and geochemical investigation of the full 183 day eruption that is based on frequent sampling of the eruption. Lavas erupted in the first 45 days displayed significant and sudden changes in geochemistry, followed by lower amplitude fluctuations until the end of the eruption. This variability can be explained by contribution from multiple magma bodies, as best distinguished using Sr-Nd-Hf-Pb isotope systematics. The lavas display unusual trace element and radiogenic isotope compositions compared to other Icelandic basalts, but are similar to other rare, highly incompatible element enriched lavas on the Reykjanes Peninsula, and thus these lavas may represent a distinct suite of Reykjanes Peninsula basalts. Our geochemical and petrological observations show that numerous, compositionally variable bodies of magma must exist in the lowermost crust or at the crust-mantle boundary. These near-Moho magma bodies transfer magma between one another on timescales as short as days-to-months, but partially crystallize over longer time periods, and periodically inject into the overlying crust.

地壳-地幔边界(即莫霍面)的岩浆过程通常是在化石蛇绿岩、大洋核心复合体中进行事后研究,或根据晶体或熔融包裹体的成分进行推断。冰岛雷克雅未克半岛的法格拉德尔斯菲亚尔(Fagradalsfjall)在2021年的喷发是由莫霍面附近的岩浆体提供的,这为研究深度在15千米左右的近莫霍面岩浆系统的时间尺度、结构和同步喷发过程提供了一个独特的机会。在此,我们基于对整个183天喷发过程的频繁取样,对整个喷发过程进行了全面的岩石学和地球化学研究。前45天喷发的熔岩在地球化学方面显示出显著的突变,随后是较小振幅的波动,直到喷发结束。这种变化可以用来自多个岩浆体的贡献来解释,使用 Sr-Nd-Hf-Pb 同位素系统学对其进行了最佳区分。与冰岛其他玄武岩相比,这些熔岩显示出不寻常的微量元素和放射性同位素组成,但与雷克雅未克半岛上其他稀有的、不相容元素高度富集的熔岩相似,因此这些熔岩可能代表了雷克雅未克半岛玄武岩的一个独特组合。我们的地球化学和岩石学观察结果表明,在最下层地壳或地壳-地幔边界一定存在大量成分可变的岩浆体。这些近莫霍区的岩浆体在短至数天至数月的时间内相互转移岩浆,但在较长的时间内部分结晶,并定期注入上覆地壳。
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引用次数: 0
Imaging Magma Reservoirs From Space With Altimetry-Derived Gravity Data 利用测高仪得出的重力数据从太空成像岩浆储层
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-26 DOI: 10.1029/2024AV001403
Hélène Le Mével

I investigate the detectability of magma reservoirs in the vertical gravity gradient (VGG) anomalies calculated from satellite altimetry data. First, I calculate a suite of synthetic seamount models to show the expected VGG anomaly characteristic wavelength and amplitude for a simplified magmatic system, hydrothermal system, and a caldera infill, varying their dimensions for a given depth and density contrast. I find that most magmatic and hydrothermal systems create VGG anomalies with a characteristic wavelength and amplitude greater than the data uncertainty and are therefore detectable. The proposed approach consists in three main steps: (a) calculate the VGG from the two components of the deflection of the vertical, (b) calculate and remove the gravity contribution of the bathymetry interface using an independent bathymetry data set (e.g., acquired by multibeam echosounders) to obtain a VGG Bouguer gravity anomaly, (c) invert the Bouguer VGG anomaly to obtain a 3D density model. I image a 6-by-8-km low density body between 3 and 9 km depth under Brothers volcano in the Kermadec arc. I hypothesize that it represents the main magmatic system, possibly with a minor fraction of hydrothermal fluids at the shallower depths. There are about 225 submarine volcanoes globally that could be studied with satellite altimetry-derived gravity data to potentially image their magmatic system. Future altimetry data will increase the gravity data resolution and allow us to image smaller features. This is thus an invaluable data set for the study of underexplored submarine volcanoes and can help improve our volcano hazards assessment.

我研究了卫星测高数据计算出的垂直重力梯度(VGG)异常中岩浆储层的可探测性。首先,我计算了一套合成海山模型,以显示简化岩浆系统、热液系统和破火山口填充物的预期 VGG 异常特征波长和振幅,并在给定深度和密度对比下改变它们的尺寸。我发现大多数岩浆和热液系统产生的 VGG 异常的特征波长和振幅都大于数据的不确定性,因此是可以探测到的。建议的方法包括三个主要步骤:(a) 利用垂直偏转的两个分量计算 VGG,(b) 利用独立的水深测量数据集(如多波束回声测深仪获取的数据)计算并去除水深测量界面的重力贡献,以获得 VGG 布盖尔重力异常,(c) 反演布盖尔 VGG 异常,以获得三维密度模型。我在凯尔马代克弧的兄弟火山下 3 至 9 千米深处拍摄到一个 6×8 千米的低密度体。我假设它代表了主要的岩浆系统,在较浅的深度可能还有一小部分热液。全球约有 225 座海底火山,可以利用卫星测高衍生重力数据对其进行研究,从而可能对其岩浆系统进行成像。未来的测高数据将提高重力数据的分辨率,使我们能够对较小的地貌进行成像。因此,这是研究未充分开发的海底火山的宝贵数据集,有助于改进我们的火山灾害评估。
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引用次数: 0
Magnetospheric Control of Ionospheric TEC Perturbations via Whistler-Mode and ULF Waves 磁层通过惠斯勒模式和超短波控制电离层 TEC 扰动
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-25 DOI: 10.1029/2024AV001302
Yangyang Shen, Olga P. Verkhoglyadova, Anton Artemyev, Michael D. Hartinger, Vassilis Angelopoulos, Xueling Shi, Ying Zou
<p>The weakly ionized plasma in the Earth's ionosphere is controlled by a complex interplay between solar and magnetospheric inputs from above, atmospheric processes from below, and plasma electrodynamics from within. This interaction results in ionosphere structuring and variability that pose major challenges for accurate ionosphere prediction for global navigation satellite system (GNSS) related applications and space weather research. The ionospheric structuring and variability are often probed using the total electron content (TEC) and its relative perturbations (dTEC). Among dTEC variations observed at high latitudes, a unique modulation pattern has been linked to magnetospheric ultra-low-frequency (ULF) waves, yet its underlying mechanisms remain unclear. Here using magnetically conjugate observations from the THEMIS spacecraft and a ground-based GPS receiver at Fairbanks, Alaska, we provide direct evidence that these dTEC modulations are driven by magnetospheric electron precipitation induced by ULF-modulated whistler-mode waves. We observed peak-to-peak dTEC amplitudes reaching <span></span><math> <semantics> <mrow> <mo>∼</mo> </mrow> <annotation> ${sim} $</annotation> </semantics></math> 0.5 TECU (1 TECU is equal to <span></span><math> <semantics> <mrow> <msup> <mn>10</mn> <mn>6</mn> </msup> </mrow> <annotation> ${10}^{6}$</annotation> </semantics></math> electrons/<span></span><math> <semantics> <mrow> <msup> <mi>m</mi> <mn>2</mn> </msup> </mrow> <annotation> ${mathrm{m}}^{2}$</annotation> </semantics></math>) with modulations spanning scales of <span></span><math> <semantics> <mrow> <mo>∼</mo> </mrow> <annotation> ${sim} $</annotation> </semantics></math> 5–100 km. The cross-correlation between our modeled and observed dTEC reached <span></span><math> <semantics> <mrow> <mo>∼</mo> </mrow> <annotation> ${sim} $</annotation> </semantics></math> 0.8 during the conjugacy period but decreased outside of it. The spectra of whistler-mode waves and dTEC also matched closely at ULF frequencies during the conjugacy period but diverged outside of it. Our findings elucidate the high-latitude dTEC generation from magnetospheric wave-induced precipitation, addressing a significant gap in current physics-based dTEC modeling. Theses results thus improve ionospheric dTEC prediction and enhance our unde
地球电离层中的弱电离等离子体受控于上方太阳和磁层输入、下方大气过程和内部等离子体电动力学之间复杂的相互作用。这种相互作用导致电离层的结构和变化,给全球导航卫星系统(GNSS)相关应用和空间天气研究的准确电离层预测带来了重大挑战。电离层结构和可变性通常利用电子总含量(TEC)及其相对扰动(dTEC)来探测。在高纬度观测到的 dTEC 变化中,有一种独特的调制模式与磁层超低频波有关,但其基本机制仍不清楚。在这里,我们利用 THEMIS 航天器和位于阿拉斯加费尔班克斯的地面 GPS 接收机的磁共轭观测结果,提供了这些 dTEC 调制是由超低频调制的惠斯勒模式波引起的磁层电子沉淀驱动的直接证据。我们观测到的峰-峰 dTEC 振幅达到 ∼ ${sim} $ 0.5 TECU(1 TECU 等于 10 6 ${10}^{6}$ 电子/ m 2 ${mathrm{m}}^{2}$ ),调制尺度为 ∼ ${sim} $ 5-100 km。在共轭周期内,我们模拟的和观测到的dTEC之间的交叉相关性达到了 ∼ ${sim} $ 0.8,但在共轭周期外则有所下降。在共轭期,惠斯勒模式波和dTEC的频谱在超低频也非常吻合,但在共轭期之外却出现了分化。我们的研究结果阐明了由磁层波引起的降水所产生的高纬度 dTEC,解决了目前基于物理学的 dTEC 建模中的一个重要空白。因此,这些结果改进了电离层 dTEC 预测,加深了我们对磁层-电离层通过超低频波耦合的理解。
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引用次数: 0
Earth-Based Transmitters Trigger Precipitation of Inner Radiation Belt Electrons: Unveiling Observations and Modeling Results 地基发射机触发内辐射带电子沉淀:揭开观测和建模结果的神秘面纱
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-21 DOI: 10.1029/2024AV001354
Zheng Xiang, Xinlin Li, Daniel N. Baker, Yang Mei, Declan O'Brien, Benjamin Hogan, Hong Zhao, David Brennan, Binbin Ni, Theodore Sarris, Michael A. Temerin

Human activity influence Earth's environment, including the space environment hundreds to thousands of kilometers above the Earth. One direct evidence is that the 19.8 kHz electromagnetic signals launched by the North West Cape (NWC) transmitter station in Australia produce a wisp-like energy distribution of precipitating energetic electrons in Earth's inner radiation belt, observed by many Low Earth Orbiting satellites. Typically, satellites observe a single wisp with energy that decreases with increasing L (approximately the radial distance in the equatorial plane), which is produced by a first-order cyclotron resonance of transmitter signals with energetic electrons. Here we report, for the first time, multiple wisps observed by the Relativistic Electron and Proton Telescope integrated little experiment-2 (REPTile-2) on board the recently launched Colorado Inner Radiation Belt Experiment (CIRBE) CubeSat. Based on simulation results, we demonstrate that harmonic cyclotron resonances including the 1, −1, and 2 orders by highly oblique NWC transmitter signals produce these multiple wisps. The discovery of multiple-order cyclotron resonances simultaneously occurring in space sheds new light on wave-particle interactions in near-Earth space. It also has implications for developing artificial radiation belt remediation techniques and understanding the propagation and scattering of plasma waves in planetary magnetospheres.

人类活动影响着地球环境,包括地球上空数百至数千公里的空间环境。一个直接证据是,澳大利亚西北角(NWC)发射站发射的 19.8 千赫电磁信号在地球内部辐射带产生了缕状的高能电子沉淀能量分布,许多低地轨道卫星都观测到了这种能量分布。通常情况下,卫星观测到的是一缕能量随 L(约为赤道平面上的径向距离)增大而减小的能量,这是由发射机信号与高能电子的一阶回旋共振产生的。在这里,我们首次报告了最近发射的科罗拉多内辐射带实验(CIRBE)立方体卫星上的相对论电子和质子望远镜集成小实验-2(REPTile-2)观测到的多缕。根据模拟结果,我们证明了高斜度 NWC 发射信号产生的包括 1、-1 和 2 阶在内的谐波回旋共振会产生这些多缕。在太空中同时发生多阶回旋共振的发现,为近地空间的波粒相互作用提供了新的启示。它还对开发人工辐射带补救技术以及了解等离子体波在行星磁层中的传播和散射具有重要意义。
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引用次数: 0
Anthropogenic Aerosols Have Significantly Weakened the Regional Summertime Circulation in the Northern Hemisphere During the Satellite Era 在卫星时代,人为气溶胶显著削弱了北半球的区域夏季环流
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-21 DOI: 10.1029/2024AV001318
Joonsuk M. Kang, Tiffany A. Shaw, Lantao Sun

Reanalysis data show a significant weakening of summertime circulation in the Northern Hemisphere (NH) midlatitudes in the satellite era with implications for surface weather extremes. Recent work showed the weakening is not significantly affected by changes in the Arctic, but did not examine the role of different anthropogenic forcings such as aerosols. Here we use the Detection and Attribution Model Intercomparison Project (DAMIP) simulations to quantify the impact of anthropogenic aerosol and greenhouse gas forcing. The DAMIP simulations show aerosols and greenhouse gases contribute equally to zonal-mean circulation weakening. Regionally, aerosol dominates the Pacific storm track weakening whereas greenhouse gas dominates in the Atlantic. Using a regional energetic framework, we show why the impact of aerosol is the largest in the Pacific. Reduced sulfate aerosol emissions over Eurasia and North America increase (clear-sky) surface shortwave radiation and turbulent fluxes. This enhances land-to-ocean energy contrast and energy transport via stationary circulations to the ocean. Consequently, energy converges poleward of oceanic storm tracks, demanding weaker poleward energy transport storm tracks, and the storm tracks weaken. The impact is larger over the Pacific following the larger emission decrease over Eurasia than North America. Similar yet opposite, increased aerosol emissions over South and East Asia decrease shortwave radiation and weaken land-to-ocean energy transport. This diverges energy equatorward of the Pacific storm track, further weakening it. Our results show aerosols are a dominant driver of regional circulation weakening during the NH summertime in the satellite era and a regional energetic framework explaining the underlying processes.

再分析数据显示,卫星时代北半球中纬度夏季环流明显减弱,对地表极端天气产生了影响。最近的研究表明,这种减弱并没有受到北极变化的显著影响,但没有研究气溶胶等不同人为作用力的作用。在此,我们利用探测和归因模式相互比较项目(DAMIP)模拟来量化人为气溶胶和温室气体强迫的影响。DAMIP 模拟显示,气溶胶和温室气体对带状平均环流减弱的作用相当。从区域来看,气溶胶主导了太平洋风暴道的减弱,而温室气体则主导了大西洋风暴道的减弱。利用区域能量框架,我们说明了为什么气溶胶对太平洋的影响最大。欧亚大陆和北美上空硫酸盐气溶胶排放的减少增加了(晴空)表面短波辐射和湍流通量。这增强了陆地到海洋的能量对比,并通过静止环流向海洋输送能量。因此,能量向海洋风暴轨迹的极地汇聚,要求较弱的极地能量传输风暴轨迹,风暴轨迹减弱。由于欧亚大陆的排放量减少幅度大于北美洲,太平洋地区受到的影响更大。南亚和东亚上空气溶胶排放量的增加减少了短波辐射,削弱了从陆地到海洋的能量传输。这使太平洋风暴轨道的能量向赤道偏移,进一步削弱了风暴轨道。我们的研究结果表明,气溶胶是卫星时代北半球夏季区域环流减弱的主要驱动因素,也是解释基本过程的区域能量框架。
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引用次数: 0
Toward a Universal Model of Hyporheic Exchange and Nutrient Cycling in Streams 建立溪流水下交换和养分循环的通用模型
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-12 DOI: 10.1029/2024AV001373
Ahmed Monofy, Stanley B. Grant, Fulvio Boano, Megan A. Rippy, Jesus D. Gomez-Velez, Sujay S. Kaushal, Erin R. Hotchkiss, Sydney Shelton

In this paper we demonstrate that several ubiquitous hyporheic exchange mechanisms can be represented simply as a one-dimensional diffusion process, where the diffusivity decays exponentially with depth into the streambed. Based on a meta-analysis of 106 previously published laboratory measurements of hyporheic exchange (capturing a range of bed morphologies, hydraulic conditions, streambed properties, and experimental approaches) we find that the reference diffusivity and mixing length-scale are functions of the permeability Reynolds Number and Schmidt Number. These dimensionless numbers, in turn, can be estimated for a particular stream from the median grain size of the streambed and the stream's depth, slope, and temperature. Application of these results to a seminal study of nitrate removal in 72 headwater streams across the United States, reveals: (a) streams draining urban and agricultural landscapes have a diminished capacity for in-stream and in-bed mixing along with smaller subsurface storage zones compared to streams draining reference landscapes; (b) under steady-state conditions nitrate uptake in the streambed is primarily biologically controlled; and (c) median reaction timescales for nitrate removal in the hyporheic zone are ${approx} $0.5 and 20 hr for uptake by assimilation and denitrification, respectively. While further research is needed, the simplicity and extensibility of the framework described here should facilitate cross-disciplinary discussions and inform reach-scale studies of pollutant fate and transport and their scale-up to watersheds and beyond.

在本文中,我们证明了几种无处不在的水汽交换机制可以简单地表示为一维扩散过程,其中扩散率随河床深度呈指数衰减。根据对之前发表的 106 项地下水交换实验室测量结果(涵盖一系列河床形态、水力条件、河床特性和实验方法)的元分析,我们发现参考扩散率和混合长度尺度是渗透性雷诺数和施密特数的函数。反过来,这些无量纲数可以根据河床的中值粒径以及河水的深度、坡度和温度来估算出特定溪流的情况。将这些结果应用于美国 72 条上游溪流的硝酸盐去除的开创性研究显示:(a) 与排水参考景观的溪流相比,排水城市和农业景观的溪流具有较弱的溪流内和河床内混合能力,以及较小的地下储存区;(b) 在稳态条件下,溪流河床的硝酸盐吸收主要受生物控制;(c) 低水文带硝酸盐去除的中位反应时标为 ≈ ${approx} $ 0.同化吸收和反硝化作用的反应时间中值分别为 5 小时和 20 小时。虽然还需要进一步研究,但本文所述框架的简易性和可扩展性应能促进跨学科讨论,并为污染物归宿和迁移及其在流域内外的推广研究提供信息。
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引用次数: 0
Emerging Climate Change Signals in Atmospheric Circulation 大气环流中新出现的气候变化信号
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-11 DOI: 10.1029/2024AV001297
T. A. Shaw, J. M. Arblaster, T. Birner, A. H. Butler, D. I. V. Domeisen, C. I. Garfinkel, H. Garny, K. M. Grise, A. Yu. Karpechko

The circulation response to climate change shapes regional climate and extremes. Over the last decade an increasing number of atmospheric circulation signals have been documented, with some attributed to human activities. The circulation signals represent an exciting opportunity for improving our understanding of dynamical mechanisms, testing our theories and reducing uncertainties. The signals have also presented puzzles that represent an opportunity for better understanding the circulation response to climate change, its contribution to climate extremes, interactions with moisture, and connection to thermodynamic discrepancies. The next decade is likely to be a golden age for dynamics with many advances possible.

环流对气候变化的响应决定了区域气候和极端气候。在过去的十年中,越来越多的大气环流信号被记录下来,其中一些可归因于人类活动。这些环流信号为我们提供了一个令人兴奋的机会,可以提高我们对动力学机制的认识,检验我们的理论并减少不确定性。这些信号也提出了一些难题,使我们有机会更好地了解环流对气候变化的响应、对极端气候的影响、与湿度的相互作用以及与热力学差异的联系。下一个十年很可能是动力学的黄金时代,有可能取得许多进展。
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引用次数: 0
Evidence for Magnetically-Driven Accretion in the Distal Solar System 远太阳系磁驱动吸积的证据
IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-11-06 DOI: 10.1029/2024AV001396
Elias N. Mansbach, Benjamin P. Weiss, Eduardo A. Lima, Michael Sowell, Joseph L. Kirschvink, Roger R. Fu, Saverio Cambioni, Xue-Ning Bai, Jodie B. Ream, Chisato Anai, Atsuko Kobayashi, Hironori Hidaka

Paleomagnetic measurements of meteorites indicate that magnetic fields existed in the inner solar nebula capable of driving accretion at rates similar to those observed for young stellar objects with protoplanetary disks. However, the field strength in the solar system beyond ∼7 astronomical units (AU) and its role in accretion remain poorly constrained. Returned samples from asteroid (162173) Ryugu offer the possibility of determining the nebular field intensity in this distal region. Here, we report paleomagnetic studies of three Ryugu particles which reveal that alteration occurred in the presence of a null or relatively weak (<15.8 μT) field within 3 million years (Ma) after solar system formation. This resolves previously contrasting reports that Ryugu's parent body experienced alteration in the presence of a strong (>80 μT) magnetic field and weak or null field (<3 μT). In addition, we re-examine previous paleomagnetic and Mn-Cr chronometry studies of three other distally-sourced meteorites, Tagish Lake, Tarda, and Wisconsin Range 91600, which measured paleointensities of <0.9, <1.7 and 5.1 ± 4.5 μT respectively. While it was previously unclear whether these records were acquired while the nebula was present, our re-analysis suggests that their records are sufficiently old (i.e., <3.5 Ma after solar system formation) to be nebular in origin. Collectively, these data demonstrate that the distal solar system nebular field, while faint, was likely still strong enough to drive accretion at rates like those observed in the inner solar system.

对陨石进行的古地磁测量表明,太阳星云内部存在磁场,能够以类似于在具有原行星盘的年轻恒星天体中观测到的速度驱动吸积。然而,太阳系中超过 ∼7 天文单位(AU)的磁场强度及其在吸积过程中的作用仍然没有得到很好的证实。从小行星(162173)"龙宫 "返回的样本为确定这一远端区域的星云场强度提供了可能。在这里,我们报告了对三颗龙宫粒子进行的古地磁研究,研究结果表明,在太阳系形成后的300万年(Ma)内,改变是在空场或相对较弱(<15.8 μT)场的存在下发生的。这解决了之前关于龙宫母体在强(80 μT)磁场和弱(3 μT)或空磁场存在时经历蜕变的不同报道。此外,我们还重新审查了以前对其他三块来源较远的陨石(塔吉什湖、塔尔达和威斯康星山脉 91600)进行的古地磁和锰铬年代测定研究,这些陨石测得的古密度分别为 <0.9、 <1.7和 5.1 ± 4.5 μT。虽然以前还不清楚这些记录是否是在星云存在时获得的,但我们的重新分析表明,它们的记录年代足够久远(即太阳系形成后3.5 Ma),足以成为星云记录。总之,这些数据表明,太阳系远端星云场虽然微弱,但很可能仍然足够强大,能够以在内太阳系观测到的速度驱动吸积。
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引用次数: 0
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AGU Advances
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