Younger Dryas时期东亚季风气候和中国东部沙区沙漠变化

位于沙漠／黄土过渡带的杨桃峁剖面,高分辨率地记录了ＹｏｕｎｇｅｒＤｒｙａｓ时期东亚季风气候和沙漠变化历史。在ＡＭＳ１４Ｃ测年基础上,磁化率、粒度和有机质含量等替代性气候指标的测试结果分析表明,ＹｏｕｎｇｅｒＤｒｙａｓ时期东亚季风气候在全球气候变化的影响下,总的表现为与北半球高纬度地区相同的干寒特征,即沙漠总的具有扩大的趋势;但又与南北半球大气相互作用,特别是赤道太平洋地区气压异常引起亚洲季风气候的不稳定有关,表现出降水变化特点,沙漠出现逆过程变化,存在短暂成壤固定时期。     

南黄海第四纪轨道事件与非轨道事件的探讨

南黄海陆架区,作为地球轨道事件的代表,最明显的表现是海侵—海退序列。其中海侵层HⅠ、HⅣ、HⅤ、HⅥ、HⅦ分别与氧同位素1、5、7、13、23等温暖阶段相对应。主要的海侵周期受控于地球轨道要素所引起的全球变化进程。 关于非轨道事件,在南黄海发现了新仙女木事件(Younger Dryas)的证据,在~(14)C测年11100±260aB.P.至10340±110aB.P.这一时段,出现了海平面短时期下落;孢扮资料发现11100aB.P.以前的植被由栎树落叶阔叶林—草原突变为干旱草原植被,持续到11340aB.P.再度变为栎树落叶阔叶林植被,证明这段时间发生了突然变旱及降温事件。从碳氧同位素资料还发现14100±810aB.P.(~(14)C)之后的冰消期在新仙女木期之前有两期更短时间的降温,可对应于老仙女木期(Older Dryas)和最老仙女木期(Oldest Dryas)。     

Origin and evolution of the granitic intrusions in the Brusque Group of the Dom Feliciano Belt,south Brazil: Petrostructural analysis and whole-rock/isotope geochemistry

In the southern Brazilian state of Santa Catarina the Dom Feliciano Belt, formed by the tectonic juxtaposition of different crustal blocks during the Brasiliano-Pan African Orogenic cycle, can be divided into three domains. In the central domain, three granitic suites intrude the metavolcanosedimentary sequence of the Brusque Group: São João Batista (SJBS), Valsungana (VS) and Nova Trento (NTS), from the oldest to the youngest. This extensive magmatism, here referred to as granitic intrusions in the Brusqe Group (GIBG), is coeval with the thermal peak in the host metamorphic successions, but postdates its main foliation. A progressive deformation starting from the magmatic stage throughout the cooling history points to the influence of the late stages of deformation recorded in the Brusque Group.The SJBS consists of gray to white leucocratic, equigranular granites, with aluminous minerals such as muscovite, garnet and tourmaline. The porphyritic VS is the largest of the suites and is characterized by its cm-sized K-feldspar megacrysts in a coarse-grained biotite-rich matrix. The granites from the NTS are equigranular, light gray to pink in color and have biotite as the main mafic mineral, but magmatic muscovite, tourmaline and hornblende can occur as well.Geochemically, the GIBG are mildly peraluminous and show a calc-alkaline affinity. Most intrusions have a high REE fractionation, but some SJBS granites show a characteristic pattern with no fractionation and strong negative Eu anomalies (“seagull pattern”). Elevated Sr(i) values, between 0.707 and 0.735, and negative ε_Nd values as low as −24 points to the melting of old evolved crust. The Nd (T_DM) ages are scattered between 1.54 and 2.76 Ga, with a predominance of values around 2.0 Ga.The GIBG have a strong crustal signature that most closely connects, within the regional units, to that of the metasedimentary rocks of the Brusque Group and its crystalline basement, the Camboriú Complex. All three suites seem to have been produced during a same regional melting event, but at different crustal levels and reflecting heterogeneities within the same source rocks. Most evidences imply that sedimentary source rocks were especially important to the SJBS, which probably originated in a shallower environment, whilst the VS and NTS represent the melting of deeper crystalline crust, probably sharing some magmatic interaction.     

How late are K-feldspar megacrysts in granites?

Various petrologists have suggested that K-feldspar megacrysts grow in granites that are extensively crystallized, even at subsolidus conditions. However, experimental evidence indicates that, though K-feldspar nucleates relatively late in the crystallization history, abundant liquid is available for development of large crystals. A great deal of evidence, involving many different factors, favours a magmatic/phenocrystic origin for K-feldspar megacrysts in granites, namely simple twinning, oscillatory zoning, euhedral plagioclase inclusions, and concentric, crystallographically controlled arrangements of inclusions. In addition, abundant evidence has been presented of (1) mechanical accumulation of K-feldspar megacrysts in granites, (2) alignment of megacrysts and megacryst concentrations in magmatic flow foliations, (3) involvement of megacrysts in zones of magma mixing in granite plutons, and (4) occurrence of megacrysts in some volcanic rocks, implying that the megacrysts were suspended in enough liquid to be moved without fracturing or plastic deformation. Detailed trace element and isotopic data also indicate that megacrysts can move between coexisting felsic and more mafic magmas. Irregular overgrowths on megacrysts are consistent with continued magmatic growth after euhedral megacrystic growth ceased, the overgrowths being impeded by simultaneously crystallizing quartz and feldspar grains.     

Evidence of temperature depression and hydrological variations in the eastern Sierra Nevada during the Younger Dryas stade

Sediment records from two lakes in the east-central Sierra Nevada, California, provide evidence of cooling and hydrological shifts during the Younger Dryas stade (YD; ~ 12,900-11,500 cal yr BP). A chironomid transfer function suggests that lake-water temperatures were depressed by 2°C to 4°C relative to maximum temperatures during the preceding Bølling-Allerød interstade (BA; ~ 14,500-12,900 cal yr BP). Diatom and stable isotope records suggest dry conditions during the latter part of the BA interstade and development of relatively moist conditions during the initiation of the YD stade, with a reversion to drier conditions later in the YD. These paleohydrological inferences correlate with similar timed changes detected in the adjacent Great Basin. Vegetation response during the YD stade includes the development of more open and xeric vegetation toward the end of the YD. The new records support linkages between the North Atlantic, the North Pacific, and widespread YD cooling in western North America, but they also suggest complex hydrological influences. Shifting hydrological conditions and relatively muted vegetation changes may explain the previous lack of evidence for the YD stade in the Sierra Nevada and the discordance in some paleohydrological and glacial records of the YD stade from the western United States.     

皖南侏罗-白垩纪两类花岗岩的岩石成因、氧逸度特征及成矿意义

皖南地区北接长江中下游铜铁金成矿带,南临赣东北德兴铜、金矿集区,成矿潜力巨大。迄今已在区域内发现多个大中型W、Mo、Cu、Au矿床。本次研究选取多个可能与成矿有关的小型花岗岩体进行岩石成因、氧逸度高低及其成矿潜力分析。研究发现:皖南侏罗-白垩纪发育两期花岗岩,早期花岗岩主要形成于160~140±5Ma,岩性多为花岗闪长岩等偏中性岩石,岩石成因与中晚侏罗世的板块俯冲挤压有关。晚期花岗岩主要形成于140±5~120Ma,岩性以花岗岩、正长花岗岩以及碱性花岗岩为主,岩石的成因与构造体制转换之后的伸展环境有关。利用锆石中稀土微量元素的含量计算出皖南及相邻地区早期(160~140±5Ma)花岗岩普遍具有比较高的Ce4+/Ce3+值,即岩浆具有高氧逸度;而晚期(140±5~120Ma)花岗岩的Ce4+/Ce3+值普遍偏低,指示了岩浆具有较低的氧逸度。通过对氧逸度与成矿关系的分析,认为皖南燕山早期发育的花岗质岩类具有良好的铜、金、钼找矿潜力。     

The younger dryas cooling in northeast Germany: summer temperature and environmental changes in the Friedländer Groβe Wiese region

A lake sediment record from the Friedländer Groβe Wiese in northeast Germany was studied to reconstruct summer temperature changes associated with changes in vegetation development during the Weichselian Lateglacial. The record was analysed for pollen, chironomids, and oxygen and carbon isotopes of lake marl. The combination of radiocarbon dates, the presence of the Laacher See Tephra and correlation of lithological and palynological changes with other records from the region indicated that the record encompassed the Allerød to the early Holocene. Pollen assemblages reflect development of birch and later pine‐dominated forests during the Allerød, comparable to other sites in the region. Chironomid‐inferred mean July air temperatures (C‐IT) for this period range between ～14.0 and 14.8°C. A temporary decrease in C‐IT of ～1°C, a negative shift in the isotope records, and a minor decline of birch may correspond to Greenland Interstadial 1b. Even though the transition to the Younger Dryas appears to be affected by reworking and redeposition processes, a drop in C‐IT to ～11.1°C is reconstructed for the later part of the Younger Dryas, while it appears that pine locally persisted in the region. Comparison with a nearby pollen record further indicates a local expansion of wetland grasses during this period. At the transition to the Holocene, C‐IT increased to ～15.7°C, while birch and pine forests re‐expanded. Copyright © 2012 John Wiley & Sons, Ltd.     

Relict rock glaciers and protalus lobes in the British Isles: implications for Late Pleistocene mountain geomorphology and palaeoclimate

Many relict rock glaciers and protalus lobes have been described in mountainous areas of the British Isles. This paper reviews their distribution, chronology, supposed origin and development, and places the research within current investigations and knowledge. Rock glaciers and protalus lobes are located in a number of different topographic locations and settings. They developed at the base of steep cliffs following the catastrophic failure of rock faces, at the base of scree slopes following the gradual accumulation of rock debris and in association with glaciers. Protalus lobes probably developed in response to the permafrost creep of talus material while rock glaciers formed through the deformation and sliding of large bodies of buried ice. Rock glaciers probably developed, or were last active, during the Younger Dryas, although the possibility exists that some of these landforms are Dimlington Stadial in age. The development of protalus lobes during the Younger Dryas suggests that precipitation levels were low and permafrost was widespread during this time. The lack of rock glaciers (sensu stricto) in the British Isles compared with other mountain areas is believed to be a consequence of the rock type and relative scarcity of weathered debris for their formation rather than a lack of suitable sites or appropriate environmental conditions. Copyright © 2007 John Wiley & Sons, Ltd.