Geomagnetic secular variation in historical lavas from the Canary Islands     

V. Soler  J. C. Carracedo  F. Heller 《Geophysical Journal International》1984,78(1):313-318

Summary. The age of historical lava flows on the Canary Islands can be traced back at least to 1585 ad . During the last 400 years eruptions occurred at fairly regular intervals. The palaeomagnetic directions of these lavas record the ambient field direction with high precision so that an historical secular variation curve (SVC) can be constructed for the Canaries which closely resembles the curve registered at Paris. The SVC can be used as a dating tool for historical eruptions of unknown age and can probably be extended into the last 4000–5000 yr of recent volcanic activity on the Canaries.  相似文献   

云南元谋盆地含古猿化石层古地磁年龄及古生物学意义   总被引：5，自引：0，他引：5  

岳乐平  张云翔  祁国琴  F.Heller  王建其  杨利荣  张睿 《中国科学D辑》2003,33(11):1069-1075

云南元谋盆地含古猿化石剖面磁性地层学研究表明, 小河剖面记录了Cande-Kent95古地磁年表中的C3Br.1n, C3Br.1r, C3Br.2n, C3Br.2r, C4n.1n, C4n.1r, C4n.2n和C4n.2r 8个极性段, 地层应当归属中新世晚期. 该剖面有两个主要含古猿化石层, 下层(剖面第1层)记录了C4n.2r下部, 古地磁年龄约8.2~8.1 Ma; 上层(剖面第16层)记录了C3Br.1n, 古地磁年龄约7.2~7.15 Ma. 该剖面古猿化石古地磁年龄约为8.2~7.15 Ma. 雷老剖面记录了Cande-Kent95古地磁年表中的C3Br, C3Br.1n, C3Br.1r, C3Br.2n, C3Br.2r, C4n.1n, C4n.1r, C4n.2n, C4n.2r, C4n.3n和C4n.3r 11个极性段, 地层应当归属中新世晚期. 该剖面也有两个主要含古猿化石层, 下层(剖面第3层)记录了C4n.2r, 古地磁年龄约8.2~8.1 Ma; 上层(剖面第19层)记录了C3Br中部, 古地磁年龄约7.15~7.1 Ma, 雷老剖面古猿化石古地磁年龄约为8.2~7.1 Ma. 小河剖面与雷老剖面记录的沉积环境极为相似, 两个剖面的古猿化石年龄相当, 下古猿化石层古地磁年龄约8.1~8.2 Ma, 上化石层古地磁年龄约7.2~7.1 Ma. 这可能反映了在雷老盆地与小河盆地生活的古猿有统一的活动范围. 该区域大约在8.00~7.00 MaBP间始终有古猿活动.  相似文献   

兰州盆地永登剖面记录的第三纪沉积环境   总被引：1，自引：0，他引：1  

岳乐平  邱占祥  颉光普  邱铸鼎  王莉  张云翔  Heller F 《沉积学报》2003,21(4):683-687

对兰州盆地永登剖面第三系沉积进行了沉积学研究、并结合年代学研究结果分析了新生代以来沉积环境变化与气候变化.古新世末至早始新世沉积了一套扇三角洲相沉积(细柳沟组),为具交错层理的砖红色砂岩,顶界年龄约51 Ma.兰州地区在51 MaB.P.经历了一次大的环境变化,气候由相对温暖湿润转为半干旱半湿润,气候炎热,湖盆由淡水湖转为盐湖,蕴示着由副热带高压控制的干旱带北移,兰州地区进入受行星风系控制的干旱带.早始新世晚期至早渐新世早期(51～31.5 Ma B.P.),在近20 Ma时间内经历了微咸湖-盐湖阶段(野狐城组),砂泥岩沉积中含有大量石膏夹层.早渐新世,兰州地区向湿润方向转化,兰州盆地由咸水湖转化为淡水湖,可能反映了东南季风逐渐形成,中国大陆由早先行星风系控制转化为季风控制,前期东南方向干旱带消失,西北干旱带出现,兰州地区相对早先湿润.早渐新世中期至中中新世(31.5～15 Ma B.P.),兰州盆地在经历了三次大的沉积旋回后湖盆逐渐干枯,三个大旋回分别由河流相砂岩-微咸水滨湖相砂泥岩、泛滥平原相泥岩,河流相砂岩-淡水滨湖相砂泥岩-沼泽相、泛滥平原相泥岩,河流相砂岩-沼泽相、泛滥平原相泥岩组成.20 MaB.P盆地接受大量砂砾石沉积,反映出周缘山体快速抬升遭受剥蚀,可能蕴示着青藏高原抬升波及到兰州地区.  相似文献   

Natural Magnetic Archives of Past Global Change   总被引：3，自引：0，他引：3  

M.E. Evans  F. Heller  J. Bloemendal  N. Thouveny 《Surveys in Geophysics》1997,18(2-3):183-196

Rock magnetic parameters of sediments reflect palaeoenvironmental and palaeoclimatic conditions during deposition in the marine and in the continental realm. The processes which lead to enhancement or degradation of the magnetic properties are well known – though not completely understood. They include variable terrigenous material influx, organic and inorganic in situ formation of ferromagnetic minerals and diagenetic destruction of these minerals. Cyclical changes in the magnetic mineral assemblages occurring at the orbital periodicities involved in standard Milankovitch theory have been observed in numerous sedimentary records, at least during the last seven million years. This confirms the relationship between rock magnetism and past global change. Quantitative interpretation of the magnetic signals, however, is still in its infancy and is hampered by the complex interplay of the signal formation processes.  相似文献   

2006年4月17日北京降尘的粒度分布与磁学特征   总被引：5，自引：1，他引：4       下载免费PDF全文

张崧  F.Heller  靳春胜  刘平  秦小光  刘东生 《第四纪研究》2008,28(2):354-362

对2006年4月17日北京降尘的粒度和磁学性质进行深入分析,提出降尘磁化率相对黄土样品较高是现代降尘磁化率的特点,源区表土磁化率普遍较高是本次降尘磁化率值高的主要原因,污染产生的磁性物质对其也有一定的影响。同时通过对比几次降尘的粒度特征和传输方式提出粒度可以有效地指示源区的变化。结合降尘的粒度、磁化率分析与沙尘暴的监测信息和卫星云图,认为此次降尘粒度为0.8～20.0μm的组分可能是来自内蒙古西部的物质;20～70μm与>70μm的组分可能是来自距离北京较近的河北北部和内蒙古中部发生强烈沙尘暴的地区。  相似文献   

Pattern speed of the stellar bar in NGC 7479     

S. Laine  I. Shlosman  & C. H. Heller 《Monthly notices of the Royal Astronomical Society》1998,297(4):1052-1059

We study the pattern speed of the bar in NGC 7479 by comparing observations with numerical simulations of gas flow in a two-dimensional gravitational potential, derived from observations. The best agreement between the observations and the modelling is achieved for the fast bar pattern speed of 27 km s⁻¹ kpc⁻¹, when the corotation radius is at 50 arcsec, i.e. 1.1 times the radial length of the bar. This result is supported by the gas and dust lane morphologies, star formation distribution, projected velocity field and overall morphology. We find that star formation is most likely to be triggered close to the large-scale shocks and dust lanes in the bar. The net gas inflow rate in the simulations at 1-kpc radius is 4–6 M⊙ yr⁻¹ at intermediate times.  相似文献   

Land-air boundary environment as recorded by the¹⁸O/¹⁶O and¹³C/¹²C isotope ratios in the shells of land snails     

Mordeckai Magaritz  Jossef Heller  Michal Volokita 《Earth and Planetary Science Letters》1981,52(1):101-106

A yearly cycle of carbon and oxygen isotope composition of shells of the Israeli land snailXeropicta vestalis is presented. The¹⁸O/¹⁶O values indicate that the snails use water from the land-air boundary zone. The¹⁸O/¹⁶O ratio of the shells is in isotopic equilibrium with the water condensate from the vapour during the winter months. During the summer months a contribution to the above water from soil water migrating upwards due to evaporation is noticeable. The δ¹³C values indicate that as in marine molluscs, the carbon isotopic composition in land snails is controlled mainly by the aqueous carbonate compound which is in equilibrium with the land-air boundary CO₂.  相似文献   

新近系谢家阶层型剖面古地磁年代学研究   总被引：9，自引：1，他引：9  

武力超  岳乐平  王建其  F.Heller  邓涛 《地层学杂志》2006,30(1):50-53

古地磁测量表明,中国新近系谢家阶界线层型剖面——西宁盆地谢家剖面共记录了18个正极性段与17个负极性段,与标准极性柱中C5Bn.2n—C7n.1n之间的极性带能很好的对应。剖面中谢家组的年龄为17.32—21.58Ma,谢家哺乳动物群的年龄约为21Ma,相当于MN2中期。  相似文献   

Über die Erzeugung großräumiger homogener Magnetfelder zum Studium des Verhaltens von Magnetkompassen und Kompensiermitteln auf verschiedenen magnetischen Breiten     

Carl Heller 《Ocean Dynamics》1955,8(4):157-164

Zusammenfassung Zur Herstellung schwacher, homogener Magnetfelder wird die Verwendung quadratförmiger Rahmenspulen vorgeschlagen, die gegenüber gleich großen Kreisringspulen den Vorteil einer größeren Homogenität des Feldes bieten. Es wird die Feldverteilung auf der Achse und in der Ebene einer Quadratspule angegeben. Für die Kombination von zwei Quadratspulen wird die Ermittlung eines optimalen Spulenabstandes gezeigt für die Fälle, daß entweder größte lineare Ausdehnung des homogenen Bereichs auf der Feldachse oder größte flächenhafte Ausdehnung in der Mittelebene des Feldes gefordert wird. Im Helmholtzfall, für den der Abstand der Quadratspulen zum 0,5445fachen der Kantenlänge berechnet wird, erweist sich der räumliche Bereich mit 1 % Feldstärkeabweichung gegen den Feldmittelpunkt um rund 72 % größer als bei einer gleich großen Helmholtzspule der üblichen Form.

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On the production of uniform magnetic fields of great volume for studying the behaviour of magnetic compasses and adjusting devices in different magnetic latitudes

Summary For the production of weak uniform magnetic fields it is proposed to use square frame coils which in contrast to circular coils of the same size offer the advantage of a greater field homogeneity. The field distribution on the axis and in the plane of a square coil is indicated. For the use of two combined square coils the determination of the optimum coil separation is given for the cases that there should either be required greatest linear extension of the uniform range on the axis or greatest homogeneous area in the median plane of the field. In the Helmholtz case, for which the separation between the square coils is calculated to the 0,5445th part of the edge's lenght the volume with 1 %deviation from the field intensity in the centre is by 72 % larger than that of a usual Helmholtz coil of the same size.

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Sur la production des champs magnétiques homogènes de grand volume pour l'étude du comportement des compas magnétiques et des dispositifs de réglage par différentes latitudes magnétiques

Résumé Pour pouvoir produire des champs magnétiques faibles et homogènes on propose d'employer des bobines à cadres carrés qui en comparaison avec des bobines annulaires de la même grandeur offrent l'avantage d'une homogénéité supérieure du champ magnétique. La distribution du champ sur l'axe et dans le plan d'une bobine à cadre carré est indiquée. Pour l'emploi de deux bobines combinées à cadres carrés on montre de quelle manière on peut déterminer la distance optimale pour les cas où il est nécessaire de demander de la plus grande extension linéaire de la région homogène sur l'axe du champ ou de la plus grande aire homogène dans le plan central. En cas des bobines Helmholtz dont la distance pour des bobines à cadres carrés a été déterminé à la 0,5445^e partie de la longueur de l'arête, le volume homogène avec une déviation de 1 % de l'intensité en comparaison avec l'intensité du centre du champ dépasse de 72 % le volume d'une bobine Helmholtz de la même grandeur et du type usuel.

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New paleomagnetic results from Upper Cretaceous arc-type rocks from the northern and southern branches of the Neotethys ocean in Anatolia     

Cengiz Cinku  Mualla  Heller  Friedrich  Ustaömer  Timur 《International Journal of Earth Sciences》2017,106(7):2575-2592

International Journal of Earth Sciences - A paleomagnetic study of Cretaceous arc type rocks in the Central-Eastern Pontides and in the Southeastern Taurides investigates the tectonic and...  相似文献