999 resultados para Wind-blown dust


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A 35 year chronology from 1965 to 2000 of the deposition of wind-blown sediment is constructed from snowpits for coastal southern Victoria Land, Antarctica. Analysis of local meteorology, contemporary eolian sedimentation, and mineralogy confirm a Victoria Valley provenance, while the presence of volcanic tephra is ascribed to an Erebus volcanic province source. Winter foelm winds associated with anticyclonic circulation are considered responsible for transporting fine-grained sediment from the snow- and ice-free Victoria Valley east toward the coast, while cyclonic storms transport tephra north along the Scott Coast. No trend could be identified in the occurrence of either tephra or wind-blown sediments sourced from the Victoria Valley and retrieved from the snowpits; excavated on the Victoria Lower and Wilson Piedmont Glaciers. We infer this to indicate that the region has not undergone a significant change in weather patterns for at least the last 35 years. Our results also confirm the McMurdo Dry Valleys as a regionally significant source of wind-blown sediment.

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Glyphosate-resistant Echinochloa colona L. (Link) is becoming common in non-irrigated cotton systems. Echinochloa colona is a small seeded species that is not wind-blown and has a relatively short seed bank life. These characteristics make it a potential candidate to attempt to eradicate resistant populations when they are detected. A long term systems experiment was developed to determine the feasibility of attempting to eradicate glyphosate resistant populations in the field. To this point the established Best Management Practice (BMP) strategy of two non-glyphosate actions in crop and fallow have been sufficient to significantly reduce the numbers of plants emerging, and remaining at the end of the season. Additional eradication treatments showed slight improvement on the BMP strategy, however were not significant overall. The effects of additional eradication tactics are expected to be more noticeable as the seed bank gets driven down in subsequent seasons.

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We present a low-complexity algorithm for intrusion detection in the presence of clutter arising from wind-blown vegetation, using Passive Infra-Red (PIR) sensors in a Wireless Sensor Network (WSN). The algorithm is based on a combination of Haar Transform (HT) and Support-Vector-Machine (SVM) based training and was field tested in a network setting comprising of 15-20 sensing nodes. Also contained in this paper is a closed-form expression for the signal generated by an intruder moving at a constant velocity. It is shown how this expression can be exploited to determine the direction of motion information and the velocity of the intruder from the signals of three well-positioned sensors.

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毛乌素沙地是我国十二大沙漠之一,地处北方干旱半干旱区向亚湿润区过渡地带,长期以来,不合理的人类土地利用,结合当地脆弱的环境生态特征,引起了严重的现代荒漠化过程,是我国北方荒漠化研究的重点地区。本文着重从自然和人文学科密切合作的角度,对毛乌素沙地土地利用/土地覆被变化的内在作用机制进行了研究,得到以下主要结论: 1. 利用多年实地观测数据资料,考察了毛乌素沙地四种主要草地类型代表性植物群落地上生物量响应气候因子波动的变化规律,建立了植物地上生物量对气候因子的逐月回归模型,揭示出如下规律:①各种气候因子对不同类型草地以及同一类型不同生长阶段草地都产生不同的影响作用;②同一气候因子在植物不同生长阶段上,对生物量形成的重要性程度存在差异:③在植物生长期内,每个生长阶段的生物量都对后一时期的生物量产生显著影响,说明植物生长的连续性对于生物量的形成和积累是重要的;④在植物的凋枯期,各种气候因子基本上都不对生物量产生显著影响;⑤水分因子对毛乌素沙地几乎各种类型草地的生物量,都是重要的影响因子,毛乌素沙地降水状况在不同年份的显著波动对草地植物地上生物量的影响,不仅直接构成了土地覆被变化的重要组成部分,而且还影响到土地利用的方式、方法和后果。 2. 在考察毛乌素沙地草地地上生物量对气候因子变化的响应规律中,利用逐月动态回归建模方法改进了传统的累积气候因子回归建模方法。逐月回归模型与累积回归模型的比较显示,逐月动态回归模型的优势表现在三个方面:①可以提供累积回归模型无法揭示的作用规律;②模拟更加精确;③可以预测不同气候条件下群落地上生物量的变化范围。 3. 利用风速、降水和潜在蒸发等气象记录资料,建立了毛乌素沙地气候因子影响沙尘暴频率的作用模型,定量地考察了沙地各处气候因子对沙尘暴频率的影响作用。研究表明,气候因素是导致毛乌素沙地沙尘暴发生的主导原因,在沙地各处,气候因子可以解释沙尘暴频率分布格局总信息的比率分别为:乌审召83.6%,乌审旗77.5%,河南82.4%,鄂托克旗79.8%,新街73.1%,伊金霍洛旗82%。 4. 在定量考察气候因素对沙尘暴频率影响作用的基础上,对影响沙尘暴频率格局的自然和人为因素进行了定量分离,研究表明:人为影响因素对对沙尘暴发生起次要作用,解释沙尘暴频率分布格局信息的比率分别为:乌审召16.4%,乌审旗22.5%,河南17.6%,鄂托克旗20.2%,新街26.9%,伊金霍洛旗18%。 自然和人为因素影响作用的定量分离研究表明,毛乌素沙地人为因素的影响作用表现出空间上的差异性:①从方位上说,呈现自东向中、西部递减的梯度:②从地点上说,城镇附近人为影响作用远高于农村地区;③从土地利用方式上说,农垦种植业区域高于畜牧业区域。 5. 在实地观测基础上,建立了裸露沙面和植被覆盖沙面风蚀输沙率模型,定量考察了植被覆盖率与风蚀输沙率之间的关系。研究表明:当植被覆盖率达到60%以上,可以保护地表土壤使风蚀在大多数条件下不致发生;当覆盖率达到40%,可以使风蚀输沙大为减少;而当植被覆盖率低于10%,植被覆盖基本不能对地表土壤起到有效的防护作用。 6. 应用植被覆盖地表风蚀输沙率模型,考察了沙地不同风速条件下植被有效覆盖率。根据当地气象台站的多年气象记录,沙地最大风速在20m/s左右,这样的风速条件下,保证风蚀不致发生的植被有效覆盖率为65%左右;在沙地常见的大风风速14-16m/s下,植被有效覆盖率大致为50-55%;对于沙地一般的中等风速l0-12m/s.植被有效覆盖率为40%。植被覆盖对风蚀的影响作用也可以理解为,植被覆盖使沙粒起动风速发生了增大效应,研究表明:与裸露沙面沙粒起动风速4.5m/s对照,70%植被覆盖率使起动风速改变为15.4m/s;60%植被覆盖率使起动风速改变为12.1m/s;40%植被覆盖率使起动风速改变为8.Om/s;而在10%植被覆盖条件下,起动风速为5.Om/s,改变量很小,说明植被覆盖的保护作用极其有限。 7. 基于野外实地观测,比较了沙地五种常见植物种和二种人工防护材料防风效应上的差异。研究表明,防风效应由高到低的次序是,沙蒿>芨芨草>杨柴和牛心朴子>沙障>栅栏>旱柳;就乔、灌、草和人工材料而言,防风效应的次序是,灌木植被>草本植被>人工材料>乔木植被。植物和人工防护材料降低风速的比率与风速呈现二次函数关系,不同植物种或人工材料,降低风速比率都表现出不同的规律,在一般情况下,降低风速效应随着风速的增大而降低。 8. 通过不同植物种防风效应的比较研究,对毛乌素沙地植被生态建设的实践有一定的指导意义。毛乌素沙地的植被建设中对植被类型和植物种类的选择,应该遵循如下原则:①选取防风固沙效应好的植物种类;②应该考虑植物水分供给与需求的平衡状况,实行适地适树;③植物防护效应应该与当地风蚀气候在时间上较好地匹配,在春季等风蚀严重季节,植被覆盖应该具有较好的防风效应。 9. 在现实中,各种影响风蚀的因素是同时发挥作用的。将风蚀影响因素分解为风速、湿润度和植被覆盖率(以及植被类型)三个方面,在此基础上,建立了风蚀影响因素的综合作用的概念模型和沙丘活动性指数定量模型。湿润程度低、风速高、植被覆盖率低的地区,是风蚀最为严重的地区;在湿润程度高、风速低、植被覆盖率高的地区,是风蚀最弱的地区;在其他地区,风蚀状况根据三个方面因素的综合状况来决定。 10. 利用风蚀影响因子综合作用的沙丘活动性指数模型,从空间、时间、植被类型变化角度,考察了毛乌素沙地的风蚀变化状况。得到如下结论:①随着空间变化,风速、降水等气候因素也随之存在差异,导致沙丘活动性指数的变化规律是,西北部鄂托克旗沙丘活动性最高,乌审旗次之,其他几个站差别不太显著,这是由各地降水、气温、沙粒粒径等因素共同决定;②随着时间的变化,气候、植被生长等方面的状况随之发生改变,导致沙丘活动性发生变化,春季最高,冬季次之,夏秋季最低:③随着沙丘植被覆盖类型的变化,沙丘活动性也发生显著变化,在一般情况下,乔木覆盖沙丘活动性>草本植物覆盖沙丘>灌木覆盖沙丘。 11. 在实地调查土地利用现实状况及其社会、经济和政策影响因素的基础上,建立了我国北方干旱半干旱区土地利用决策机制的概念模型,分析了与土地利用密切相关的农牧民一政府一环境科学家这三个社会群体对土地利用的立场和影响作用力上的差异,分析了毛乌素沙地土地利用的现状及其影响因素,探讨了现实中不可持续土地利用行为发生的社会、经济和政策原因。 12. 在实地调查基础上,分别利用产出一费用分析法和过程影响因素分析法,建立了毛乌素沙地土地利用经济收益的定量模型。产出一分析研究表明,无论是农垦种植业,还是草地畜牧业,农牧民从这两种土地利用方式都只能获得较低下的经济收益。造成这种状况的原因,主要在于两个方面:一是低下且不断处于波动之中的农牧业产品物价,二是沉重的农牧业税收。 13. 将影响农牧业产出的因素,划分为四个方面:土地面积(牲畜头数)、环境状况、管理水平和利用强度,在此基础上建立了定量的影响作用模型。研究表明:环境状况指数每增加0.1,农牧业经济收益增加26%;管理水平因子每提高0.1,农牧业经济收益增加12.7%;农牧业经济收益最优的土地利用强度在0.4左右,在此之前,随着利用强度的增加,经济收益随之增大,而在此之后,随着利用强度的增大,经济收益逐渐降低,当土地利用强度达到0.9左右时,呈现负的经济收益。 14. 毛乌素沙地实施土地资源可持续利用,必须从技术的革新和社会经济政策等因素的调整两条途径同时入手,二者缺一不可。通过改进和应用节水灌溉、风能光能利用、生物增产技术,尽可能地提高各种资源的利用效率;通过应用免耕或浅耕技术,尽量减轻土地利用对资源和环境的破坏;通过栽培、速生技术,提高植被建设的成效和速度。而通过税收、物价政策的调整,尽可能地提高农牧民经济收益增长的速度,减轻土地利用压力;通过政府与人民之间对话和合作机制的建立,让广大农牧民参与到土地利用的决策和管理的过程中去;通过土地利用管理政策、措施的调整和完善,调动农牧民保护资源的积极性和自觉性;通过激励机制的建立,引导农牧民土地利用向着可持续的方向发展。 15. 实现毛乌素沙地土地资源可持续利用的有效途径,在于这样几个方面:①建立和完善政府及其管理部门与人民之间有效的对话和合作机制,让广大农牧民参与到土地利用决策和管理的过程中去:②实行产业结构调整,转变片面追求经济增长的做法,制订适应当地自然条件和生态特征的发展模式;③降低农牧业税收、稳定并提高农牧业产品的物价,增加农牧民经济收入,减轻土地利用压力;④进一步改进和完善土地利用管理政策和法规;⑤建立有效激励机制,引导农牧民土地利用向着可持续的方向发展:⑥努力改进节水灌溉技术、生物增产技术,提高土地利用的科技水平:⑦改进环境保护和植被建设决策的科学性,提高植被建设的成效。

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Particle velocity distribution in a blowing sand cloud is a reflection of saltation movement of many particles. Numerical analysis is performed for particle velocity distribution with a discrete particle model. The probability distributions of resultant particle velocity in the impact-entrainment process, particle horizontal and vertical velocities at different heights and the vertical velocity of ascending particles are analyzed. The probability distributions of resultant impact and lift-off velocities of saltating particles can be expressed by a log-normal function, and that of impact angle comply with an exponential function. The probability distribution of particle horizontal and vertical velocities at different heights shows a typical single-peak pattern. In the lower part of saltation layer, the particle horizontal velocity distribution is positively skewed. Further analysis shows that the probability density function of the vertical velocity of ascending particles is similar to the right-hand part of a normal distribution function, and a general equation is acquired for the probability density function of non-dimensional vertical velocity of ascending particles which is independent of diameter of saltating particles, wind strength and height. These distributions in the present numerical analysis are consistent with reported experimental results. The present investigation is important for understanding the saltation state in wind-blown sand movement. (C) 2009 Elsevier B.V. All rights reserved.

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The transportation and deposition of eolian materials of Chinese loess is correlated and effected by the monsoon from the mid-high latitude. Therefore study of the winter monsoon evolution can help us to understand the dynamic mechanism to climate changes in the east-Asian areas. The anisotropy of magnetic susceptibility (AMS) measurements have been carried out on the samples from the last 250ka wind -blown loess-paleosol sequences at Baicaoyuan and Luochuan. And the main conclusions are following:The magnetic foliation is almost horizontal of the two sections. AMS canthus be represented by an oblate ellipsoid with average K3 perpendicular to thebedding plane and Ki within the bedding plane. It has also shown that the ^-factor isless than 0.5 of the majority of samples. So the two sections are normal magneticfabric for sediments.The degree of anisotropy always shows a strong correlation with the foliationrather than with lineation, therefore the anisotropy is controlled by the foliation.Furthermore the foliation is nearly less than 1.02 and shows the typical wind-blownsediments anisotropy.The intensity of winter monsoon, grain size of the eolian inputs, the foliationand the degree of anisotropy are somewhat inter-related. Generally, the higherintensity of the winter monsoon will carry coarser-grained eolian material, therebyresulting in a larger foliation during deposition. Also the post-depositional compactioncontributes to the anisotropy.The AMS features between loess and paleosol are somewhat different. Wefound that the F, P values of paleosol are lower than that of its parent loess respectively. Moreover, the difference does also exists between the two sections. The anisotropy of Baicaoyuan is more significant than Luochuan section, which maybe related with the location and the intensity of the post-deposition reworks.5. We note that the declination of the long axis is NWW in Baicaoyuan section and the observed NWW direction of the winter monsoon winds based on AMS is consistent with the view that the winter monsoons prevail along the NW-SE direction. But at the Luochuan section, because of the strong affection of the post-deposition reworks, the direction of the long axis is nearly random in the foliation and hardly recognizes the paleowind direction since the last two interglacials.Correlation between the two loess-paleosol sequences implies that it is available in arid or semi-arid areas to take AMS to recognize the paleowind directions on the Loess Plateau.

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We report on new VLT optical spectroscopic and multiwavelength archival observations of SN 1996cr, a previously identified ultraluminous X-ray source known as Circinus galaxy X-2. Our optical spectrum confirms SN 1996cr as a bona fide Type IIn supernova, while archival imaging from the Anglo-Australian Telescope archive isolates the explosion date to between 1995 February 28 and 1996 March 16. SN 1996cr is one of the closest SNe (approximate to 3.8 Mpc) in the last several decades, and in terms of flux ranks among the brightest radio and X-ray SNe ever detected. The wealth of optical, X-ray, and radio observations that exist for this source provide relatively detailed constraints on its postexplosion expansion and progenitor history, including a preliminary angular size constraint from VLBI. Archival X-ray and radio data imply that the progenitor of SN 1996cr evacuated a large cavity just prior to exploding: the blast wave likely spent similar to 1-2 yr in relatively uninhibited expansion before eventually striking the dense circumstellar material which surrounds SN 1996cr. The X-ray and radio emission, which trace the progenitor mass-loss rate, have respectively risen by a factor of greater than or similar to 2 and remained roughly constant over the past 7 years. This behavior is reminiscent of the late rise of SN 1987A, but 1000 times more luminous and much more rapid to onset. SN 1996cr may likewise provide us with a younger example of SN 1978K and SN 1979C, both of which exhibit flat X-ray evolution at late times. Complex oxygen line emission hints at a possible concentric shell or ringlike structure. The discovery of SN 1996cr suggests that a substantial fraction of the closest SNe observed in the last several decades have occurred in wind-blown bubbles, and argues for the phenomena being widespread.

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Concentrated solar power systems are expected to be sited in desert locations where the direct normal irradiation is above 1800 kWh/m2.year. These systems include large solar collector assemblies, which account for a significant share of the investment cost. Solarreflectors are the main components of these solar collector assemblies and dust/sand storms may affect their reflectance properties, either by soiling or by surface abrasion. While soiling can be reverted by cleaning, surface abrasion is a non reversible degradation.The aim of this project was to study the accelerated aging of second surface silvered thickglass solar reflectors under simulated sandstorm conditions and develop a multi-parametric model which relates the specular reflectance loss to dust/sand storm parameters: wind velocity, dust concentration and time of exposure. This project focused on the degradation caused by surface abrasion.Sandstorm conditions were simulated in a prototype environmental test chamber. Material samples (6cm x 6cm) were exposed to Arizona coarse test dust. The dust stream impactedthese material samples at a perpendicular angle. Both wind velocity and dust concentrationwere maintained at a stable level for each accelerated aging test. The total exposure time in the test chamber was limited to 1 hour. Each accelerated aging test was interrupted every 4 minutes to measure the specular reflectance of the material sample after cleaning.The accelerated aging test campaign had to be aborted prematurely due to a contamination of the dust concentration sensor. A robust multi-parametric degradation model could thus not be derived. The experimental data showed that the specular reflectance loss decreasedeither linearly or exponentially with exposure time, so that a degradation rate could be defined as a single modeling parameter. A correlation should be derived to relate this degradation rate to control parameters such as wind velocity and dust/sand concentration.The sandstorm chamber design would have to be updated before performing further accelerated aging test campaigns. The design upgrade should improve both the reliability of the test equipment and the repeatability of accelerated aging tests. An outdoor exposure test campaign should be launched in deserts to learn more about the intensity, frequencyand duration of dust/sand storms. This campaign would also serve to correlate the results of outdoor exposure tests with accelerated exposure tests in order to develop a robust service lifetime prediction model for different types of solar reflector materials.

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We conducted a high-resolution study of a unique Holocene sequence of wind-blown sediments and buried soils in Southern Siberia, far from marine environment influences. This was accomplished in order to assess the difference between North Atlantic marine and in-land climate variations. Relative wind strength was determined by grain size analyses of different stratigraphic units. Petromagnetic measurements were performed to provide a proxy for the relative extent of pedogenesis. An age model for the sections was built using the radiocarbon dating method. The windy periods are associated with the absence of soil formation and relatively low values of frequency dependence of magnetic susceptibility (FD), which appeared to be a valuable quantitative marker of pedogenic activity. These events correspond to colder intervals which registered reduced solar modulation and sun spot number. Events, where wind strength was lower, are characterized by soil formation with high FD values. Spectral analysis of our results demonstrates periodic changes of 1500, 1000 and 500 years of relatively warm and cold intervals during the Holocene of Siberia. We presume that the 1000 and 500 year climatic cycles are driven by increased solar insolation reaching the Earth surface and amplified by other still controversial mechanisms. The 1500 year cycle associated with the North Atlantic circulation appears only in the Late Holocene. Three time periods - 8400-9300 years BP, 3600-5100 years BP, and the last ~250 years BP - correspond to both the highest sun spot number and the most developed soil horizons in the studied sections

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The distribution of pollen in marine sediments is used to reconstruct pathways of terrigenous input to the oceans and provides a record of vegetation change on adjacent continents. The wind transport routes of aeolian pollen is comprehensively illustrated by clusters of trajectories. Isobaric, 4-day backward trajectories are calculated using the modelled wind-field of ECHAM3, and are clustered on a seasonal basis to estimate the main pathways of aeolian particles to sites of marine cores in the south-eastern Atlantic. Trajectories and clusters based on the modelled wind-field of the Last Glacial Maximum hardly differ from those of the present-day. Trajectory clusters show three regional, and two seasonal patterns, determining the pathways of aeolian pollen transport into the south-eastern Atlantic ocean. Mainly, transport out of the continent occurs during austral fall and winter, when easterly and south-easterly winds prevail. South of 25°S, winds blow mostly from the west and southwest, and aeolian terrestrial input is very low. Generally, a good latitudinal correspondence exists between the distribution patterns of pollen in marine surface sediments and the occurrence of the source plants on the adjacent continent. The northern Angola Basin receives pollen and spores from the Congolian and Zambezian forests mainly through river discharge. The Zambezian vegetation zone is the main source area for wind-blown pollen in sediments of the Angola Basin, while the semi-desert and desert areas are the main sources for pollen in sediments of the Walvis Basin and on the Walvis Ridge. A transect of six marine pollen records along the south-western African coast indicates considerable changes in the vegetation of southern Africa between glacial and interglacial periods. Important changes in the vegetation are the decline of forests in equatorial Africa and the north of southern Africa and a northward shift of winter rain vegetation along the western escarpment.

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Parabolic reflectors, also known as parabolic troughs, are widely used in solar thermal power plants. This kind of power plants is usually located on desert climates, where the combined action of wind and dust can be of paramount importance. In some cases it becomes necessary to protect these devices from the joined wind and sand action, which is normally accomplished through solid windbreaks. In this paper the results of a wind tunnel test campaign, of a scale parabolic trough row having different windward windbreaks, are reported. The windbreaks herein considered consist of a solid wall with an upper porous fence. Different geometrical configurations, varying the solid wall height and the separation between the parabolic trough row and the windbreak have been considered. From the measured time series, both the mean and peak values of the aerodynamic loads were determined. As it would be expected, mean aerodynamic drag, as well as peak values, decrease as the distance between the windbreak and the parabolic increases, and after a threshold value, such drag loads increase with the distance.