On the Red Rectangle optical emission bands     

Robert J. Glinski  Christopher M. Anderson 《Monthly notices of the Royal Astronomical Society》2002,332(2):L17-L22

We have observed the Red Rectangle nebula with the Multi-Object Spectrograph on the WIYN telescope. Moderate-resolution spectra (Δ λ =0.4 Å) in the region of 5800 Å were obtained in 3-arcsec apertures at over 50 positions in the nebula. Accurate and precise wavelength calibrations were obtained against a thorium–argon lamp and the sodium lines in the sky and nebula. The peak position and full width at half-maximum of the 5800-Å Red Rectangle band (RRB) were measured to beyond 15 arcsec from the star. The shortest wavelength of the band is found to be 5799.10±0.15 Å in the rest frame of the nebula. None of the emission bands has intensity coincident with the wavelength of the diffuse interstellar band (DIB) at 5797.11±0.05 Å. The 2-Å offset cannot be explained by an instrumental, spectroscopic or photophysical effect. The hypothesis that the same molecule may be the carrier of the RRB and the DIB is contradicted by these observations. As a further test of the hypothesis, absorption has been sought that would be due to a potential DIB carrier in the nebula. Tentative evidence for absorption is found in the RRB spectra taken within 9 arcsec of the star; but any absorption has a peak position essentially coincident in wavelength with the band maximum of the emission band.  相似文献   

Clinopyroxene REE Geochemistry of the Red Hills Peridotite, New Zealand: Interpretation of Magmatic Processes in the Upper Mantle and in the Moho Transition Zone   总被引：1，自引：0，他引：1  

Sano  Sakae; Kimura  Jun-Ichi 《Journal of Petrology》2007,48(1):113-139

The Red Hills peridotite in the Dun Mountain ophiolite of SouthIsland, New Zealand, is assumed to have been produced in a paleo-mid-oceanridge tectonic setting. The peridotite is composed mostly ofharzburgite and dunite, which represent residual mantle andthe Moho transition zone (MTZ), respectively. Dunite channelswithin harzburgite blocks of various scales represent the MTZcomponent. Plagioclase- and clinopyroxene-bearing dunites occursporadically within common dunites. These dunites representproducts of melt–wall-rock interaction. Chondrite-normalizedrare earth element (REE) patterns of MTZ clinopyroxenes showa wide compositional range. Clinopyroxenes in plagioclase dunitesare extremely depleted in light REE (LREE) ([Lu/La]_N >100),and are comparable with clinopyroxenes in abyssal peridotitesfrom normal mid-ocean ridges. Interstitial clinopyroxenes inthe common dunite have flatter patterns ([Lu/La]_N 2) comparablewith those for dunite in the Oman ophiolite. Clinopyroxenesin the lower part of the residual mantle harzburgites are evenmore strongly depleted in LREE ([Lu/La]_N = 100–1000) thanare mid-ocean ridge peridotites, and rival the most depletedabyssal clinopyroxenes reported from the Bouvet hotspot. Incontrast, those in the uppermost residual mantle harzburgiteand harzburgite blocks in the MTZ are less LREE depleted ([Lu/La]_N= 10–100), and are similar to those in plagioclase dunite.Clinopyroxenes in the clinopyroxene dunite in the MTZ are similarto those reported from mid-ocean ridge basalt (MORB) cumulates,and clinopyroxenes in the gabbroic rocks have compositions similarto those reported from MORB. Strong LREE and middle REE (MREE)depletion in clinopyroxenes in the harzburgite suggests thatthe harzburgites are residues of two-stage fractional melting,which operated initially in the garnet field, and subsequentlycontinued in the spinel lherzolite field. The early stage meltingproduced the depleted harzburgite. The later stage melting wasresponsible for the gabbroic rocks and dunite. Strongly LREE–MREE-depletedclinopyroxene in the lower harzburgite and HREE-enriched clinopyroxenein the upper harzburgite and plagioclase dunite were formedby later reactive melt migration occurring in the harzburgite. KEY WORDS: clinopyroxene REE geochemistry; Dun Mountain ophiolite; Moho transition zone; orogenic peridotite; Red Hills  相似文献   

湖北武汉地区志留系下红层的古鱼类化石及其生物古地理意义^*          下载免费PDF全文

山显任  朱敏  赵文金  盖志琨 《古地理学报》2023,25(2):327-340

依据在湖北武汉古姆山志留系浅海红层中新发现的古鱼类化石,确证了兰多维列统特列奇阶下部红层——志留系下红层在鄂东南地区广泛存在,并在前人工作基础上对武汉地区原坟头组进行了重新厘定,将其一分为二,上部仍为坟头组,下部则称清水组。新厘定后的坟头组以黄绿色、灰绿色、灰黄色泥岩、泥质粉砂岩、粉砂岩为主,富含腕足类、双壳类、腹足类、三叶虫和遗迹化石; 清水组下部以紫红色、红褐色泥岩、泥质粉砂岩为主,夹少量石英砂岩,上部以紫红色、黄绿色石英砂岩为主,夹泥岩、泥质粉砂岩、粉砂岩。在清水组上部新发现的鱼类化石包括盔甲鱼类锅顶山汉阳鱼(Hanyangaspis guodingshanensis)、意外洪山鱼(Hongshanaspis inexpectatus)、后棘江夏鱼(Jiangxialepis retrospina)及软骨鱼类中华棘鱼(Sinacanthus)、新中华棘鱼(Neosinacanthus)。这些新发现的古鱼均为张家界脊椎动物群温塘鱼类化石组合中的成员,其中,后棘江夏鱼可以跟产自江西武宁地区下红层清水组中的九江江夏鱼(J. jiujiangensis)直接对比,二者同属于真盔甲鱼目曙鱼科江夏鱼属,而曙鱼科成员则可以作为志留系下红层的标志性分子。根据鱼群面貌和地层层序,武汉地区的志留系下红层可以与皖、苏地区的侯家塘组、浙西北地区的唐家坞组、赣西北地区的清水组、湘西北地区的溶溪组以及新疆塔里木地区的塔塔埃尔塔格组进行很好的对比,其时代为志留纪兰多维列世特列奇期早期。华南板块志留系下红层的分布特征表明, 在特列奇期早期,上、下扬子海之间存在一狭长的浅海区域,这为盔甲鱼类在湖北武汉和江西武宁两地之间的扩散与交流提供了便利条件和可能。  相似文献   

哀牢山—红河剪切带新生代热史演化及其构造意义     

孙崇波  李敏同  李俊  周洪兵  陈晓东 《地质论评》2023,69(2):2023020007-2023020007

笔者等通过对哀牢山—红河剪切带5件砂岩磷灰石样品裂变径迹分析,获得测试分析样品的表观年龄,对所有样品利用模拟退火法进行了热史模拟,取得其热演化史;得出哀牢山—红河剪切带在新生代发生了相似的构造演化过程,其经历了2次快速冷却剥露事件,分别发生在37～14 Ma和5. 1～0 Ma,平均冷却速率分别为3. 98℃/Ma和11. 15℃/Ma;在发生快速冷却的时间上,存在自东向西逐渐变晚的趋势,说明哀牢山—红河剪切带在新生代可能为自东向西的幕式隆升。  相似文献   

晚中新世-上新世黄土高原佳县红粘土剖面碳同位素记录与C4植被演化     

何同  刘连文  陈旸  强小科  季峻峰 《第四纪研究》2015,35(4)

新生代C4植被开始扩张的年代、过程和驱动机制是全球古气候变化研究的焦点问题.中国黄土高原的黄土-红粘土剖面保存了连续的古生态演化记录,是研究这一关键科学问题的理想载体.本文选择黄土高原北部佳县厚达64m的红粘土剖面(8.2～2.7Ma),对190个层位的次生方解石矿物进行了无机碳同位素测试,由此分析了晚中新世-上新世末的C4植被扩张和演化过程.C4植被持续增长与全球冰盖的扩张基本一致,表明气候变冷很可能导致了黄土高原区域气候的干旱化与降雨季节性的增强.C4植被的扩张存在明显的3个阶段,分别以6.6Ma和3.6Ma为界限,每一次扩张增加10％左右,暗示了全球性的构造事件对黄土高原植被演化的控制.此外,佳县红粘土剖面呈现10次持续时间为10 ～ 20万年的碳同位素正漂移事件,平均每40万年发生一次,说明40万年轨道周期也控制着C4植被的演化.  相似文献   

美国阿拉斯加红狗铅锌矿床地质特征及成矿模式     

张辉  徐九华  成曦晖 《地质通报》2015,34(6):1011-1025

美国阿拉斯加红狗(Red Dog)铅锌矿床为典型的喷流沉积型(SEDEX)或页岩容矿矿床,拥有世界上最丰富的锌储量。矿床赋存于石炭纪库纳组中。该地层由黑色富有机质的硅质泥岩和页岩组成,局部有大量的碳酸盐浊积岩。根据闪锌矿结构和成分变化,矿化可分为4个阶段:早期褐色闪锌矿阶段、黄褐色闪锌矿阶段、红褐色闪锌矿阶段和晚期棕褐色闪锌矿阶段,其中第2和第3阶段为主矿化阶段。成矿年代学及古地磁研究表明,矿化作用与库纳组沉积作用同时发生,且存在中生代热液叠加。矿床形成经历了4个沉积-热液成矿过程:未固结泥中重晶石和硫化物沉积、重晶石的热液重结晶和硫化物沉淀、重晶石和硫化物脉的形成并交代早期重晶石,以及晚期角砾岩-细粒石英和晚期棕褐色闪锌矿的形成。  相似文献   

Evaluating the feasibility of multitemporal hyperspectral remote sensing for monitoring bioremediation     

《International Journal of Applied Earth Observation and Geoinformation》2015

In recent years, several studies focused on the detection of hydrocarbon pollution in the environment using hyperspectral remote sensing. Particularly the indirect detection of hydrocarbon pollution, using vegetation reflectance in the red edge region, has been studied extensively. Bioremediation is one of the methods that can be applied to clean up polluted sites. So far, there have been no studies on monitoring of bioremediation using (hyperspectral) remote sensing. This study evaluates the feasibility of hyperspectral remote sensing for monitoring the effect of bioremediation over time. Benzene leakage at connection points along a pipeline was monitored by comparing the red edge position (REP) in 2005 and 2008 using HyMap airborne hyperspectral images. REP values were normalized in order to enhance local variations caused by a change in benzene concentrations. 11 out of 17 locations were classified correctly as remediated, still polluted, or still clean, with a total accuracy of 65%. When only polluted locations that were remediated were taken into account, the (user's) accuracy was 71%.  相似文献   

Labour struggles and the formation of demands: The spatial politics of Red Clydeside     

《Geoforum》2015

This paper combines labour history and labour geography through an analysis of the making of labour demands in Glasgow during the early twentieth century. The paper asserts how revisiting histories such as Red Clydeside reveals complexities within labour movements and links to more recent debates within labour geography. Archival research provides a relational account of the place-based politics of Glasgow that emerged during the forty hours movement in 1919. This allows the paper to juxtapose the broader international linkages forged by Scottish workers alongside racialised hostilities within the city. In particular, the paper compares and contrasts the progressive internationalism of the strike newspaper with the Broomielaw race riot between local and foreign sailors during the same month as the strike. This comparison also raises the longer-term trajectories of labour grievances to foreground the ambivalent and contested nature of labour demands, identities and histories. In particular, the paper pays close attention to contrasting practices of labour internationalism emerging from the relevant archives. This historical approach makes a broader contribution to debates within labour geography by engaging with the complexities and tensions of labour organising and demand making.  相似文献   

北美地区一次冬季中尺度对流系统上空红色精灵现象的空间观测及其母体雷暴分析     

钟丽华  杨静  陆高鹏  王庸平  何其佳  郄秀书 《大气科学》2020,44(5):997-1012

红色精灵是发生在雷暴云上空的一种大尺度瞬态放电发光现象,它们通常出现在地面上空40～90 km之间,是由地闪回击和随后可能存在的连续电流产生的。目前,由于综合同步观测资料较少,与夏季红色精灵相比,全世界对冬季红色精灵的研究屈指可数。2008年12月27～28日,受高空槽及低层暖湿气流的影响,北美阿肯色州地区爆发了一次冬季雷暴天气过程,搭载于FORMOSAT-2卫星上的ISUAL（Imager of Sprites and Upper Atmospheric Lightning）探测器有幸在这次雷暴上空记录到了两例红色精灵事件。本文利用ISUAL获取的红色精灵观测资料、多普勒天气雷达资料、美国国家闪电定位资料、超低频磁场数据、美国国家环境中心/气候预测中心提供的云顶亮温和探空数据等综合观测数据,对产生红色精灵的这次冬季雷暴特征和相关闪电活动规律进行了详细研究。结果表明,在两例红色精灵中,ISUAL均未观测到伴随的“光晕（halo）”现象,第一例为“圆柱状”红色精灵,第二例红色精灵由于发光较暗,无法判断其具体形态。产生红色精灵的母体雷暴是一次中尺度对流系统,该系统于27日15:00（协调世界时,下同）左右出现在阿肯色州北部附近,并自西向东移动。23:59系统发展到最强,最大雷达反射率因子（55～60 dBZ）的面积达到339 km2,之后开始减弱。03:03雷暴强度有所增加,随后云体便逐渐扩散,雷暴开始减弱,并在11:00完全消散。两例红色精灵发生分别在04:46:05和04:47:14,此时雷暴处于消散阶段,正负地闪频数均处于一个较低水平且正地闪比例显著增加,并且多位于云顶亮温?40°C～?50°C的层状云区上空。红色精灵的出现伴随着30～35 dBZ回波面积的增加。在红色精灵发生期间,雷达反射率大于40 dBZ的面积减少,10～40 dBZ的面积增加,表明红色精灵的产生与雷暴对流的减弱和层状云区的发展有关,这与已有的夏季红色精灵的研究结果类似。红色精灵的母体闪电为正地闪单回击,位于中尺度对流系统雷达反射率为25～35 dBZ的层状云降水区,对应的雷达回波顶高分别为2.5 km和5 km,峰值电流分别为+183 kA和+45 kA。根据超低频磁场数据估算两个母体闪电的脉冲电荷矩变化（iCMC）分别为+394 C km和+117 C km。超低频磁天线记录到了第一例红色精灵内部的电流信号,表明这例红色精灵放电很强。  相似文献   

Hipparcos and red dwarf populations     

C. Turon  F. Crifo  D. Morin 《Astrophysics and Space Science》1994,217(1-2):77-82

The European Space Agency's Hipparcos satellite, launched in August 1989, and operated until August 1993, sent back scientific data for about 36 months. The reduction of the first 18 months already shows that the target accuracy for the five astrometric parameters of each star (0.002 arcsec for the position and annual proper motion components, and for the parallax) and for the photometric data (a few milli-magnitudes) will be achieved or even exceeded for most of the 118 000 pre-selected programme stars. These preliminary results will be presented.The contents of the Hipparcos observing programme with respect to red stars and anticipated improvements in the study of red dwarfs will be underlined.  相似文献