History of scoria-cone eruptions on the eastern shoulder of the Kenya–Tanzania Rift revealed in the 250-ka sediment record of Lake Chala near Mount Kilimanjaro     

Catherine Martin-Jones  Christine Lane  Maarten Van Daele  Thijs Van Der Meeren  Christian Wolff  Heather Moorhouse  Emma Tomlinson  Dirk Verschuren 《第四纪科学杂志》2020,35(1-2):245-255

Reconstructions of the timing and frequency of past eruptions are important to assess the propensity for future volcanic activity, yet in volcanic areas such as the East African Rift only piecemeal eruption histories exist. Understanding the volcanic history of scoria-cone fields, where eruptions are often infrequent and deposits strongly weathered, is particularly challenging. Here we reconstruct a history of volcanism from scoria cones situated along the eastern shoulders of the Kenya–Tanzania Rift, using a sequence of tephra (volcanic ash) layers preserved in the ~250-ka sediment record of Lake Chala near Mount Kilimanjaro. Seven visible and two non-visible (crypto-) tephra layers in the Lake Chala sequence are attributed to activity from the Mt Kilimanjaro (northern Tanzania) and the Chyulu Hills (southern Kenya) volcanic fields, on the basis of their glass chemistry, textural characteristics and known eruption chronology. The Lake Chala record of eruptions from scoria cones in the Chyulu Hills volcanic field confirms geological and historical evidence of its recent activity, and provides first-order age estimates for seven previously unknown eruptions. Long and well-resolved sedimentary records such as that of Lake Chala have significant potential for resolving regional eruption chronologies spanning hundreds of thousands of years.  相似文献   

内蒙古贺斯格乌拉牧场白音高老组火山岩U-Pb年龄及地球化学特征     

胡振华 《地质与勘探》2020,56(2):359-371

白音高老组火山岩在大兴安岭地区广泛分布,本文对大兴安岭中南部贺斯格乌拉牧场白音高老组酸性火山岩进行了锆石U-Pb年代学、岩石地球化学和Sr-Nd同位素分析,探讨其岩石成因及构造背景。位于大兴安岭中南段东乌旗地区的白音高老组火山岩,主要岩性为流纹岩、流纹质凝灰岩等,LA-ICP-MS锆石U-Pb年龄分别为129. 8±0. 8 Ma、128. 2±2. 8 Ma,属早白垩世早期;从岩石地球化学特征上看,其主量元素SiO_2含量68. 76%～76. 18%、Al_2O_3含量11. 84%～13. 38%,属高钾钙碱性岩石;稀土总量较高,(La/Yb)N 6,(La/Sm)_N 3,显示为轻稀土富集型,δEu显示负铕异常(0. 4～0. 6),微量元素以富集大离子亲石元素K、Rb、Ba,贫高场强元素Nb、P、Ti为特征; Sr-Nd同位素组成上具有低I_(Sr)、高ε_(Nd)(t)和低t_(DM)的特征(I_(Sr)=0. 7039～0. 7045,ε_(Nd)(t)=2. 65～4. 39)。火山岩浆来源于下地壳基性物质的部分熔融,综合研究并结合前人资料认为,白音高老组流纹岩形成于滨太平洋板块俯冲后伸展及蒙古-鄂霍次克洋闭合后的综合效应下。  相似文献   

城市建成环境对居民体力活动的影响 ——以福州市的经验研究为例   总被引：2，自引：1，他引：1  

张延吉  陈小辉  赵立珍  马妍 《地理科学》2019,39(5):779-787

利用福州中心城区的社会调查、POI、道路网、用地性质等数据,在社区尺度探究城市建成环境对居民休闲型中高强度体力活动的影响。研究发现：① 低密度土地利用与体力活动时长呈正向关联,功能单一和邻近主干道则对体力活动起到抑制作用。② 体力活动目的地对不同人群具有差异化影响,体育用地和付费运动场所仅能促进中高阶层和中高收入者的体力活动,而周边公共运动设施的丰富程度更具普适性意义。③ 通过纳入运动偏好和单独分析保障房、单位大院及房改房住户达到规避居住自选择的目的,证明上述建成环境特征对体力活动的影响是独立且稳健的。  相似文献   

浑河断裂地球物理场特征及地震活动性     

张鐘月  万波  彭虎  田德欣 《世界地质》2020,39(1):176-184

浑河断裂是辽宁省内一条重要的北东向地震构造带,断裂两侧的地球物理重磁场存在差异。通过浑河断裂的区域重力场与磁场研究,认为浑河断裂既控制了深、浅部岩石地层的发育,同时浑河断裂的重力场、磁场分布随着深、浅部地层岩性发育的差异而有所变化。浑河断裂的重力场和磁场梯度带主要位于抚顺以西至沈阳一带,浑河断裂历史以来有记录的最大破坏性地震位于重力梯度变化较大的沈阳段。综合浑河断裂地球物理场特征及区域地质资料,浑河断裂虽然活动性一般,但抚顺地区的采煤活动对断裂的活动性有一定影响。近些年抚顺地区频发的沉降、滑坡和地裂缝等地质灾害应当引起对浑河断裂活动性研究的重视。  相似文献   

大兴安岭南部二叠系—三叠系界线及沉积环境演化     

陈树旺  郑月娟  张健  张海华  张德军  苏飞  黄欣  公繁浩  甄甄 《中国地质》2020,47(3):821-838

北方陆相二叠系—三叠系界线研究是界线地层研究的重要问题之一,对采自内蒙古巴林右旗幸福之路组二段建组剖面的安山质岩屑晶屑凝灰岩开展锆石LA-ICP-MS U-Pb测年,结果为(255.5±1.1)Ma,火山岩上部多个层位粉砂质泥岩中发现孢粉化石,计17属20种,时代为晚二叠世—早三叠世,推断幸福之路组的时代为晚二叠世—早三叠世,大兴安岭地区二叠系—三叠系界线在幸福之路组内部,二者为整合接触。幸福之路组以红层做为划分标志,岩性为正常沉积碎屑岩夹火山岩,见大量泥灰岩夹层、钙质结核及干裂现象,反映了炎热、干燥及强氧化条件的气候环境,大兴安岭地区晚二叠世晚期(幸福之路组二段下部)就已出现反映干旱气候的红层沉积,与相邻的华北及新疆准噶尔盆地相似。  相似文献   

Isolation, distribution and evaluation of cytotoxic and antioxidant activity of cultivable actinobacteria from the Oman Sea sediments     

Gozari Mohsen  Bahador Nim  Jassbi Amir Rez  Mortazavi Mohammad Seddiq  Hamzehei Sam  Eftekhar Ebrahim 《海洋学报(英文版)》2019,38(12):84-90

Screening bioactive natural products from bacteria is a determinative step in the drug discovery programs. The present study aim to isolate actinobacteria from the Oman Sea sediments for determining the effects of different culture media and treatments on the yield of the isolation process, and measure the DPPH radical scavenging and Artemia cytotoxic activity of culture extracts of the actinobacterial isolates. A total of 290 actinobacterial isolates were collected from 14 sediment samples. Heat treatment(40.68%) and M_4 medium(29.31%) exhibited the maximum isolation rates of actinobacteria. Streptomyces isolates were dominantly distributed in all of the investigated stations according to 16 S rRNA gene sequencing. The distribution pattern of Streptomyces followed a depth-dependent frequency trend, whereas the members of rare genera including Micromonospora, Nocardia Actinoplanes, Nocardiopsis, Saccharopolyspora and Crossiella were distributed in deeper stations. Approximately,25% of the examined isolates could scavenge 90% of 10~(–4) mol/L DPPH solutions at 1 250 μg/mL final concentration of their ethyl acetate culture extracts. Furthermore, the most potent extracts could scavenge DPPH radicals with IC50 ranges from 356.8 to 566.4 μg/mL. Brine shrimp cytotoxicity tests showed that 38.88% of the examined culture extracts exhibited LC_(50) lower than 1 000 μg/mL against the Artemia cells. Moreover, the most potent culture extracts exhibited LC_(50) range from 335.4 to 534.4 μg/mL. Phylogenetic analysis by 16 S rRNA gene sequence revealed that the OS 005, OS 263 and OS 157 closely related to Streptomyces djakartensis, Streptomyces olivaceus and Nocardiopsis dassonvillei respectively. These results suggested the widespread distribution of the antioxidant and cytotoxic producing actinobacteria in the Oman Sea sediments, which could be considered as promising candidates for the discovery of microbial bioactive compounds.  相似文献   

Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo     

Tan Bao-lin  Cheng Jun  Tan Cheng-ming  Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.  相似文献   

两郧断裂郧县盆地段地质与地球物理特征研究     

林松  李媛  王薇  廖武林  乔岳强 《大地测量与地球动力学》2019,39(2):148-152

通过野外地质调查，结合地球物理探测手段，研究两郧断裂郧县盆地段地质与地球物理特征；参照两郧断裂带多个位置采集断层物质的SEM、TL测试成果，并结合本次对断层上断点沉积物OSL测年数据，对两郧断裂该段第四纪活动性进行分析。研究结果表明，两郧断裂在郧县盆地段埋深相对较深；断裂特征主要为逆断层，部分分支断裂显示为正断性质；断裂带最新活动时代为中更新世晚期-晚更新世早期。  相似文献   

福建大田—漳平地区构造-热对煤系石墨成矿及赋存的控制探讨     

丁正云  王路  曾欢  李阳  陈泉霖  邓瑞锦  程乔  林晓炎  曹代勇 《煤田地质与勘探》2020,48(1):55-61

福建省大田—漳平地区位于东部滨太平洋构造带上，不同时期的岩浆热液作用和复杂多变的构造形变格局，为该地区形成丰富的石墨矿床提供了良好的成矿条件。为了查明大田—漳平地区煤系石墨的成矿控制因素及分布规律，通过工业分析、元素分析、X射线衍射和激光拉曼光谱等实验，对不同矿区不同变质程度的煤和煤成石墨的化学组成及微观结构特征等煤成石墨化特征进行了研究，并将不同变形特征的样品划分为煤成石墨、煤成半石墨和石墨化无烟煤三大类。研究表明:煤的变形特征与煤成石墨的演化类型基本一致，且韧性变形样品的石墨化程度最高，说明构造应力作用能促进煤的石墨化作用；煤成石墨的分布受到岩浆-构造活动的控制，石墨矿床多产出于岩浆岩侵入体外接触带或附近断裂带的有利围岩地层中，且大田—漳平地区煤系石墨矿具有明显的成区、成带分布特点，煤成石墨成矿区主要集中在闽西南坳陷南部的漳平一带；而北部大田一带分布的矿区矿体石墨化程度较漳平一带低，多为煤成半石墨或石墨化无烟煤，研究结果可为该地区煤系石墨矿产综合勘探开发利用提供有利依据。   相似文献   

A shift towards wetter and windier conditions in southern Sweden around the prominent solar minimum 2750 cal a BP          下载免费PDF全文

ANETTE MELLSTRÖM  NATHALIE VAN DER PUTTEN  RAIMUND MUSCHELER  RIXT DE JONG  SVANTE BJÖRCK 《第四纪科学杂志》2015,30(3):235-244

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