The Ashima/MIT Mars GCM and argon in the martian atmosphere

We investigate the ability of modern general circulation models (GCMs) to simulate transport in the martian atmosphere using measurements of argon as a proxy for the transport processes. Argon provides the simplest measure of transport as it is a noble gas with no sinks or sources on seasonal timescales. Variations in argon result solely from ‘freeze distillation’, as the atmosphere condenses at the winter poles, and from atmospheric transport. Comparison of all previously published models when rescaled to a common definition of the argon enhancement factor (EF) suggest that models generally do a poor job in predicting the peak enhancement in southern winter over the winter pole – the time when the capability of the model transport approaches are most severely tested. Despite observed peak EF values of ～6, previously published model predictions peaked at EF values of only 2–3. We introduce a new GCM that provides a better treatment of mass conservation within the dynamical core, includes more sophisticated tracer transport approaches, and utilizes a cube–sphere grid structure thus avoiding the grid-point convergence problem at the pole that exists for most current Mars GCMs. We describe this model – the Ashima Research/Massachusetts Institute of Technology Mars General Circulation Model (Ashima/MIT Mars GCM) and use it to demonstrate the significant sensitivity of peak EF to the choices of transport approach for both tracers and heat. We obtain a peak EF of 4.75 which, while over 50% higher than any prior model, remains well short of the observed value. We show that the polar EF value in winter is primarily determined by the competition between two processes: (1) mean meridional import of lower-latitude air not enriched in argon and (2) the leakage of enriched argon out of the polar column by eddies in the lowest atmospheric levels. We suggest possibilities for improving GCM representation of the CO₂ cycle and the general circulation that may further improve the simulation of the argon cycle. We conclude that current GCMs may be insufficient for detailed simulation of transport-sensitive problems like the water cycle and potentially also the dust cycle.     

京津冀一次飑线过程的精细时空演变特征分析

利用常规探空资料、多普勒天气雷达资料和风廓线雷达资料对2013年3月19日夜里到20日凌晨发生在湖南中南部和广东北部的一次区域性雷暴大风天气进行了分析,发现本次强对流天气过程的天气尺度背景是北支高压脊的崩溃和南支槽的建立,槽前出现较强的低空急流和切变线并在湖南中南部和广东北部形成了上干冷下暖湿的温湿配置结构下发生并强烈发展的;地面自动站观测显示北风侵入到前期露点温度较高的贵州黄平地区并形成风向辐合触发了对流,之后对流单体东移进入前期地面辐合线和露点锋相配合,同时500 hPa极为干冷的湖南中部偏南地区不断发展加强成对流带;雷达观测显示19日夜里在湖南西部不断出现对流单体并在其东移南下过程中最终形成飑线结构,该飑线中存在多个超级单体;通过多普勒天气雷达的中气旋产品与雷暴大风出现时间对应比较发现：大多数由中气旋引发的雷暴大风,在雷暴大风出现前2~3个体扫,其中气旋底高不断下降至2 km左右或以下,且在雷暴大风出现前1~2个体扫,中气旋的最强切变高度显著下降至中气旋底高位置附近;通过风廓线雷达数据与雷暴大风出现时间对应比较发现：底层大气折射率结构常数(C2n)大幅度的跃升通常在雷暴大风出现前10~15 min左右出现,其对雷暴大风的出现可能具有一定的指示意义。基于雷达资料快速更新四维变分同化（RR4DVar）分析系统,利用京津冀6部新一代多普勒天气雷达资料和区域（约700个）自动站资料对2013年7月30—31日京津冀地区一次飑线系统在移动过程中系统不同部位的热动力结构及其环境场时空演变特征进行了分析。结果表明,这次飑线过程是在有利的天气尺度背景形势下发生发展的。飑线形成初期,其中段和南段前部有强的暖湿空气辐合上升运动,并受到强的中层垂直风切变的影响,且在飑线中南段两侧水平正负涡度近似平衡,这种环境下,十分有利于飑线中南段的组织发展。而北段前部受弱的中层垂直风切变及辐散下沉运动影响,不利于北段系统有组织的发展;随着飑线移动下山,中段和南段前部在较强的中层垂直风切变控制下,出现强的暖湿空气辐合上升运动,且存在偏南暖湿气流稳定输送到系统上升运动区中,这对飑线系统中段和南段自身对流单体新生及高度组织化极为有利。随着飑线演变为弓形回波,中段环境场仍维持强的中层垂直风切变且位于冷池出流边界的控制之下,由于地形强迫效应,有利于弓形回波前沿低空偏南暖湿气流的辐合上升,是飑线下山迅速增强并发展成弓形回波,且稳定维持的主要原因。     

新生代增温情景下自然火历史的研究

自然火是地球系统的重要组成部分,与气候、植被关系紧密。全球增温情景下,自然火的演化规律和控制因素已经成为学术界的研究热点,通过整理分析自然火实际监测记录、模型模拟结果以及古记录反映的自然火历史,发现还存在一些亟待解决的问题:全球不同增温情景下自然火增多还是减少?其控制因素如何改变?本文选取距今最近的地质历史时期新生代中的典型增温期"中中新世气候适宜期"和"全新世大暖期",对其自然火研究进行分析总结,归纳得出温度是增温情景下自然火的重要控制因素,但是不同地区自然火控制因素有所不同,雨热条件的季节分配、植被类型的演替、雷电和火山活动等因素也对自然火有重要影响。季风区气候变幅大、植被类型丰富,其自然火演化及控制因素具有复杂性,是自然火研究的重要区域,建议在今后研究中,在东亚季风区选择涵盖未来百年可能增温幅度的理想沉积记录,对其记录的自然火历史、增温幅度、植被演替进行系统研究,进而探讨未来增温情景下自然火的演化规律和控制因素。     

Refining the ice flow chronology and subglacial dynamics across the migrating Labrador Divide of the Laurentide Ice Sheet with age constraints on deglaciation

The Laurentide Ice Sheet was characterized by a dynamic polythermal base. However, important data and knowledge gaps have led to contrasting reconstructions in areas such as the Labrador Ice Divide. In this study, detailed fieldwork was conducted at the southeastern edge of a major landform boundary to resolve the relative ice flow chronology and constrain the evolution of the subglacial dynamics, including the migration and collapse of the Labrador Ice Divide. Surficial mapping and analysis of 94 outcrop‐scale ice flow indicators were used to develop a relative ice flow chronology. ¹⁰Be exposure ages were used with optical ages to confine the timing of deglaciation within the study area. Four phases of ice flow were identified. Flow 1 was a northeasterly ice flow preserved under non‐erosive subglacial conditions associated with the development of an ice divide. Flow 2 was a northwest ice flow, which we correlate to the Ungava Bay Ice Stream and led to a westward migration of the ice divide, preserving Flow 2 features and resulting in Flow 3's eastward‐trending indicators. Flow 4 is limited to sparse fine striations within and around the regional uplands. The new optical ages and ¹⁰Be exposure ages add to the regional geochronology dataset, which further constrains the timing of ice margin retreat in the area to around 8.0 ka. Copyright © 2019 The Authors. Journal of Quaternary Science Published by John Wiley & Sons Ltd.     

基于问题探究式学习开展初中跨学科教学的研究——以九年级"小龙虾的'逆袭'"为例

在新一轮课改的指引下,如何将不同学科知识体系融合在真实情境中,引导学生解决具体问题,以培养学生跨学科的学习意识和分析能力,成为教学实践者普遍关心的问题。本文对基于问题探究式的初中跨学科教学的背景、意义与教学模式展开研究,并以九年级“小龙虾的‘逆袭’”为例,进行了基于问题探究式学习的课堂教学设计。     

利用太阳法自动标定L波段探空雷达天线指向

L波段探空雷达方位、仰角的标定通常借助北极星和经纬仪来完成,对其正确性缺乏可靠有效的检验工具,本文利用高精度的太阳位置算法,采用Python语言进行程序设计和封装,根据台站实际经纬度、太阳赤纬角和时差,从理论上计算出太阳实时位置去标定雷达天线指向,并在多个台站进行了测试和偏差分析,其精度为≤0.3°,参考国内新一代天气雷达天线波束指向定标技术指标(≤0.3°),其精度达到相关业务要求。同时,该算法软件还能为探空员日常检查雷达性能,判断雷达有无故障提供更为快捷的手段,确保探空资料的可靠性。     

Python在FY 2G定量业务产品自动可视化中的应用

利用Python语言实现了每日对CMACast下发的最新风云二号G星(FY-2G)云导风(AMV)和射出长波辐射(OLR)两个定量业务产品的实时自动解码和可视化出图,并与国家卫星气象中心下发的卫星天气应用平台(SWAP)的显示进行了对比。结果表明:两者显示一致。在显示所有AMV文件风矢量数据的前提下,本文可视化产品较目前版本SWAP的显示更为疏密均匀,没有出现重叠现象;Python出图自带的高洛德(Gouraud)明暗处理渲染方式则在对OLR格点产品可视化显示中提供了一种更为平滑,细腻的方法。利用本研究方法对风云二号卫星定量产品进行可视化具备自动化和视觉美观的特点,值得在基层气象部门业务中推广。     

Identification of paralytic shellfish toxin-producing microalgae using machine learning and deep learning methods

Journal of Oceanology and Limnology - Paralytic shellfish poisoning (PSP) microalgae, as one of the harmful algal blooms, causes great damage to the offshore fishery, marine culture, and marine...     

太阳高能观测技术

通常将太阳高能观测划分为三个能段,软Ｘ 射线能段（０ ．１ｋｅＶ～１０ｋｅＶ） ,Ｘ 射线及软γ射线能段（０ ．１ ＭｅＶ～１０ ＭｅＶ） ,γ射线能段（１ ＭｅＶ 以上） 。本文就各个能段的探测技术,包括成像系统和探测器,作了全面的调研,重点在新技术的应用。     

岩溶水研究中岩溶裂隙介质的地质力学和数理分析

本文以济南泉域为例,试用地质力学和数理分析方法研究北方岩溶区岩溶水系统中构造场和岩溶场对岩溶裂隙介质渗透场的控制响应关系,模拟岩溶水系统,以查清岩溶水的赋存运移规律。