Do weather fluctuations cause people to seek information about climate change?     

Corey Lang 《Climatic change》2014,125(3-4):291-303

Learning about the causes and consequences of climate change can be an important avenue for supporting mitigation policy and efficient adaptation. This paper uses internet search activity data, a distinctly revealed preference approach, to examine if local weather fluctuations cause people to seek information about climate change. The results suggest that weather fluctuations do have an effect on climate change related search behavior, however not always in ways that are consistent with the projected impacts of climate change. While search activity increases with extreme heat in summer and extended periods of no rainfall and declines in extreme cold in winter, search activity also increases with colder winter and spring average temperatures. Some of the surprising results are magnified when heterogeneity by political ideology and educational attainment in responsiveness is modeled, which could suggest that different people have different perceptions about what types of weather define climate change or that climate science deniers seek information through Google. However, the results also indicate that for all groups in the political and educational spectrum, there exist weather events consistent with the predicted impacts of climate change that elicit increased information seeking.  相似文献   

西藏雄村矿区地面磁测异常特征及其对找矿方向的指示     

郎兴海 《地质与勘探》2014,50(3):411-418

雄村矿区是西藏冈底斯斑岩铜矿带内已查明资源/储量达大型规模的Cu-Au矿区,已经发现了I、Ⅱ、Ⅲ号Cu-Au矿体。矿区地面磁测结果表明,矿区存在明显的高磁异常区和低磁异常区,两类异常区均有矿化显示,I号矿体位于低磁异常区,Ⅱ号矿体位于高磁异常区,磁异常特征的差异主要是因为磁铁矿含量显著不同造成的。通过对矿区地面磁测异常特征的研究,圈定出了2个低磁异常区和3个高磁异常区,综合地、物、化资料,对5个磁异常区今后的找矿思路进行了分析,为矿区及外围开展综合方法找矿提供了参考,同时,对于冈底斯斑岩铜矿带其它地段寻找该类型矿床具有十分重要的意义。  相似文献   

Bayesian modelling the retreat of the Irish Sea Ice Stream     

Richard C. Chiverrell  Ian M. Thrasher  Geoffrey S. P. Thomas  Andreas Lang  James D. Scourse  Katrien J. J. van Landeghem  Danny Mccarroll  Chris D. Clark  Colm Ó Cofaigh  David J. A. Evans  Colin K. Ballantyne 《第四纪科学杂志》2013,28(2):200-209

We present an 8000‐year history spanning 650 km of ice margin retreat for the largest marine‐terminating ice stream draining the former British–Irish Ice Sheet. Bayesian modelling of the geochronological data shows the ISIS expanded 34.0–25.3 ka, accelerating into the Celtic Sea to reach maximum limits 25.3–24.5 ka before a collapse with rapid marginal retreat to the northern Irish Sea Basin (ISB). This retreat was rapid and driven by climatic warming, sea‐level rise, mega‐tidal amplitudes and reactivation of meridional circulation in the North Atlantic. The retreat, though rapid, is uneven, with the stepped retreat pattern possibly a function of the passage of the ice stream between normal and adverse ice bed gradients and changing ice stream geometry. Initially, wide calving margins and adverse slopes encouraged rapid retreat (～550 m a^?1) that slowed (～100 m a^?1) at the topographic constriction and bathymetric high between southern Ireland and Wales before rates increased (～200 m a^?1) across adverse bed slopes and wider and deeper basin configuration in the northern ISB. These data point to the importance of the ice bed slope and lateral extent in predicting the longer‐term (>1000 a) patterns and rates of ice‐marginal retreat during phases of rapid collapse, which has implications for the modelling of projected rapid retreat of present‐day ice streams. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

Whipple telescope observations of LS I +61 303: 2004–2006     

A. Smith  R. W. Atkins  S. Bradbury  O. Celik  Y. C. K. Chow  P. Cogan  C. Dowdall  S. J. Fegan  P. Fortin  D. Gall  G. H. Gillanders  J. Grube  K. J. Gutierrez  T. A. Hall  D. Hanna  J. Holder  D. Horan  S. B. Hughes  T. B. Humensky  I. Jung  P. Kaaret  G. Kenny  M. Kertzman  D. B. Kieda  A. Konopelko  H. Krawczynski  F. Krennrich  M. J. Lang  S. Le Bohec  G. Maier  J. Millis  P. Moriarty  R. A. Ong  J. S. Perkins  K. Ragan  G. H. Sembroski  J. A. Toner  L. Valcarcel  V. V. Vassiliev  R. G. Wagner  S. P. Wakely  T. C. Weekes  R. J. White  D. A. Williams 《Astrophysics and Space Science》2007,309(1-4):299-303

In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set.   相似文献   

Biodegradation and transport of benzene,toluene, and xylenes in a simulated aquifer: comparison of modelled and experimental results     

Jiin‐Shuh Jean  Ching‐Lang Tsai  Shen‐Haw Ju  Chun‐Wen Tsao  Shih‐Ming Wang 《水文研究》2002,16(16):3151-3168

Both laboratory experiments and numerical modelling were conducted to study the biodegradation and transport of benzene–toluene–xylenes (BTX) in a simulated semi‐confined aquifer. The factors incorporated into the numerical model include advection, hydrodynamic dispersion, adsorption, and biodegradation. The various physico‐chemical parameters required by the numerical model were measured experimentally. In the experimental portion of the study, BTX compounds were introduced into the aquifer sand. After the contaminants had been transported through the system, BTX concentrations were measured at 12 equally spaced wells. Subsequently, microorganisms obtained from the activated sludge of a sewage treatment plant and cultured in BTX mixtures were introduced into the aquifer through the 12 sampling wells. The distribution data for BTX adsorption by the aquifer sand form a nonlinear isotherm. The degree of adsorption by the sand varies, depending on the composition of the solute. The degradation time, measured from the time since the bacteria were added to the aquifer until a specific contaminant was no longer detectable, was 35–42 h for BTX. The dissolved oxygen, after degradation by BTX compounds and bacteria, was consumed by about 40–60% in the entire simulated aquifer; thus the aerobic conditions were maintained. This study provides insights for the biodegradation and transport of BTX in aquifers by numerical modelling and laboratory experiments. Experimental and numerical comparisons indicate that the results by Monod degradation kinetics are more accurate than those by the first‐order degradation kinetics. Copyright © 2002 John Wiley & Sons, Ltd.  相似文献   

A North-South Transect across the Central Mexican Volcanic Belt at ~100{degrees}W: Spatial Distribution, Petrological, Geochemical, and Isotopic Characteristics of Quaternary Volcanism     

Blatter  Dawnika L.; Lang Farmer  G.; Carmichael  Ian S. E. 《Journal of Petrology》2007,48(5):901-950

Within the Zitácuaro–Valle de Bravo (ZVB) regionof the central Mexican Volcanic Belt (MVB), three lava serieshave erupted during the Quaternary: (1) high-K₂O basaltic andesitesand andesites; (2) medium-K₂O basaltic andesites, andesitesand dacites; (3) high-TiO₂ basalts and basaltic andesites. Thedominant feature of the first two groups is the lack of plagioclaseaccompanying the various ferromagnesian phenocrysts (olivine,orthopyroxene, augite, and hornblende) in all but the dacites.This absence of plagioclase in the phenocryst assemblages ofthe high-K₂O and medium-K₂O intermediate lavas is significantbecause it indicates high water contents during the stage ofphenocryst equilibration. In contrast, the high-TiO₂ group ischaracterized by phenocrysts of plagioclase and olivine. Thespatial distribution of these three lava series is systematic.The southern section of the ZVB transect, 280–330 km fromthe Middle America Trench (MAT), is characterized by high-K₂Omelts that are relatively enriched in fluid-mobile elementsand have the highest ⁸⁷Sr/⁸⁶Sr ratios. Medium-K₂O basaltic andesiteand andesite lavas are present throughout the transect, butthose closest to the MAT are MgO-rich (3·5–9·4wt %) and have phenocryst assemblages indicative of high magmaticwater contents (3·5–6·5 wt % water) andrelatively low temperatures (950–1000°C). In markedcontrast, the northern section of the ZVB transect (380–480km from the MAT) has high-TiO₂, high field strength element(HFSE)-enriched magmas that have comparatively dry (< 1·5wt % magmatic water) and hot (1100–1200°C) phenocrystequilibration conditions. The central section of the ZVB transect(330–380 km from the MAT) is a transition zone and producesmoderately light rare earth element (LREE) and large ion lithophileelement (LILE)-enriched, medium-K₂O lavas with phenocryst assemblagesindicative of intermediate (1·5–3·5 wt %)water contents and temperatures. The high-K₂O series compositionsare the most enriched in LILE and LREE, with a narrow rangeof radiogenic ⁸⁷Sr/⁸⁶Sr from 0·704245 to 0·704507,¹⁴³Nd/¹⁴⁴Nd values ranging from 0·512857 to 0·512927(_Nd = 4·27–5·63), and ²⁰⁸Pb/²⁰⁴Pb valuesfrom 38·248 to 38·442, ²⁰⁷Pb/²⁰⁴Pb values from15·563 to 15·585, and ²⁰⁶Pb/²⁰⁴Pb values from18·598 to 18·688. The medium-K₂O series compositionsare only moderately enriched in the LILE and LREE, with a broaderrange of ⁸⁷Sr/⁸⁶Sr, but similar ¹⁴³Nd/¹⁴⁴Nd and ²⁰⁸Pb/²⁰⁴Pbvalues to those of the high-K₂O series. In contrast, the high-TiO₂series compositions have little enrichment in LILE or LREE andinstead are enriched in the HFSE and heavy rare earth elements(HREE). The high-TiO₂ lavas are isotopically distinct in theirlower and narrower range of ¹⁴³Nd/¹⁴⁴Nd. The isotopic variationsare believed to reflect the upper mantle magma source regionsas the low content of phenocrysts in most lavas precludes significantupper crustal assimilation or magma mixing, other than thatrepresented by the presence of quartz xenocrysts (< 2 vol.%) with rhyolitic glass inclusions, which are found in manyof these lavas. The systematic spatial variation in compositionof the three lava series is a reflection of the underlying subduction-modifiedmantle and its evolution. KEY WORDS: central Mexico; geochemistry; isotopes; Quaternary volcanism; hydrous lavas  相似文献   

基于颗粒阻尼器的多鼓型古柱抗震性能研究     

周占学  于爽  郭帅  黄晓峥  周小龙 《震灾防御技术》2022,17(2):392-400

为保护地震作用下历史遗迹帕特农神庙多鼓石柱,提出将破损的石鼓替换为填充颗粒的空鼓,以减轻多鼓石柱动力响应。本文基于PFC3D与FLAC3D软件,实现了离散-有限耦合作用,模拟了附有颗粒阻尼器帕特农神庙多鼓型石柱,研究了颗粒阻尼器对帕特农神庙石柱的减震效果,并分析地震强度、频率、阻尼器位置等因素对减震效果的影响。研究结果表明,将颗粒阻尼器替换破损的空鼓,PFC3D与FLAC3D耦合计算结果与试验结果基本一致,减震效果显著,说明耦合分析方法研究颗粒阻尼器抗震性能具有较高的可靠性;地震强度不同时,分层颗粒阻尼器仍可较好地耗散能量;颗粒阻尼器对结构的减震性能受激励频率的影响显著,频率越高,减震效果越好;颗粒阻尼器布置在古柱中上部减震效果优于布置在古柱下部。  相似文献   

Where Is the PFAS? Innovations in PFAS Detection and Characterization     

John Horst  Craig Divine  Joe Quinnan  Johnsie Lang  Erika Carter  Theresa Guillette  Vivek Pulikkal 《Ground Water Monitoring & Remediation》2022,42(1):13-23

  相似文献   

On the origin of the wide HI absorption line towards Sgr A*     

K. S. Dwarakanath  W. M. Goss  J. H. Zhao  C. C. Lang 《Journal of Astrophysics and Astronomy》2004,25(3-4):129-141

We have imaged a region of ∼ 5′ extent surrounding Sgr A* in the HI 21 cm-line absorption using the Very Large Array. A Gaussian decomposition of the optical depth spectra at positions within ∼ 2′ (∼ 5 pc at 8.5 kpc) of Sgr A* detects a wide line underlying the many narrow absorption lines. The wide line has a mean peak optical depth of 0.32 ± 0.12 centered at a mean velocity of V_1sr = −4 ± 15 km s{−1}. The mean full width at half maximum is 119 ± 42 km s⁻¹. Such a wide line is absent in the spectra at positions beyond ∼ 2′ from Sgr A*. The position-velocity diagrams in optical depth reveal that the wide line originates in various components of the circumnuclear disk (radius ∼ 1.3′ ) surrounding Sgr A*. These components contribute to the optical depth of the wide line in different velocity ranges. The position-velocity diagrams do not reveal any diffuse feature which could be attributed to a large number of HI clouds along the line of sight to Sgr A*. Consequently, the wide line has no implications either to a global population of shocked HI clouds in the Galaxy or to the energetics of the interstellar medium as was earlier thought.  相似文献   

电力系统潮流量的微机快速跟踪测量     

王筱珍 《广东海洋大学学报》1995,(2)

提出了一种电力系统潮流量的快速跟踪测量方法，其响应时间只有一个采样时间间隔。实验表明，其准确度可满足实用要求。  相似文献