雪冰电导率反映的南、北极和青藏高原大气环境差异

青藏高原（无论南部、北部）雪冰电导率与雪冰体的酸碱度及雪冰内各类杂质成分的关系明显不同于极地冰盖（南极冰盖与格陵兰冰盖）,青藏高原雪冰电导率依赖于地壳来源的碱性矿物盐类杂质（如Ｃａ２＋,Ｍｇ２＋,ＳＯ２－４等）,因而与雪冰酸度（即Ｈ＋）呈反相关;极地冰盖雪冰电导率依赖于海洋来源的酸根离子（如Ｃｌ－,ＳＯ２－４等）,因而与雪冰酸度呈正相关。但在北极地区,雪冰电导率与各离子的关系存在复杂的地域分异,如在北极中心地区,极可能由于“北极霾”的干扰,打破了格陵兰冰盖内电导率与酸根离子间明确的函数关系。总之,雪冰电导率是寒区大气环境的替代性“指示器”     

基于人机交互方式的海图集一体化分幅

根据海图集制作中分幅设计需要处理的多种情况,提出了海图集一体化分幅方法,采用开放式模块化的方案流程,利用人机交互的方式,使计算数据与矢量数据相结合,结果可以在电脑屏幕上显示出来,使设计者的思想得以充分体现。同时利用批量数据联动处理的方式,提高了图幅设计的效率。     

四川彭州葛仙山巨型冰川漂砾的发现及意义

四川彭州市葛仙山巨型冰川漂砾距四川盆地边缘地带约３～４ｋｍ,规模巨大（约６ｋｍ×２５ｋｍ×０３ｋｍ）,是目前世界上发现的罕见巨型冰川漂砾。现有资料研究结果表明,葛仙山巨型漂砾是早更新世青藏大冰盖冰流的搬运作用所形成的。是青藏大冰盖存在的有力证据之一,也是全球泛大冰盖形成的重要历史见证。同时对众多相关边缘学科的重大基础理论问题的研究,提供了新的思路、途径和方法     

内蒙古东部大陆冰川地貌卫星图像解译

在赤峰境内发现大量冰臼和冰臼群后,利用遥感图像对大兴安岭及其两侧的冰蚀、冰碛地貌类型进行解译发现:它们中的绝大多数原本在巨型冰川漂砾、羊背石或基岩鼓丘上。它们是蒙古大冰盖之一部分在沿东南方向越过大兴安岭时其南端受到黄岗梁、七老图山、大马群山的分流、阻隔、旋转的必然结果。      

Stationary magnetospheric convection on November 24, 1981. 1. A case study of “pressure gradient/minimum-B” auroral arc generation

We present two case studies in the night and evening sides of the auroral oval, based on plasma and field measurements made at low altitudes by the AUREOL-3 satellite, during a long period of stationary magnetospheric convection (SMC) on November 24, 1981. The basic feature of both oval crossings was an evident double oval pattern, including (1) a weak arc-type structure at the equatorial edge of the oval/polar edge of the diffuse auroral band, collocated with an upward field-aligned current (FAC) sheet of ≈1.0 μA m⁻², (2) an intermediate region of weaker precipitation within the oval, (3) a more intense auroral band at the polar oval boundary, and (4) polar diffuse auroral zone near the polar cap boundary. These measurements are compared with the published magnetospheric data during this SMC period, accumulated by Yahnin et al. and Sergeev et al., including a semi-empirical radial magnetic field profile B_Z in the near-Earth neutral sheet, with a minimum at about 10–14 R_E. Such a radial B_Z profile appears to be very similar to that assumed in the “minimum B/cross-tail line current” model by Galperin et al. (GVZ92) as the “root of the arc”, or the arc generic region. This model considers a FAC generator mechanism by Grad-Vasyliunas-Boström-Tverskoy operating in the region of a narrow magnetic field minimum in the near-Earth neutral sheet, together with the concept of ion non-adiabatic scattering in the “wall region”. The generated upward FAC branch of the double sheet current structure feeds the steady auroral arc/inverted-V at the equatorial border of the oval. When the semi-empirical B_Z profile is introduced in the GVZ92 model, a good agreement is found between the modelled current and the measured characteristics of the FACs associated with the equatorial arc. Thus the main predictions of the GVZ92 model concerning the “minimum-B” region are consistent with these data, while some small-scale features are not reproduced. Implications of the GVZ92 model are discussed, particularly concerning the necessary conditions for a substorm onset that were not fulfilled during the SMC period.     

Substorm observations in the early morning sector with Equator-S and Geotail

Data from Equator-S and Geotail are used to study the dynamics of the plasma sheet observed during a substorm with multiple intensifications on 25 April 1998, when both spacecraft were located in the early morning sector (03–04 MLT) at a radial distance of 10–11 R_E. In association with the onset of a poleward expansion of the aurora and the westward electrojet in the premidnight and midnight sector, both satellites in the morning sector observed plasma sheet thinning and changes toward a more tail-like field configuration. During the subsequent poleward expansion in a wider local time sector (20−04 MLT), on the other hand, the magnetic field configuration at both satellites changed into a more dipolar configuration and both satellites encountered again the hot plasma sheet. High-speed plasma flows with velocities of up to 600 km/s and lasting 2–5 min were observed in the plasma sheet and near its boundary during this plasma sheet expansion. These high-speed flows included significant dawn-dusk flows and had a shear structure. They may have been produced by an induced electric field at the local dipolarization region and/or by an enhanced pressure gradient associated with the injection in the midnight plasma sheet.     

冰盖消融的海平面指纹变化及其对GRACE监测结果的影响

全球变暖背景下的冰盖消融以及由此带来海平面上升日益明显,直接影响地球表面的陆地水质量平衡,以及固体地球瞬间弹性响应,研究冰盖质量变化的海平面指纹能够帮助深入了解未来海平面区域变化的驱动因素.本文基于海平面变化方程并考虑负荷自吸效应（SAL）与地球极移反馈的影响,借助美国德克萨斯大学空间研究中心（Center for Space Research,CSR）发布的2003年到2012年十年期间的GRACE重力场月模型数据（RL05）,结合加权高斯平滑的区域核函数,反演得到格陵兰与南极地区冰盖质量变化的时空分布,并利用海平面变化方程计算得到了相对海平面的空间变化,结果表明：格陵兰与南极冰盖质量整体呈明显的消融趋势,变化速率分别为-273.31 Gt/a及-155.56 Gt/a,由此导致整个北极圈相对海平面降低,最高可达约-0.6 cm·a^-1;而南极地区冰盖质量变化趋势分布不一,导致西南极近海相对海平面下降,而东南极地区近海相对海平面上升,最高可达约0.2 cm·a^-1.远离质量负荷区域的全球海平面以上升趋势为主,平均全球相对海平面上升0.71 mm·a^-1,部分远海地区相对海平面上升更加突出（例如北美与澳大利亚）,高出全球平均海平面上升速率将近30%.此外,本文也重点探讨了GRACE监测冰盖消融结果中由于极地近海海平面变化导致的泄漏影响,经此项影响校正后的结果表明：海平面指纹效应对GRACE监测格陵兰与南极地区2003-2012期间整体冰盖消融速率的贡献分别为约3%与9%,建议在后期利用GRACE更精确地估算研究区冰盖质量变化时,应考虑海平面指纹效应的渗透影响.     

地球磁尾等离子体片磁洞的统计分析

本文利用THEMIS卫星的磁场数据和等离子体观测数据,统计分析地球磁尾等离子体片区域线性磁洞的发生率、时空尺度、分布特征、和发生率与地磁AE指数的相关性.分析结果表明磁尾等离子体片区域的磁洞的时间尺度为几秒到几十秒,空间尺度小于当地的质子回旋半径.通过磁洞在空间的位置分布和卫星数据在空间的数据采样分布的对比,我们发现线性磁洞在等离子体片内经常发生,然而在磁尾等离子体片中的发生率要小于太阳风中磁洞的发生率.本文最后统计分析了磁洞发生和AE指数的相关性,结果表明磁洞可能与地磁活动有关系.     

Soil erosion in the Anthropocene: Research needs

Soil erosion is a geomorphological and, at the same time, a land degradation process that may cause environmental and property damage, loss of livelihoods and services as well as social and economic disruption. Erosion not only lowers soil quality on‐site, but causes also significant sediment‐related problems off‐site. Given the large number of research papers on this topic, one might therefore conclude that we know now almost everything about soil erosion and its control so that little new knowledge can be added. This conclusion can be refuted by pointing to some major research gaps. There is a need for more research attention to (1) improved understanding of both natural and anthropogenic soil erosion processes and their interactions, (2) scaling up soil erosion processes and rates in space and time, and (3) innovative techniques and strategies to prevent soil erosion or reduce erosion rates. This is illustrated with various case studies from around the world. If future research addresses these research gaps, we will (1) better understand processes and their interactions operating at a range of spatial and temporal scales, predict their rates as well as their on‐site and off‐site impacts, which is academically spoken rewarding but also crucial for better targeting erosion control measures, and (2) we will be in a better position to select the most appropriate and effective soil erosion control techniques and strategies which are highly necessary for a sustainable use of soils in the Anthropocene. Copyright © 2017 John Wiley & Sons, Ltd.     

One Million Years tephra record at IODP Sites U1436 and U1437: Insights into explosive volcanism from the Japan and Izu arcs

The 1 Myr tephra records of IODP (International Ocean Discovery Program) Holes U1436A and U1437B in the Izu‐Bonin fore‐ and reararc were investigated in order to assess provenance and eruptive volumes, respectively. In total, 304 tephra samples were examined and 260 primary tephra layers were identified. Tephra provenance was determined by means of major and trace element compositions of glass shards and distinguished between Japan and Izu‐Bonin arc origin of the tephra layers. A total of 33 marine tephra compositions were correlated to the Japan arc and 227 to the Izu arc. Twenty marine tephra layers were correlated between the two drilling sites. Additionally, we defined eleven correlations of marine tephra deposits to major widespread Japanese eruptions; from the 1.05 Ma Shishimuta‐Pink Tephra to the 30 ka Aira‐Tn Tephra, both from Kyushu Island. These eruptions provide independent time markers within the sediment record and six correlations were used to date tephra layers from Japan in Hole U1436A to establish an alternative age model for this hole. Furthermore, the minimum distal tephra volumes of all detected events were calculated, which enabled the comparison of the tephra volumes that derived from the Japan and the Izu‐Bonin arcs. For some of the major Japanese eruptions these are the first volume estimations that also include distal deposits. All of the Japanese tephras derived from events with eruption magnitude M_v ≥ 5.6 and three of the investigated eruptions reach magnitudes M_v ≥ 7. Volcanic events of the Izu‐Bonin arc have mostly eruption magnitudes M_v ≤ 5.