贝尔直升机航磁仪磁补偿结果分析

贝尔直升机采用固定式安装氦光泵磁力仪的方案。对磁探杆进行改进设计后,使用GB-10型氦光泵磁力仪和16项自动磁补偿器用于航磁测量。给出磁补偿前后氦光泵磁力仪的输出结果对比。分析补偿前后的数据,对磁补偿器改进设计及机动飞行方法提出建议。     

兴凯湖沉积物磁化率和色度反映的28kaBP以来区域古气候环境演化

对兴凯湖长269 cm的沉积岩心的研究结果显示:沉积物的色度和磁化率特征可以较好地反映区域气候环境变化。沉积物明度分别与红度、磁化率、黏土和有机质含量之间及磁化率与黏土之间有很好的相关性;红度高值与明度低值对应暖湿气候环境,磁化率低值反映沉积物较粗的较低湖面,对应冷干气候。28480~26160 cal.aBP,湖区处于温湿气候时期;22880~18170 cal.aBP,岩心孢粉浓度很低,流域处于末次盛冰期疏桦林草原环境;18170~12650 cal.aBP处于Bφlling/Older Dryas/Allerφd暖期。岩心深度90~78 cm段,对应于新仙女木期;11500~4570 cal.aBP,进入全新世暖期,其中8000~5000 cal.aBP,本区处于全新世大暖期(气候适宜期);4570~1470 cal.aBP气候变为凉干;1470 cal.aBP以来,流域又变为暖湿气候环境,同时,人类活动逐渐增强造成水土流失加剧。     

Effect of superstrong magnetic field on electron screening at the crusts of neutron stars

The influences of electron screening (ES) and electron energy correction (EEC) are investigated by superstrong magnetic field (SMF). We also discuss in detail the discrepant factor between our results and those of Fushiki, Gudmundsson and Pethick (FGP) in SMF. The results show that SMF has only a slight effect on ES when B < 10⁹ T on the surfaces of most neutron stars. Whereas for some magnetars, SMF influence ES greatly when B > 10⁹ T . For instance, due to SMF the ES potential may be increased about 23.6% and the EEC may be increased about 4 orders of magnitude at ρ/μ_e = 1.0×10⁶ mol/cm³ and T₉ = 1. On the other hand, the discrepant factor shows that our results are in good agreement with FGP's when B < 10⁹ T . But the difference will be increased with increasing SMF.     

Effect of strong magnetic field on chemical potential and electron capture in magnetar

The chemical potential of electrons in a strong magnetic field is investigated. It is shown that the magnetic field has only a slight effect on electron chemical potential when B<10¹¹ T, but electron chemical potential will decrease greatly when B>10¹¹ T. The effects of a strong magnetic field on electron capture rates for ⁶⁰Fe are discussed, and the result shows that the electron capture sharply decreases because of the strong magnetic field.     

冲绳海槽北段的重磁场特征及地质意义

１９９２年之前,国内对冲绳海槽的调查研究主要集中在海槽的中部和南部,而对其北段的调查研究工作却很少。根据实测的重磁异常,较深入地分析了海槽北段的地球物理场特征,构造活动地壳结构及应力状态,结果表明冲绳海槽北段同样具有强烈的地壳构造活动。     

水成沉积与风成沉积及古土壤的磁组构特征

晚第四纪水成沉积、风成沉积、古土壤等的磁组构研究表明,不同成因的沉积物具有明显不同的磁组构特征。一般地,水成沉积的体积磁化率Ｋ受物源和水动力因素控制,Ｐ和Ｆ均＞１．０２,ｑ＜０．５;风成沉积的Ｋ受物源控制,内陆黄土的Ｋ明显高于沿海黄土及海岸风沙Ｋ,Ｐ和Ｆ均＜１．０２,ｑ的平均值＞０．５５;古土壤的Ｋ受母质沉积类型和成土环境的氧化还原条件控制,内陆古土壤的Ｋ偏高,沿海古土壤的Ｋ偏低,内陆古土壤的Ｋ远高于沿海古土壤的Ｋ,Ｐ和Ｆ均＜１．０２,ｑ的平均值在０．５左右。运用典型沉积的磁组构特征对比分析未知沉积物,可以得到未知沉积物的物源、沉积过程和环境信息。     

Three-dimensional inversion of marine magnetic anomalies: Implications for crustal accretion along the Mid-Atlantic Ridge (28°–31°30′ N)

We present magnetic field data collected over the Mid-Atlantic Ridge in the vicinity of the Atlantis Fracture Zone and extending out to 10 Ma-old lithosphere. We calculated a magnetization distribution which accounts for the observed magnetic field by performing a three-dimensional inversion in the presence of bathymetry. Our results show the well-developed pattern of magnetic reversals over our study area. We observe a sharp decay in magnetization from the axis out to older lithosphere and we attribute this decay to progressive low temperature oxidation of basalt. In crust which is 10 Ma, we observe an abrupt increase in magnetic field intensity which could be due to an increase in the intensity of magnetization or thickness of the magnetic source layer. We demonstrate that because the reversal epoch was of unusually long duration, a two-layer model comprised of a shallow extrusive layer and a deeper intrusive layer with sloping polarity boundaries can account for the increase in the amplitude of anomaly 5. South of the Atlantis Fracture Zone, high magnetization is correlated with bathymethic troughts at segment end points and lower magnetization is associated with bathymetric highs at segment midpoints. This pattern can be explained by a relative thinning of the magnetic source layer toward the midpoint of the segment. Thickening of the source layer at segment endpoints due to alteration of lower oceanic crust could also cause this pattern. Because we do not observe this pattern north of the fracture zone, we suggest it is a result of the nature of crustal formation process where mantle upwelling is focused. South of the fracture zone, reversals along discontinuity traces only continue to crust 2 Ma old. In crust >2 Ma, we observe bands of high, positive magnetization along discontinuity traces. We suggest that within the discontinuity traces, a high, induced component of magnetization is produced by serpentinized lower crust/upper mantle and this masks the contribution of basalts to the magnetic anomaly signal.     

苏门答腊裂谷盆地带构造分带及其成藏模式

苏门答腊弧后裂谷盆地带是印尼乃至东南亚最大的油气产区,由于勘探程度高, 近十年来勘探成效差,盆地油气发现进入瓶颈期。为了指明苏门答腊弧后裂谷盆地带勘探方向,以盆地带构造演化为主线,以构造带为研究对象,在构造特征、构造对成藏模式控制作用等多方面研究的基础上,预测了苏门答腊盆地带有利勘探领域。根据构造特征分析,苏门答腊弧后裂谷盆地带可划分为近岛弧带、中央反转带和远岛弧带3个构造带。近岛弧带以继承性隆起为构造特征,油气主要通过断裂垂向运移,聚集在局部构造高部位生物礁和背斜之中,近岛弧带为旁生侧储型成藏模式,基底潜山圈闭是近岛弧带未来的勘探方向;中央反转带构造样式为挤压反转的半地堑、铲式正断层,中央反转带油气来自底部深凹陷,上部多层系做储层,垂向断层或侧向砂体发育,沟通烃源岩与圈闭,具有近水楼台的优势成藏条件,为下生上储型成藏模式,该带基底潜山圈闭和源内构造—岩性圈闭也具有较好的烃—运—储匹配关系,可能形成好的油气藏;远岛弧带以单斜构造背景为主,局部发育深洼陷,远岛弧带局部洼陷具有一定的生烃能力,该构造带钻井揭示了地层超覆油气藏,但目前勘探程度较低,尚存在较大勘探潜力。     

地磁日变测量系统便携化方案研究

分析目前海洋磁力测量时,采用G88X系列海洋磁力仪的地磁日变测量系统存在功耗高、体积大、质量重等问题。通过对磁力仪、电缆、数据采集计算机、UPS等各个部件的改装、改造、替换构思,提出一套完整的便携化方案,使整套系统的功耗、体积、质量均显著降低,从而实现系统便携化。     

太阳静日变化的特征分析

根据北京明陵地磁台2010年观测数据,采用磁静日数据,选用其特征值——日变幅度和相位,对太阳静日变化特征进行了初步分析,并用调和分析方法将其分解为3个周期的谐波分量。对地磁数据的分析处理具有一定的参考价值。