电测量在中国地震预报中的应用

唐山等大地震地电阻率中期下降系压缩应变积累所致 ,为基线缩短、井水位下降所支持。地电阻率、自然电位对起潮力的异常响应及自然电位快急始、慢衰减特殊图象与废油井喷油同步等短临前兆 ,与中期前兆相反显示出向震中迁移的规律 ,表明能量积累从震中向外围传播 ,而能量释放从外围向震中传播。海城地震时喷砂冒水可引起自然电位垂直分量跃变及地光。IIMT法和过剩海洋电流H极化结果表明 ,唐山地震与地壳高阻层及其中存在深大断裂有     

Provenance of long‐travelled dust determined with ultra‐trace‐element composition: a pilot study with samples from New Zealand glaciers

We report high‐precision inductively coupled plasma mass spectrometric (ICP‐MS) compositional data for 39 trace elements in a variety of dust deposits, trapped sediments and surface samples from New Zealand and Australia. Dusts collected from the surface of alpine glaciers in the Southern Alps, New Zealand, believed to have undergone long‐distance atmospheric transport from Australia, are recognizable on account of their overabundances of Pb and Cu with respect to typical upper crustal values. Long‐travelled dust from Australia therefore scavenges these and other metals (e.g. Zn, Sb and Cd) from the atmosphere during transport and deposition. Hence, due to anthropogenic pollution, long‐travelled Australian dusts can be recognized by elevated metal contents. The relative abundance of 25 other elements that are not affected by atmospheric pollution, mineral sorting (Zr and Hf) and weathering[sol ]solubility (alkali and earth alkali elements) reflects the geochemistry of the dust source sediment. As a result, we are able to establish the provenance of dust using ultra‐trace‐element chemistry at regional scale. Comparison of long‐travelled dust chemistry with potential Australian sources shows that fits of variable quality are obtained. We propose that the best fitting potential source chemistry most likely represents the major dust source area. A binary mixing model is used to demonstrate that admixture of small quantities of local dust provides an even better fitting dust chemistry for the long‐travelled dusts. Copyright © 2005 John Wiley & Sons, Ltd.     

Horseshoe Crab (<Emphasis Type="Italic">Limulus polyphemus</Emphasis>) Movements Following Tagging in the Delaware Inland Bays,USA

The Delaware Bay region is the epicenter of horseshoe crab, Limulus polyphemus, activity, and despite the ecological and commercial importance of this species, few studies have examined the long-term movements of horseshoe crabs in this area and the amount of mixing that takes place between smaller coastal embayments within the region and the Delaware Bay proper, factors that are critical to effective management. To better understand these factors, 5568 crabs were tagged in the Delaware Inland Bays as part of the U.S. Fish and Wildlife Service’s (USFWS) Cooperative Horseshoe Crab Tagging Program in 2002–2016. A high re-sight rate of 20.1% (1123 crabs) was reported to the USFWS. Re-sights suggest that the Delaware Bay population is distributed between coastal New Jersey (south of Barnegat Bay) and coastal Virginia (north of Chincoteague Inlet). There were 90 re-sights in the Inland Bays and 148 re-sights in Delaware Bay, with 320 days or more between tagging and re-sight, showing that substantial interchange between successive spawning seasons occurs. Distance analyses demonstrated that crabs can move between the Inland Bays and other Delaware Bay region waterbodies within a single year. The findings of this study support the current management strategy of splitting the harvest of Delaware Bay crabs between New Jersey, Delaware, Maryland, and Virginia and also demonstrate that the waterbodies within the Delaware Bay region are highly connected. This connectivity supports protecting spawning habitat within the smaller embayments of the Delaware Bay region and including spawning surveys from these systems in future stock assessments.     

Identifying regional dust transport pathways: ­application of kinematic trajectory modelling to a trans‐Tasman case

A kinematic trajectory model is used to investigate potential pathways of dust transport from Australia to New Zealand. Historically, these have been assumed to follow rather direct west–east trajectories spanning 2 to 3 days, often resulting in red snow events in the Southern Alps of New Zealand. However, results from the present study which examined the route taken by air parcels originating in southern Australia during dust storms on 24 and 25 May 1994, indicate that trans‐Tasman dust transport trajectories are more diverse than previously thought, and display considerable variation during single events. These more divergent pathways tie in more closely with aeolian dust sedimentation patterns identified by ocean coring in the Tasman Sea, and may account for the deposition of Australian dust on sub‐Antarctic islands located well south of the Australian continent. Copyright © 2000 John Wiley & Sons, Ltd.     

Observations of dry season surface energy exchanges over a desert clay pan,Queensland, Australia

Clay pans (playas) are common landforms of semi-arid and arid desert regions ranging in size from 1 to 2 km² to greater than 10,000 km². The first observations of surface energy exchanges over a clay pan in central Australia using the eddy covariance method are presented. Measurements were obtained in the late dry season (September) before the onset of the Australian summer monsoon under clear skies and weak synoptic winds for five consecutive days. Sensible heat flux displayed an upward trend over the observation period reaching a peak of approximately 50% of net radiation over the period, while latent heat flux declined as the clay pan became dryer. Ground heat flux was similar in magnitude to sensible heat flux reaching maximum values near noon, approximately 2 h before daily maximum sensible heat flux. Net radiation and ground heat flux both reached minimum values 1–2 h after sunset and then gradually increased towards sunrise, while sensible and latent heat flux remained close to zero. Bowen Ratio values increased from 4.08 to 6.12 over the study period as the surface dried. Results highlight clay pans as significant sources of sensible heat in desert landscapes.     

Visual assessment of the Australian Land Erodibility Model

There is a growing requirement for techniques to assess land susceptibility to wind erosion, i.e. land erodibility, over large geographic areas (>10⁴ km²). This requirement stems from a lack of wind erosion research between the field (10¹ km²) and regional scales, and a need to evaluate the performance of spatially explicit wind erosion models across these scales. This paper addresses this issue by presenting a methodology for monitoring land erodibility at the landscape scale (10³ km²). First, we define criteria suitable for evaluating land erodibility based on empirical relationships between soil texture, vegetation cover, geomorphology, and wind erosion. The criteria were used to visually assess land erodibility over long distances (10³ km) using vehicle-based transects run through the rangelands of western Queensland, Australia. Application of the data for testing the performance of a spatially explicit land erodibility model (AUSLEM) is then demonstrated by comparing the visual assessments of land erodibility with the model output. The model performed best in the west of the study area in the open rangelands. In regions with higher woody shrub and tree cover the model performance decreases. This highlights the need for research to better parameterise controls on erodibility in semi-arid landscapes consisting of forested and rangeland mosaics.     

Changes in carbon and nitrogen cycling in a floodplain lake over recent decades linked to littoral expansion,declining riverine influx,and eutrophication

This study aimed to understand changes in the biogeochemical processing of organic matter (OM) in response to multiple stressors (e.g., littoral area expansion, wastewater input, and hydrological regulation) in East Dongting Lake (Central China) over the past 60 years, using analyses of total organic carbon (TOC), total nitrogen (TN), C/N ratios, δ¹³C, δ¹⁵N, and diatoms from 2 sediment cores collected from the littoral and central parts of the lake. OM mainly originated from phytoplankton and C₃ plant‐derived soil OM based on the ranges of C/N ratios (from 7 to 11) and δ¹³C (between ?27‰ and ?23‰). Littoral area expansion due to siltation caused an increasing influx of terrestrial soil OM in the 1980s and the 1990s, subsequently lowering δ¹³C values and rising C/N ratios in both sediment cores. Meanwhile, higher δ¹⁵N was linked to a high influx of isotopically heavy nitrate from urban and agricultural wastewaters. After 2000, slight decreases in TOC and TN in the littoral area were attributable to reducing inputs of external OM, likely linked to declining sediment influx from the upper reaches resulting from the Three Gorges Dam impoundment. Contrasting increases in TOC, TN, and C/N ratios in the central part indicated a high influx of terrestrial soil OM due to the declining distance from the shoreline with littoral area expansion. Declining δ¹⁵N values after 2000 indicated an increase in N₂‐fixing cyanobacteria with eutrophication. Changes in diatom assemblages in both the littoral and central zones reflected nutrient enrichment and hydrological alterations. These results indicate that littoral expansion, declining riverine influx, and anthropogenic nutrient inputs are potential driving forces for the biogeochemical processing of OM in floodplain lakes. This study provides sedimentary biogeochemical clues for tracking past limnological conditions of floodplain lakes that are subjected to increasing disturbances from hydrological regulation and eutrophication.     

High-mass X-ray binary SXP18.3 undergoes the longest type II outburst ever seen in the Small Magellanic Cloud

On 2006 August 30, SXP18.3 a high-mass X-ray binary (HMXB) in the Small Magellanic Cloud (SMC) with an 18.3 s pulse period was observed by Rossi X-ray Timing Explorer ( RXTE ). The source was seen continuously for the following 36 weeks. This is the longest type II outburst ever seen from a HMXB in the SMC. During the outburst, SXP18.3 was located from serendipitous XMM–Newton observations. The identification of the optical counterpart has allowed SXP18.3 to be classified as a Be/X-ray binary. This paper will report on the analysis of the optical and weekly RXTE X-ray data that span the last 10 yr. The extreme length of this outburst has for the first time enabled us to perform an extensive study of the pulse timing of a SMC Be/X-ray binary. We present a possible full orbital solution from the pulse timing data. An orbital period of 17.79 d is proposed from the analysis of the Optical Gravitational Lensing Experiment (OGLE) III light curve placing SXP18.3 on the boundary of known sources in the Corbet diagram.