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’97全国古地磁学、环境磁学与岩石磁学学术会议于1997年10月30日至11月3日在上海华东师范大学举行,河口海岸国家重点实验室承办了这次会议．来自全国35个科研单位、大专院校和生产部门62位代表参加了会议．会议收到论文60篇,有28位代表就30个专题作了学术报告,内容丰富,涉及构造磁学、磁性地层学、岩石磁学、环境磁学、土壤磁学及测磁仪器和实验方法等．这些论文反映了近年来我国在上述领域研究工作的最新进展和成果．其中,中国黄土低温剩磁测量与热磁研究及其古气候意义、中国南方海相石灰岩的岩石磁学研究、南黄海冰消期以来环境磁… 相似文献
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苏联地球物理学家沙佩罗(V.A.Shapi-ro)教授应邀于1990年10月25日至11月1日访问了国家地震局地球物理研究所。沙佩罗教授现任苏联地磁学科学委员会委员、构造地磁学工作组组长、苏联科学院乌拉尔分院地球物理研究所地磁学与磁力仪科学实验室主任。他领导的地磁学与磁力仪科学实验室现有科技人员24名,分5个组,分别研究地磁异常场、构造磁学(震磁效应与地震前兆)与地磁异常场的动力学、古地磁学、磁层来源的地磁场、地磁台站与地磁长期变化等。在访问期间,沙佩罗教授与国家地震局地 相似文献
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四川旺苍地区中三叠世雷口坡组重磁化机理初步研究 总被引：1，自引：0，他引：1
对四川北部旺苍地区中三叠世雷口坡组进行了古地磁学和岩石磁学研究,结果表明,主要载磁矿物为多畴磁铁矿和磁赤铁矿,所携带的特征剩磁在地理坐标下与近代地磁场方向接近,可能是由于后期白云岩化作用和热粘滞剩磁引起的重磁化所致. 相似文献
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四川旺苍早三叠世古地磁学结果及其大地构造学意义 总被引：4，自引：0，他引：4
对四川北部旺苍地区(32.14°106.17°)早三叠世地层进行了古地磁学和岩石磁学研究,其结果表明剩磁载磁矿物主要为磁铁矿,另有少量赤铁矿.采样地层岩石高温剩磁分量(D=45.1°,I=18.0°,a_(95)5. 9°),通过褶皱及倒转检验,表明认岩石中获得的高温分量为原生分量.由原生分量求得扬子地块早三叠世虚地磁极为:42.5°N,214.6°E(d_(p)=3.2,d_m=6.1),古纬度为9.2°.认为,华北与扬子地块在自早三叠世期间已基本拼合,现有古地磁结果支持秦岭造山带为陆内造山作用的结果 相似文献
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本文对密云水库表层沉积物中的磁性矿物进行了岩石磁学和透射电子显微学的综合研究.本实验建立的磁选方法实现将70%~85%左右的磁性矿物从沉积物中分离出来.岩石磁学研究表明,密云水库沉积物中的磁性矿物以多畴和单畴磁铁矿为主,还含有少量高矫顽力弱磁性载磁矿物(可能为赤铁矿).对磁选矿物的透射电镜观测表明,样品中部分单畴磁铁矿具有纳米尺寸和化学纯度高等特点,为拉长的立方-八面体磁铁矿,是趋磁细菌产生的化石磁小体;多畴磁铁矿多数具有微米尺寸,形状不规则,为碎屑成因;超顺磁磁铁矿粒径约为5~20nm,且含硅、铝等元素,可能为自生成因.研究结果表明,岩石磁学和透射电子显微学的综合应用可以更全面、准确地分析沉积物中磁性矿物的成分、含量、粒径和化学成分等信息,为环境磁学、生物地磁学和古地磁学研究提供依据. 相似文献
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英国第五届地球物理学年会于1981年4月6日至9日在剑桥大学新卡文迪什实验室(NewCavendish Laboratory)召开,约有300名科学工作者参加。在年会上有160余篇报告分别在三个讲演室进行,其内容分为12个部分:①地壳的演化;②地震及新构造;③数学地球物理学;④地磁学;⑤包括新的仪器技术的海洋研究;⑥反射和折射地震学;⑦古地磁学;⑧热 相似文献
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本文对四川北部旺苍-南江地区晚侏罗世蓬莱镇组进行了较为详细的岩石磁学和古地磁学研究．逐步热退磁揭示出蓬莱镇组岩石所携带的剩磁由两个分量组成,其中低温组分（次生剩磁）的解阻温度低于420℃;高温组分（特征分量）可通过褶皱及倒转检验,由此求得磁偏角和磁倾角分别为18．4°和29．3°（构造校正后）,95％置信回（α95）为8．5°,对应的古地磁极经纬度分别为236．4°E和66．6°N．基于古地磁结果,并结合已有的地质证据,提出根据古地磁学确定的扬子地块晚侏罗世古纬度偏低的原因可能是由真极移造成的． 相似文献
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本文对四川北部旺苍-南江地区晚侏罗世蓬莱镇组进行了较为详细的岩石磁学和古地磁学研究．逐步热退磁揭示出蓬莱镇组岩石所携带的剩磁由两个分量组成,其中低温组分（次生剩磁）的解阻温度低于420℃;高温组分（特征分量）可通过褶皱及倒转检验,由此求得磁偏角和磁倾角分别为18．4°和29．3°（构造校正后）,95％置信回（α95）为8．5°,对应的古地磁极经纬度分别为236．4°E和66．6°N．基于古地磁结果,并结合已有的地质证据,提出根据古地磁学确定的扬子地块晚侏罗世古纬度偏低的原因可能是由真极移造成的． 相似文献
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Matasova G. G. Kazansky A. Yu. Shchetnikov A. A. Erbajeva M. A. Filinov I. A. 《Izvestiya Physics of the Solid Earth》2020,56(3):392-412
Izvestiya, Physics of the Solid Earth - Abstract—An integrated study combining laser granulometry, rock-magnetic, and paleomagnetic investigations is conducted for the deposits of the Tologoi... 相似文献
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Rafael García-Ruiz Avto Goguitchaichvili Miguel Cervantes-Solano Juan Morales Rafael Maciel-Peña José Rosas-Elguera Ruben Cejudo-Ruiz Jaime Urrutia-Fucugauchi 《Studia Geophysica et Geodaetica》2017,61(2):249-263
A rock magnetic and paleomagnetic investigation was performed on some selected, radiometrically dated lava flows from the Mascota Volcanic Field (MVF), western Trans- Mexican Volcanic Belt. A set of rock-magnetic experiments and standard paleomagnetic analysis were carried out on 19 sites spanning the time interval from 2268 to 72 kyr. The paleomagnetic directions are anchored to absolute radiometric ages while no such information was available in previous studies. This makes possible to correctly evaluate the fluctuation of Earth’s magnetic field from Pliocene to Pleistocene and reveal the firm evidence of possible Levantine excursion. Both Ti-poor and Ti-rich titanomagnetites seem to carry the remanent magnetization with Curie temperatures ranging from 350°C to 537°C. Thirteen flows correspond to the Brunhes chron, one of them exhibits transitional directions, while the remaining six sites belong to the Matuyama chron. New and existing dataset for MVF were used to estimate the paleosecular variation parameters. The selected data include 35 Plio-Quaternary lava flows. After excluding the poor quality data, as well as the transitional directions, the mean paleodeclination is 356.1° and oaleoinclination 39.9°, which agree well with the geocentric axial dipole (GAD) and the expected paleodirections for the Plio-Pleistocene, as derived from the reference poles for the stable North America. The corresponding mean paleomagnetic poles are paleolongitude 226.7° and paleolatitude 86.0°. The virtual geomagnetic pole scatter for the MVF is 15.2°, which is consistent with the value expected from model G at latitude of 20° (this model provides an interpretation of the paleosecular variation at different latitudes for the time of interest). The combined paleomagnetic data, supported by positive reversal test, indicate no paleomagnetically detectable vertical-axis rotations in the study area. The evidence of one transitional directions was detected, which may correspond to the Levantine excursion (360-370 kyr) or unnamed event between 400-420 kyr. 相似文献
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Miguel Cervantes-Solano Lisa Kapper Avto Goguitchaichvili Vicente Carlos Ruiz-Martínez José Rosas-Elguera Juan Morales Rafael Maciel-Peña Rubén Cejudo-Ruiz 《Studia Geophysica et Geodaetica》2017,61(2):233-248
We present a detailed rock-magnetic and paleomagnetic survey from Autlan volcanic succession in western Mexico. The principal aim of this study is to extend paleomagnetic data from Autlan lavas in order to confirm vertical-axis rotation observed in reconnaissance study and to evaluate long-term variation of the geomagnetic field strength based on existing and global data. The mean inclination (44.7°) is in agreement with the expected inclination for 60 and 70 Ma, as derived from available reference poles for the North American craton. The declination (333.6°), however, is significantly different from those expected, which suggests a statistically significant counterclockwise tectonic rotation ranging between 10° ± 6° and 14° ± 7°. As a measure of paleosecular variation (PSV), we obtained a geomagnetic field dispersion of 9.6° (upper and lower limits: 7.2°–11.9°) in perfect agreement with the previously published PSV compilation of selected Cretaceous data from lavas. The mean virtual dipole moments available for Autlan lavas are about 65% of the present geomagnetic axial dipole but are in reasonably good agreement with other comparable quality determinations between 5 and 90 Ma. This reinforces the hypothesis that low geomagnetic field strengths persisted for the entire Jurassic extending into the Upper Cretaceous. 相似文献
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Miguel Cervantes Solano Avto Goguitchaichvili Leda Sánchez Bettucci Ruben Cejudo Ruiz Manuel Calvo-Rathert Vicente Carlos Ruiz-Martinez Ruth Soto Luis M. Alva-Valdivia 《Studia Geophysica et Geodaetica》2010,54(4):533-546
We report detailed rock-magnetic and paleomagnetic directional data from 35 lava flows (302 standard paleomagnetic cores)
sampled in the Central-Northern region of Uruguay in order to contribute to the study of the paleosecular variation of the
Earth’s magnetic field during early Cretaceous and to obtain precise Cretaceous paleomagnetic pole positions for stable South
America. The average unit direction is rather precisely determined from 29 out of 35 sites. All A95 confidence angles are less than 8°, which points to small within-site dispersion and high directional stability. Normal polarity
magnetizations are revealed for 19 sites and 10 are reversely magnetized. Two other sites yield well defined intermediate
polarities. The mean direction, supported by a positive reversal test is in reasonably good agreement with the expected paleodirection
for Early Cretaceous stable South America and in disagreement with a 10° clockwise rotation found in the previous studies.
On the other hand, paleomagnetic poles are significantly different from the pole position suggested by hotspot reconstructions,
which may be due to true polar wander or the hotspot motion. Our data suggest a different style of secular variation during
(and just before) the Cretaceous Normal Superchron and the last 5 Ma, supporting a link between paleosecular variation and
reversal frequency. 相似文献
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An integrated paleomagnetic study of Rio Grande de Santiago volcanic succession (trans-Mexican volcanic belt): revisited 总被引：1，自引：0，他引：1
Avto Goguitchaichvili Luis Alva-Valdivia Jose Rosas-Elguera Jaime Urrutia-Fucugauchi Jose Antonio Gonzalez Juan Morales Jesus Sol 《Physics of the Earth and Planetary Interiors》2002,130(3-4):175-194
We carried out an integrated paleomagnetic, rock-magnetic and paleointensity study of Miocene volcanic succession from the trans-Mexican volcanic belt (TMVB) north of Guadalajara. A total of 37 consecutive basaltic lava flows (326 oriented standard paleomagnetic cores) were collected at Lazo locality. Continuous susceptibility measurements with temperature and hysteresis experiments yield in most cases reasonably reversible curves with Curie points close to that of pseudo-single-domain magnetite. Two geomagnetic reversals were observed in the 300 m thick composite section. Paleosecular variation was lower than the one observed in general during Miocene. It appears that the volcanic units have been emplaced during a relatively short time span of about 1 Ma. The mean paleomagnetic directions obtained from this study do not differ significantly from that expected for the middle Miocene. The mean paleomagnetic direction calculated from all data is I=31.1°, D=354.6°, k=124 and 95=2.1°, N=37. Seventy-two samples with apparently preserved primary magnetic mineralogy and without secondary magnetization, mostly belonging to reverse polarity chron were pre-selected for Thellier paleointensity determination. The flow-mean paleointensity values are ranging from 22.4±3.4 to 53.8±6.0 μT and the corresponding virtual dipole moments (VDMs) are ranging from (5.4±0.8) to (12.0±1.4)×1022 A m2. This corresponds to mean value of (7.7±2.2)×1022 A m2, which is close to present day geomagnetic field strength. Altogether, our data suggest the existence of relatively high geomagnetic field strength undergoing low fluctuations. 相似文献
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Jose Rosas-Elguera Bertha Aguilar Reyes Avto Goguitchaichvili Macario Rocha Margarita López Martínez Miriam M. Tostado-Plascencia Luis M. Alva Valdivia Cecilia Caballero Miranda 《Studia Geophysica et Geodaetica》2011,55(2):265-278
For long time the western-central Mexico has been affected by oblique subduction caused by Farallon plate beneath North America.
As result, smaller plates (e.g. Cocos Plate), several fault systems outlining crustal blocks (e.g. Michoacán block) and magmatic
arcs (e.g. Paleocene-Early Oligocene magmatism and the Trans-Mexican Volcanic Belt) were developed. Still, no paleomagnetic
data are available for Oligocene and Miocene. The principal aim of this study is to evaluate whether the tectonic rotations
and relative motions of these blocks occurred before the Miocene. Here, we report a detailed rock-magnetic and paleomagnetic
results from Tecalitlan area, located in the Michoacán block. Sixteen sites (about 150 oriented samples) were collected including
one radiometrically dated diabase dike (35.0 ± 1.8 Ma). Rock-magnetic experiments permitted identification of magnetic carriers
and assessment of the paleomagnetic stability. Continuous susceptibility measurements vs temperature in most cases yield reasonably
reversible curves with Curie points close to that of magnetite. Reliable paleomagnetic directions were obtained for 12 sites.
Inclination I and declination D of the mean paleomagnetic direction obtained in this study are I = 33.1°, D = 345.0°, and
Fisherian statistical parameters are k = 25, α95 = 8.9°. The corresponding mean paleomagnetic pole position is Plat = 75.7°, Plong = 166.6°, K = 31, A95 = 8.0°. The mean inclination is in reasonably good agreement with the expected value, as derived from reference poles for
the stable North America. Magnetic declination is not significantly different from that expected which is in disagreement
with a counterclockwise tectonic rotation of about 20° previously reported for the studied area. Based on paleomagnetic results
obtained in this study compiled with those currently available from the Michoacán Block, we propose a simple model suggesting
that sometime in Eocene epoch the convergence vector of the Farallon plate relative to North America plate was normal to the
trench before reaching an actual oblique convergence. 相似文献
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蛇绿岩中枕状玄武岩的古地磁学研究可为古海洋的恢复与演化提供定量化依据.黑龙江省饶河地区中侏罗世枕状玄武岩的岩石学、岩石磁学研究表明,该岩石具备水下喷出特点,发育辉长结构,载磁矿物为磁铁矿.17个采点181块样品的热退磁实验表明,中侏罗世枕状玄武岩记录了高温分量和中温分量,前者为熔岩喷发记录的原生剩磁方向,平均方向D/I=59.4°/46.3°,α95=6.8°,对应的极位置为40.3°N,224.6°E,A95=7°;后者可能为晚侏罗世—早白垩世岩浆热事件的叠加,平均方向D/I=55.4°/60.6°,α95=3.9°,对应的极位置为50.8°N,210.6°E,A95=5.2°.综合考虑区域地质背景,将这一结果与邻区同时代的古地磁数据对比,推测在中侏罗世之前,在饶河杂岩与佳木斯地体之间存在一定规模的海域,与现今日本海相似;早白垩世时期,该海域封闭,饶河杂岩与华北、西伯利亚板块在动力学上已成为整体. 相似文献
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Genrietta A. Pospelova Elżbieta Król Galina M. Levkovskaya Jadwiga Kruczyk Magdalena Kądziałko-Hofmokl Sergey A. Kulakov 《Acta Geophysica》2007,55(4):619-639
The paper presents the results of experimental rock-magnetic, paleomagnetic and palynologic study of Paleolithic sediments
sampled along two profiles in the Akhshtyrskaya cave, situated in the vicinity of Black Sea shore. In the upper part of profiles,
some magnetite was observed; in the middle and lower parts, strongly oxidized non-stoichiometric magnetite and hematite prevail.
Thin maghemite covers on the surface of fine magnetite grains are present in the majority of specimens. Natural remanence
has one characteristic component (CHRM), mostly of chemical origin, although in few specimens containing magnetite it may
be sedimentary. Directions of CHRM obtained by standard paleomagnetic methods revealed anomalous pattern only in layer 3/2,
which is slightly older than the overlying layer 3/1 whose age was established as (35±2)×103 years BP by the U-Th method. This suggests that this paleomagnetic anomaly (PMA) can be correlated with Kargapolovo excursion
dated on about (45−39)×103 years BP. In the remaining overlying and underlying layers, directions of CHRM are grouped around the present geomagnetic
field. Depth distributions of scalar magnetic parameters generally coincide with the lithological division of the profiles.
Palynologic study revealed the presence of 22 pollen zones. Five thermomers separated with colder periods were found in the
middle and lower parts of profile. The non-magnetite composition of magnetic fraction of the majority of studied sediments
— oxidized nonstoichiometric magnetite and hematite — resulted in the lack of correlations between paleoclimatic and scalar
magnetic characteristics. 相似文献
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In order to establish the magnetic carriers and assess the reliability of previous paleomagnetic results obtained for Eocene marine marls from the south Pyrenean basin, we carried out a combined paleo- and rock-magnetic study of the Pamplona-Arguis Formation, which crops out in the western sector of the southern Pyrenees (N Spain). The unblocking temperatures suggest that the characteristic remanent magnetization (ChRM) is carried by magnetite and iron sulphides. The ChRM has both normal and reversed polarities regardless of whether it resides in magnetite or iron sulphides, and represents a primary Eocene magnetization acquired before folding. Rock magnetic results confirm the presence of magnetite and smaller amounts of magnetic iron sulphides, most likely pyrrhotite, in all the studied samples. Framboidal pyrite is ubiquitous in the marls and suggests that iron sulphides formed during early diagenesis under sulphate-reducing conditions. ChRM directions carried by magnetic iron sulphides are consistent with those recorded by magnetite. These observations suggest that magnetic iron sulphides carry a chemical remanent magnetization that coexists with a remanence residing in detrital magnetite. We suggest that the south Pyrenean Eocene marls are suitable for magnetostratigraphic and tectonic purposes but not for studies of polarity transitions, secular variations and geomagnetic excursions, because it is difficult to test for short time differences in remanence lock-in time for the two minerals. The presence of iron sulphide minerals contributing to the primary magnetization in Eocene marine marls reinforces the idea that these minerals can persist over long periods of time in the geological record. 相似文献