MIDAS-W: a workstation-based incoherent scatter radar data acquisition system     

J. M. Holt  P. J. Erickson  A. M. Gorczyca  T. Grydeland 《Annales Geophysicae》2000,18(9):1231-1241

The Millstone Hill Incoherent Scatter Data Acquisition System (MIDAS) is based on an abstract model of an incoherent scatter radar. This model is implemented in a hierarchical software system, which serves to isolate hardware and low-level software implementation details from higher levels of the system. Inherent in this is the idea that implementation details can easily be changed in response to technological advances. MIDAS is an evolutionary system, and the MIDAS hardware has, in fact, evolved while the basic software model has remained unchanged. From the earliest days of MIDAS, it was realized that some functions implemented in specialized hardware might eventually be implemented by software in a general-purpose computer. MIDAS-W is the realization of this concept. The core component of MIDAS-W is a Sun Microsystems UltraSparc 10 workstation equipped with an Ultrarad 1280 PCI bus analog to digital (A/D) converter board. In the current implementation, a 2.25 MHz intermediate frequency (IF) is bandpass sampled at 1 s intervals and these samples are multicast over a high-speed Ethernet which serves as a raw data bus. A second workstation receives the samples, converts them to filtered, decimated, complex baseband samples and computes the lag-profile matrix of the decimated samples. Overall performance is approximately ten times better than the previous MIDAS system, which utilizes a custom digital filtering module and array processor based correlator. A major advantage of MIDAS-W is its flexibility. A portable, single-workstation data acquisition system can be implemented by moving the software receiver and correlator programs to the workstation with the A/D converter. When the data samples are multicast, additional data processing systems, for example for raw data recording, can be implemented simply by adding another workstation with suitable software to the high-speed network. Testing of new data processing software is also greatly simplified, because a workstation with the new software can be added to the network without impacting the production system. MIDAS-W has been operated in parallel with the existing MIDAS-1 system to verify that incoherent scatter measurements by the two systems agree. MIDAS-W has also been used in a high-bandwidth mode to collect data on the November, 1999, Leonid meteor shower.  相似文献   

Uncertainties in projected impacts of climate change on European agriculture and terrestrial ecosystems based on scenarios from regional climate models     

J. E. Olesen  T. R. Carter  C. H. Díaz-Ambrona  S. Fronzek  T. Heidmann  T. Hickler  T. Holt  M. I. Minguez  P. Morales  J. P. Palutikof  M. Quemada  M. Ruiz-Ramos  G. H. Rubæk  F. Sau  B. Smith  M. T. Sykes 《Climatic change》2007,81(1):123-143

The uncertainties and sources of variation in projected impacts of climate change on agriculture and terrestrial ecosystems depend not only on the emission scenarios and climate models used for projecting future climates, but also on the impact models used, and the local soil and climatic conditions of the managed or unmanaged ecosystems under study. We addressed these uncertainties by applying different impact models at site, regional and continental scales, and by separating the variation in simulated relative changes in ecosystem performance into the different sources of uncertainty and variation using analyses of variance. The crop and ecosystem models used output from a range of global and regional climate models (GCMs and RCMs) projecting climate change over Europe between 1961–1990 and 2071–2100 under the IPCC SRES scenarios. The projected impacts on productivity of crops and ecosystems included the direct effects of increased CO₂ concentration on photosynthesis. The variation in simulated results attributed to differences between the climate models were, in all cases, smaller than the variation attributed to either emission scenarios or local conditions. The methods used for applying the climate model outputs played a larger role than the choice of the GCM or RCM. The thermal suitability for grain maize cultivation in Europe was estimated to expand by 30–50% across all SRES emissions scenarios. Strong increases in net primary productivity (NPP) (35–54%) were projected in northern European ecosystems as a result of a longer growing season and higher CO₂ concentrations. Changing water balance dominated the projected responses of southern European ecosystems, with NPP declining or increasing only slightly relative to present-day conditions. Both site and continental scale models showed large increases in yield of rain-fed winter wheat for northern Europe, with smaller increases or even decreases in southern Europe. Site-based, regional and continental scale models showed large spatial variations in the response of nitrate leaching from winter wheat cultivation to projected climate change due to strong interactions with soils and climate. The variation in simulated impacts was smaller between scenarios based on RCMs nested within the same GCM than between scenarios based on different GCMs or between emission scenarios.  相似文献   

Thermal diffusivity of olivine     

J.B. Holt 《Earth and Planetary Science Letters》1975,27(3):404-408

The thermal diffusivity of a naturally occurring polycrystalline olivine (Fo₉₁Fa₀₉) was measured by the Flash technique in the temperature range of 450–1500 K. At 450 K the thermal diffusivity was 10.7 × 10^?7 m²/s and decreased as a function of reciprocal temperature to 7.0 × 10^?7 m²/s at 800 K. From that temperature, the values gradually increased to a maximum of 7.8 × 10^?7 m²/s at 1000 K, and then steadily decreased to 5.6 × 10^?7 m²/s at 1500 K. The unusual decrease above 1000 K was caused by a reduction of the previously oxidized samples. The olivine's oxidation state plays a significant role in the value of thermal diffusivity at high temperatures.  相似文献   

Whaling: will the Phoenix rise again?     

Holt SJ 《Marine pollution bulletin》2007,54(8):1081-1086

It is argued that Japan’s authorities and entrepreneurs involved in whaling and the whale-meat trade have a long-term goal of rebuilding a large and profitable industry of pelagic whaling, particularly in the Southern Hemisphere, in the next 20 years or so. They have made large investments in this enterprise since the so-called moratorium on commercial whaling was adopted by the International Whaling Commission in 1982. These include, but are not confined to, state subsidizing of an expanding and diversifying 20-year programme of commercial whaling under provisions in all relevant international agreements since 1937 that permit unlimited and unilaterally decreed whaling, supposedly for scientific purposes, provided that the commodities from the whales killed are fully utilized. The context of this is the monopoly of technical knowledge, special skills and the market for valuable whale-meat that Japanese enterprises acquired in the post-world war II period, having broken - in 1937 - the strongly defended de facto Anglo-Norwegian monopoly of technology, skills, access to Antarctic whaling grounds and the market for whale-oil that had existed until then. The attraction of ‘scientific whaling’ is not only that it by-passes any internationally agreed catch-limits but that it also circumvents all other rules - many dating fr/om the League of Nations whaling convention of 1931 - regarding protected species, closed areas, killing of juveniles, less inhumane killing methods, etc. The groundwork is being laid to justify that resumed whaling on partially recovered whale stocks will be at the unsustainable levels that will be profitable again. This justification is based on spurious assertions that numerous and hungry whales threaten the world’s fisheries, and that the abundance and possible increase in some whale species is impeding the recovery of other, severely depleted, and potentially more valuable species such as the blue whale. If the scenario presented here is correct it has important implications for attempts by the international community either to bring a negotiated end to commercial whaling or to bring all whaling back under international control, as the international law of the sea requires, and to ensure that any permitted exploitation of recovered whale populations will be sustainable, under a precautionary regime.  相似文献   

安徽铜陵凤凰山夕卡岩型铜矿床中辉钼矿Re-Os同位素年龄及其地质意义   总被引：5，自引：2，他引：3  

瞿泓滢  裴荣富  王永磊  李进文 《岩石学报》2010,26(3):785-796

铜陵矿集区是我国长江中下游Cu-Au-Fe-Mo成矿带中最重要的有色金属基地之一,凤凰山矿床是铜陵矿集区的重要组成部分,为一个典型的夕卡岩型铜矿床。本文利用Re-Os同位素定年方法对凤凰山铜矿床进行了成矿时代测定,获得了辉钼矿的Re-Os同位素模式年龄范围为139.1±2.4～142.0±2.2Ma,等时线年龄为141.1±1.4Ma,与矿区内石英二长闪长岩和花岗闪长岩SHRIMP锆石U-Pb年龄(144.2±2.3Ma)相吻合,也与铜陵地区其他矿田的成矿时代基本一致,可能为岩石圈减薄事件的成矿响应。  相似文献   

赣南营前岩体的年代学、地球化学、Sr-Nd-Hf同位素组成及其地质意义   总被引：6，自引：1，他引：5  

郭春丽  毛景文  陈毓川 《岩石学报》2010,26(3):919-937

赣南营前岩体由早期似斑状花岗闪长岩和晚期细粒黑云母花岗岩组成,在前者中普遍发育暗色基性包体。SHRIMP锆石U-Pb测年显示似斑状花岗闪长岩为172.2±3.1Ma,细粒黑云母花岗岩为168±3Ma,包体为167.6±3.3Ma。所有的岩石均为钙碱性系列,稀土元素显示LREE富集,HREE亏损,Eu负异常并不明显的特征,Nb-Ta负异常显示壳源物质的特征。晚期细粒黑云母花岗岩、早期似斑状花岗闪长岩、暗色包体的(87Sr/86Sr)i和εNd(t)值分别为0.70885～0.70965、0.71058～1.46393、0.70788～0.70923和-6.38～-5.31、-6.51～-5.17、-5.47～-4.31;锆石εHf(t)值分别为-12.4～-5.7、-9.2～-4.2、-9.4～+0.1。结合岩相学、地球化学研究,初步认为营前岩体的两期花岗质岩石源于地壳重熔,地幔底侵导致地壳熔融形成营前岩体,基性岩浆加入到未冷却的酸性岩浆中形成了目前所见到的暗色包体。结合区域上的研究资料,认为中侏罗世期间,沿"十杭"断裂带及与其相平行的一些深断裂发生了板块的撕裂,这些缝合带是岩石圈相对薄弱的地带,有利于幔源物质底侵上升以及壳幔相互作用。  相似文献   

新疆阿尔泰克因布拉克铜锌矿床地质特征及成矿作用   总被引：4，自引：1，他引：3  

杨富全  毛景文  刘锋  董永观  柴凤梅  耿新霞 《岩石学报》2010,26(2):361-376

克因布拉克中型铜锌矿床赋存于早二叠世花岗岩外接触带的上志留统-下泥盆统康布铁堡组黑云石英片岩、变质石英砂岩中。矿床的形成经历了夕卡岩期、热液期和表生期,铜锌矿主要形成于热液期。矿石中石英和方解石流体包裹体划分为H_2O-NaCl型和H_2O-CO_2(±CH_4/N_2)-NaCl型。成矿温度变化于146～448℃,在170℃、270℃和350℃出现峰值;流体盐度变化于0.2%～46.9%NaCl_(eq),峰值为1.5%NaCl_(eq)和5.5%NaCl_(eq);流体的密度0.55～1.19g/cm~3。硫化物的δ~(34)S集中变化于-8.4‰～1.9‰,峰值为0‰,表明硫来自岩浆。石英和方解石δD_(SMOW)介于-130‰～-79‰,δ~(18)O_(SMOW)值介于8.0‰～11.6‰,δ~(18)O_(H2O)值为-1.7‰～4.43‰,表明成矿流体主要是岩浆水,混合大气降水。方解石中δ~(13)C_(PDB)变化于-5.3‰～-1.1‰,暗示碳来自花岗质岩浆。成矿时代为早中二叠世,成矿作用与花岗质岩浆期后的热液活动有关。  相似文献   

The co-evolution of the obscured quasar PKS 1549−79 and its host galaxy: evidence for a high accretion rate and warm outflow     

J. Holt  C. Tadhunter  R. Morganti  M. Bellamy  R. M. González Delgado  A. Tzioumis  K. J. Inskip 《Monthly notices of the Royal Astronomical Society》2006,370(4):1633-1650

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Managing fish stocks: The role of international organizations in the Mediterranean Area     

Sidney J. Holt 《Marine Policy》1978,2(2):133-141

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Long term storage of relativistic particles in the solar corona     

George M. Simnett  Stephen S. Holt 《Solar physics》1971,16(1):208-223

A model is presented which shows that large numbers of energetic electrons (0.3-> 10 MeV) and protons (1–30 MeV) can be stored in the solar corona at altitudes around 3 × 10⁵ km for periods in excess of 5 days. Specific reference is made to the time period July 6–16 1968 as an excellent example of energetic solar particle storage. Time histories of interplanetary charged particle intensities observed by the IMP-4 and Pioneer 8 satellites are used to substantiate this contention. Detailed reference is also made to solar X-ray, optical and radio data obtained during the period in question, in addition to interplanetary magnetometer data. This model provides a unique solution to many hitherto unexplained solar particle events, and can also account for the lack of prompt particle emission from certain large solar flares recorded in the past.  相似文献