Contrasting metamorphic conditions in the Neoproterozoic collision-related Nappes south of São Francisco Craton, SE Brazil     

Maria da Glria Motta Garcia  Mrio da Costa Campos Neto 《Journal of South American Earth Sciences》2003,15(8):853-870

Metamorphic conditions are described for three major tectonic entities on the basis of geothermobarometry in a huge Neoproterozoic nappe complex that verges toward the southern border of the São Francisco craton. The uppermost Socorro-Guaxupé Nappe, represented by its granulite facies basal portion, yields a maximum temperature and pressure of 890 °C and 11 kbar. Its metamorphic evolution is consistent with heating at the base of the crust as a result of an abnormally high geothermal gradient, probably due to underplating by the lithospheric mantle. The underlying Três Pontas-Varginha Nappe yields two somewhat distinct P–T paths, both characterized by peak assemblages in the kyanite stability field. The basal kyanite-bearing granulites show higher peak pressure values (15 kbar at 840 °C) and a trajectory that continues in the kyanite stability field, whereas the upper sillimanite granulites show higher temperatures (880 °C at 13 kbar) and a steeper path toward the sillimanite stability field. Data for the Carmo da Cachoeira nappe reveal a steep trajectory, in which the elevated maximum pressure (18.5 kbar at 820 °C) was obtained from a garnet amphibolite that lies along its basal contact. The inverted metamorphic pattern previously observed across these sequences is confirmed by our thermobarometric data, which reveal that the highest temperatures were attained toward the top of the pile.  相似文献   

The seismological picture of the inner core: structure and rotation     

Annie Souriau  Raphaël Garcia  Georges Poupinet 《Comptes Rendus Geoscience》2003,335(1):51-63

This paper presents a review of recent results concerning the structure and the rotation of the inner core, as inferred from seismological observations. We first focus on the apparent hemispherical pattern of the inner core structure, observed in both the anisotropy and the heterogeneity of the uppermost layers, whereas isotropic velocities seem to be homogeneous in a broad wavelength domain. Then we present results on the radial variations of the attenuation and its possible anisotropy, for which viscoelasticity and wave scattering provide complementary explanations. Linked to these results is a discussion about the detection of the PKJKP phase, which propagates as S-wave inside the inner core. Finally, the seismological observations of a possible inner core rotation are discussed; recent results seem to favour rotation rates below 0.2° yr^?1.  相似文献   

Population Belongs on the Johannesburg Agenda     

Wolfgang Lutz  Mahendra Shah  Richard E. Bilsborrow  John Bon-gaarts  Partha DasGupta  Barbara Entwisle  Günther Fischer  Brigida Garcia  Daniel J. Hogan  Arne Jernelöv  Zhenghua Jiang  Robert W. Kates  Sanjaya Lall  F. Landis MacKellar  P.K. Makinwa-Adebusoye  Anthony J. McMichael  Vinod Mishra  Norman Myers  Nebojsa Nakicenovic  Sten Nilsson  Brian C. O'Neill  Xizhe Peng  Harriet B. Presser  Nafis Sadik  Warren C. Sanderson  Gita Sen  Barbara Torrey  Dirk van de Kaa  Hans J.A. van Ginkel  Brenda Yeoh  Huda Zurayk 《Global Change & Human Health》2002,3(1):33-35

The forthcoming World Summit on Sustainable Development (WSSD) in Johannesburg (August 26-September 4, 2002) has been set by the United Nations to consider strategies toward sustainable development in all its dimensions. Hence, its mandate is broader than that of the Rio 1992 United Nations Conference on Environment and Development (UNCED). Population issues have so far been discussed in a separate series of World Population Conferences (Bucharest 1974, Mexico City 1984, Cairo 1994). With no new World Population Conference scheduled for 2004 and Johannesburg having a mandate that is stated to explicitly include social and economic aspects, population as a key component of sustainable development should figure prominently on the Johannesburg agenda. Yet, after the third of four preparatory meetings for Johannesburg (which ended in New York on April 5th), consideration of population is completely absent. The reasons for this are not entirely clear. We assume that they have to do with the fear of entering into political controversies over abortion. We are concerned that, despite its broader mandate, in most countries inputs to Johannesburg are being prepared mainly by environment ministries who have little experience in dealing with population questions. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Agrometeorological models for forecasting the qualitative attributes of “Valência” oranges     

Victor?Brunini?MoretoEmail author  Glauco?de Souza?Rolim  Bruno?Gustavo?Zacarin  Ana?Paula?Vanin  Leone?Maia?de?Souza  Rodrigo?Rocha?Latado 《Theoretical and Applied Climatology》2017,130(3-4):847-864

Forecasting is the act of predicting unknown future events using available data. Estimating, in contrast, uses data to simulate an actual condition. Brazil is the world’s largest producer of oranges, and the state of São Paulo is the largest producer in Brazil. The “Valência” orange is among the most common cultivars in the state. We analyzed the influence of monthly meteorological variables during the growth cycle of Valência oranges grafted onto “Rangpur” lime rootstocks (VACR) for São Paulo, and developed monthly agrometeorological models for forecasting the qualitative attributes of VACR in mature orchard. For fruits per box for all months, the best accuracy was of 0.84 % and the minimum forecast range of 4 months. For the relation between °brix and juice acidity (RATIO) the best accuracy was of 0.69 % and the minimum forecast range of 5 months. Minimum, mean and maximum air temperatures, and relative evapotranspiration were the most important variables in the models.  相似文献   

Mercury in itabirite-hosted soft hematite ore in the Quadrilátero Ferrífero of Minas Gerais     

Alexandre Raphael Cabral  Orlando Garcia Rocha Filho  Richard David Jones 《Journal of Geochemical Exploration》2008,96(1):69-76

Mercury contents in Precambrian banded iron formation-hosted hematite ores are virtually unknown. In an attempt to provide information on the abundance and distribution of Hg in Fe ore, we present analyses for Hg in samples of high-grade soft hematite ore from Gongo Soco, Minas Gerais, Brazil. Bulk samples contain from <  5 to 25  ppb Hg without obvious correlation with major elements. Granulometric fractions of follow-up samples have amounts of Hg from 6 to 48  ppb and display positive linear correlations with total Mn as MnO (r = 0.87), LOI (r = 0.87) and SiO₂ (r = 0.76), as well as a negative linear correlation with total Fe as Fe₂O₃ (r = −  0.87). The correlations suggest that Hg is associated with a hydrated ferruginous groundmass bearing residual Mn, Al and Si, which replaced gangue minerals in itabirite in the process of formation of the Gongo Soco soft hematite ore.  相似文献   

Identifying Environmental and Human Factors Associated With Tick Bites using Volunteered Reports and Frequent Pattern Mining   总被引：1，自引：0，他引：1       下载免费PDF全文

Irene Garcia‐Martí  Raul Zurita‐Milla  Arno Swart  Kees C. van den Wijngaard  Arnold J.H. van Vliet  Sita Bennema  Margriet Harms 《Transactions in GIS》2017,21(2):277-299

Tick populations and tick‐borne diseases like Lyme borreliosis have been steadily increasing since the mid‐1990s. Realizing the threat that ticks pose to public health, two Dutch citizen science projects have collected tick bite reports since 2006. This unique volunteered geographical dataset, which currently has nearly 35,000 reports, was used to identify environmental and other circumstantial factors associated with tick bites. For this, we first enriched the tick bite reports with temperature, precipitation, vegetation and volunteered data associated with the location of the tick bite. Using this enriched dataset, we then derived a series of features to characterize the environmental and volunteer‐related conditions in which each tick bite occurred. Next, we discretized these features using the Jenks Natural Breaks algorithm and, after that, we mined frequent environmental patterns associated with tick bites using the AprioriClose algorithm. Finally, we checked that these patterns are specifically associated with the tick bites by comparing them with the frequent patterns mined from pseudo‐random locations. The frequent patterns were visualized using heat maps and ring maps and two representative patterns associated with tick bites were projected into geographic space to study their spatio‐temporal distribution. Our results show that factors linked to human activity are more relevant to model tick bites than seasonal accumulations of temperature, vegetation or precipitation. In particular, the number of warm and dry days per season are present in a significant number of patterns and the majority of tick bites are produced within a distance of half a kilometer of a forest, recreational or built‐up area. The study of patterns in the time‐series revealed that there are several persistent patterns consistently occurring each year and the validation process showed that the volunteer tick bites collection is capturing environmental conditions associated with tick bites, suggesting that these reports have a high scientific value. These results support the creation of a Dutch tick bite risk map that, in turn, will open the door to the design of public health interventions to reduce the incidence of Lyme disease.  相似文献   

A Surface-Layer Study of the Transport and Dissipation of Turbulent Kinetic Energy and the Variances of Temperature,Humidity and CO$$_$$     

João A. Hackerott  Mostafa Bakhoday Paskyabi  Joachim Reuder  Amauri P. de Oliveira  Stephan T. Kral  Edson P. Marques Filho  Michel dos Santos Mesquita  Ricardo de Camargo 《Boundary-Layer Meteorology》2017,165(2):211-231

We discuss scalar similarities and dissimilarities based on analysis of the dissipation terms in the variance budget equations, considering the turbulent kinetic energy and the variances of temperature, specific humidity and specific CO\(_2\) content. For this purpose, 124 high-frequency sampled segments are selected from the Boundary Layer Late Afternoon and Sunset Turbulence experiment. The consequences of dissipation similarity in the variance transport are also discussed and quantified. The results show that, for the convective atmospheric surface layer, the non-dimensional dissipation terms can be expressed in the framework of Monin–Obukhov similarity theory and are independent of whether the variable is temperature or moisture. The scalar similarity in the dissipation term implies that the characteristic scales of the atmospheric surface layer can be estimated from the respective rate of variance dissipation, the characteristic scale of temperature, and the dissipation rate of temperature variance.  相似文献   

The Solar Minimum Active Region 7978, Its X2.6/1B Flare,CME, and Interplanetary Shock Propagation of 9 July 1996     

Dryer  M.  Andrews  M. D.  Aurass  H.  DeForest  C.  Galvin  A. B.  Garcia  H.  Ipavich  F. M.  Karlický  M.  Kiplinger  A.  Klassen  A.  Meisner  R.  Paswaters  S. E.  Smith  Z.  Tappin  S. J.  Thompson  B. J.  Watari  S. I.  Michels  D. J.  Brueckner  G. E.  Howard  R. A.  Koomen  M. J.  Lamy  P.  Mann  G.  Arzner  K.  Schwenn  R. 《Solar physics》1998,181(1):159-183

The first X-class flare in four years occurred on 9 July 1996. This X2.6/1B flare reached its maximum at 09:11 UT and was located in active region 7978 (S10° W30°) which was an old-cycle sunspot polarity group. We report the SOHO LASCO/EIT/MDI and SOONSPOT observations before and after this event together with Yohkoh SXT images of the flare, radio observations of the type II shock, and GOES disk-integrated soft X-ray flux during an extended period that included energy build-up in this active region.The LASCO coronagraphs measured a significant coronal mass ejection (CME) on the solar west limb beginning on 8 July at about 09:53 UT. The GOES 8 soft X-ray flux (0.1–0.8 nm) had started to increase on the previous day from below the A-level background (10^-8 W m^-2). At the start time of the CME, it was at the mid-B level and continued to climb. This CME is similar to many events which have been seen by LASCO and which are being interpreted as disruption of existing streamers by emerging flux ropes.LASCO and EIT were not collecting data at the time of the X-flare due to a temporary software outage. A larger CME was in progress when the first LASCO images were taken after the flare. Since the first image of the 'big' CME was obtained after the flare's start time, we cannot clearly demonstrate the physical connection of the CME to the flare. However, the LASCO CME data are consistent with an association of the flare and the CME. No eruptive filaments were observed during this event.We used the flare evidence noted above to employ in real time a simplified Shock-Time-of-Arrival (STOA) algorithm to estimate the arrival of a weak shock at the WIND spacecraft. We compare this prediction with the plasma and IMF data from WIND and plasma data from the SOHO/CELIAS instrument and suggest that the flare - and possibly the interplanetary consequences of the 'big' CME - was the progenitor of the mild, high-latitude, geomagnetic storm (daily sum of Kp=16+, Ap=8) on 12 July 1996. We speculate that the shock was attenuated enroute to Earth as a result of interaction with the heliospheric current/plasma sheet.presently at High Altitude Observatory, Boulder, CO80309, U.S.A.presently at Naval Research Laboratory, Washington DC, 20375, U.S.A.  相似文献   

Extended (15 × 6 AU) Hα Emission Around T Tau N     

P. J. V. Garcia  E. Thiébaut 《Astrophysics and Space Science》1998,261(1-4):141-142

We present an image of T Tauri N reconstructed from speckle interferometry observations made at the 3.6 m Canada-France-Hawaii telescope (CFHT). Two spectral windows, at Hα [6540-6580 Å] and red continuum [6580-6840 Å] were used. The star is unresolved in the continuum (θ ≤ 0″038), setting an upper limit for its size of ≤ 5.3 AU (assuming a 140 pc distance). At Hα (continuum subtracted) two components are observed, an unresolved one with 70% of the Hα flux and a resolved 0″106 × 0″043 (15 × 6 AU) with 30 %. The extended component is elongated in the North-South direction. The extended Hα component scale, it's non-detection in the continuum, and TTau Hα profile shape suggest that the extension is a disk corona.  相似文献   

Flare plasma diagnostics based on the soft X-ray photometric data from GOES and PROGNOZ     

Howard A. Garcia  Frantisek Fárník 《Solar physics》1992,141(1):127-146

Concurrent observations of solar soft X-ray photometers aboard the US weather and space environment monitoring satellite GOES 6 and the USSR geophysical research satellite PROGNOZ 9 made it possible to compare physical parameters of flare plasmas obtained from both instruments as they observed the same solar events. Because of significant instrumental differences, a new method for comparing results had to be developed; this method is described.This paper addresses two related topics: (1) the intercomparison of two dissimilar X-ray photometers that cover approximately the same region of the X-ray spectrum, and (2) the analysis of flare plasma during the rise and decay phases, utilizing the dissimilar response characteristics of the X-ray sensors to discriminate the non-isothermal from isothermal epochs and to identify some of the main properties of those epochs.The intercomparison work considered the different spectral responses of the two photometers, but it was found that the residual differences in the respective X-ray fluxes were apparently due to a combination of environmental factors and uncertainties in the sensor calibrations. These sources of error affected the overall output of the photometers and the relative output of the two channels within each instrument. The effect of the error sources was largest at low flux levels and low temperatures; consequently the computed temperatures and emission measures were in relatively good agreement near X-ray maximum, particularly for those flares registering the highest temperatures.The analysis of flare plasma composition indicated that at the initial stage the plasma is strongly non-isothermal; it then thermalizes gradually, becoming mainly isothermal during the decay phase. A method for quantifying the distribution of the non-isothermal plasma is presented.  相似文献