共查询到18条相似文献，搜索用时 609 毫秒
1.
分析了影响磁通门磁变仪定向状态函数和经典磁变仪定向状态函数改变的因素，对磁通门磁变仪定向状态函数和经典磁变仪定向状态函数及其稳定性进行了比较，得出了有益的结论。 相似文献
2.
磁通门磁变仪定向状态函数的稳定性分析 总被引：4，自引：0，他引：4
朱兆才 《地震地磁观测与研究》2001,22(4):86-89
在地磁观测中 ,磁变仪的稳定性是基本要求。磁通门磁变仪的稳定性依赖于电子反馈、补偿线路的稳定性和磁通门磁变仪定向状态函数的稳定性。本文对后者进行讨论。1 磁通门磁变仪的定向要求磁通门磁变仪的定向就是使传感器线圈轴方向与被测磁场方向一致。设磁通门 3个探头线圈分别与定向方向 X、Y、Z间有微小差角 ,省略电子放大部分 ,忽略温度影响 ,有(周锦屏等 ,1 999)TX =X0 + SXn X=X + tanε* Y + tanβX* Z ( 1 )TY=Y0 + SYn Y=Y + tanδ* X + tanβY* Z ( 2 )TZ=Z0 + SZn Z-Z + tanθX* X + tanθY* Y ( 3 )其中 X0 ,Y0… 相似文献
3.
本文通过对 Ｄ 磁变仪的定向讨论和实验发现, Ｄ 磁变仪可在 Ｚ 仪等固定铁磁影响环境中, 直接用“扭头正反向对称法”定向, 且无须再做任何改正。其定向结果在某种意义上较在无磁环境中定向后再做 Ｚ 磁系等影响改正的方法可靠。 相似文献
4.
本文对磁通门磁变仪定向标准、定向稳定性、影响定向的因素进行了分析，将定向标准分为定向操作标准和定向期望标准，讨论了实际记录精度等问题。 相似文献
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分析了磁通门磁变仪定向状态函数对电磁转换函数测定位的影响，指出在利用转换函数分析预报地震时，定向状态函数的影响不容忽视。 相似文献
8.
叶富华 《地震地磁观测与研究》1997,18(1):75-76
Ｈ磁变仪的定向讨论叶富华（中国四川６１１７３０成都地震台）通常认为，Ｈ磁变仪（以下简称Ｈ仪）的精确定向应是在没有Ｚ磁系等铁磁物质影响的所谓无磁环境中，用“扭头带动镜面法”（简称镜面法）定向，然后再做Ｚ仪的影响改正。在实际工作中，Ｈ仪需要重新定向的情况... 相似文献
9.
对磁通门磁变仪状态函数的测定方法进行了研究，提出了磁通门磁变仪标度值——状态函数的测定和磁通门磁变仪记录的校正计算方法。 相似文献
10.
对磁通门磁变仪和经典光记录磁变仪记录进行比较分析。认为可以用磁通门磁变仪记录和处理日常数据。用经典磁变仪来判断和改正磁通门磁变仪的记录错误。 相似文献
11.
SMALL项目数字化地磁资料可靠性分析 总被引：4，自引：1，他引：3
在对中美合作 SMALL (中国低纬地磁台阵 )项目安装在北京地磁台 (白家疃 )和云南通海地磁台的磁通门磁力仪记录资料与磁变仪模拟记录资料进行了详细的对比分析后 ,得出的结果表明 ,两者的日变形态、日变幅有较好的一致性 ,所选特定事件的变化幅度非常一致 ,说明磁通门磁力仪记录到的变化磁场的资料是真实可靠的。尽管目前磁通门磁力仪的基线值存在温度影响和离散度较大的问题 ,但随温度变化有明显的规律性 ,若能采取改进观测条件和观测方法以及缩短观测时间等措施 ,并对基线值进温度校正 ,磁通门磁力仪完全可以提供长期连续可靠的资料。而其为地震预报 ,空间环境预报 ,为日地物理 ,空间物理和地磁学的研究提供的高精度、高分辨率、连续可靠的数字化变化磁场资料是磁变仪模拟记录无法比拟的。 相似文献
12.
分量质子旋进磁力仪定向方法的研究 总被引：1，自引：0，他引：1
朱兆才 《地震地磁观测与研究》2000,21(5):16-20
根据分量质子旋进磁力仪补偿线圈电流允许误差 ,补偿线圈轴定向应满足的关系式和给出的允许误差 ,研究并给出了实现分量质子旋进磁力仪各定向标准的实用方法。 相似文献
13.
Optically pumped vapour magnetometers have an orientation dependency in measuring the scalar component of the ambient magnetic field which leads to challenges for integration with mobile platforms. Quantifying the three-dimensional attitude variations (yaw, pitch and roll) of an optically pumped vapour magnetometer, while in-flight and suspended underneath a rotary unmanned aerial vehicle, aids in the successful development of reliable, high-resolution unmanned aerial vehicle magnetometry surveys. This study investigates the in-flight three-dimensional attitude characteristics of a GEM Systems Inc. GSMP-35U potassium vapour magnetometer suspended 3 m underneath a Dà-Jiāng Innovations S900 multi-rotor unmanned aerial vehicle. A series of unmanned aerial vehicle-borne attitude surveys quantified the three-dimensional attitude variations that a simulated magnetometer payload experienced while freely (or semi-rigidly) suspended underneath the unmanned aerial vehicle in fair weather. Analysis of the compiled yaw, pitch and roll data resulted in the design of a specialized semi-rigid magnetometer mount, implemented to limit magnetometer rotation about the yaw axis. A subsequent unmanned aerial vehicle-borne magnetic survey applying this specialized mount resulted in more than 99% of gathered GSMP-35U magnetic data being within industry standards. Overall, this study validates that maintaining magnetometer attitude variations within quantified limits (±5° yaw, ±10° pitch and roll) during flight can yield reliable, continuous and high-resolution unmanned aerial vehicle-borne magnetic measurements. 相似文献
14.
成都地磁台绝对观测系统分析 总被引：1，自引：1，他引：1
对成都地磁台绝对观测仪器的配置情况作了简要介绍。对数字化地磁绝对观测仪器(DI磁通门经纬仪)和模拟观测仪器(GSI)的理论与实际观测精度作了对比分析。认为CTM—DI磁通门经纬仪与GSI一等磁力仪观测结果一致性较好。数字化仪器优于模拟仪器，并对DI仪的工作状况作了总结。 相似文献
15.
使用长周期大地电磁测深网 (Network -MT)等技术 ,在长春和三岔河等地对太平洋板块弧后的上地幔电导率结构进行了探测。用陆地电话线或电缆接收长基线的电场 ,由设置在长春地磁台的三分量磁通门磁力仪记录磁场变化 ,得到Network -MT等观测资料的最长周期可达 10 5～10 6 s,反演结果的深度可达约 10 0 0km。 1)在两个区的 10 0～ 2 0 0 ,30 0 ,50 0～ 6 0 0km深度附近存在电性间断面 ;2 )长春测区的 850km深度存在电性间断面 ;3)平滑模型的电导率随深度增大而单调增加 ;4 )三岔河测区 6 0 0km深度、长春测区 850km深度的电导率达到 1S/m。上述结果表明 ,地幔内存在不连续界面和不均匀性 ,有些结果可与岩石学的研究结果对比 相似文献
16.
Kyle R. Murphy Ian R. Mann I. Jonathan Rae David K. Milling 《Journal of Atmospheric and Solar》2011,73(11-12):1500-1510
Utilising fifteen (1990–2005) years of ground-based magnetometer data from four magnetometer stations, we characterise the statistical dependence of the Pc5 ULF wave power spectra on variations in F10.7 solar radio flux and on solar cycle phase. We show that the median Pc5 ULF wave power spectra can be characterised as a power-law with a localised Gaussian centred at a specific frequency superimposed on the power-law spectrum. Further, we demonstrate that the location of the Gaussian in frequency systematically varies with both solar cycle phase and F10.7 and is more pronounced during high-speed solar wind intervals. We postulate that the localised power spectrum enhancement (or Gaussian) is a manifestation of the local eigenfrequency of field line resonances in the Earth's magnetosphere and that the variation in the location of the Gaussian occurs as a result of increased ionospheric outflow during periods of enhanced F10.7 and active solar activity. 相似文献
17.
A multipoint study of a substorm occurring on 7 December, 1992, and its theoretical implications 总被引：1，自引：0，他引：1
N. J. Fox S. W. H. Cowley V. N. Davda G. Enno E. Friis-Christensen R. A. Greenwald M. R. Hairston M. Lester M. Lockwood H. Lühr D. K. Milling J. S. Murphree M. Pinnock G. D. Reeves 《Annales Geophysicae》1999,17(11):1369-1384
On 7 December 1992, a moderate substorm was observed by a variety of satellites and ground-based instruments. Ionospheric flows were monitored near dusk by the Goose Bay HF radar and near midnight by the EISCAT radar. The observed flows are compared here with magnetometer observations by the IMAGE array in Scandinavia and the two Greenland chains, the auroral distribution observed by Freja and the substorm cycle observations by the SABRE radar, the SAMNET magnetometer array and LANL geosynchronous satellites. Data from Galileo Earth-encounter II are used to estimate the IMF Bz component. The data presented show that the substorm onset electrojet at midnight was confined to closed field lines equatorward of the pre-existing convection reversal boundaries observed in the dusk and midnight regions. No evidence of substantial closure of open flux was detected following this substorm onset. Indeed the convection reversal boundary on the duskside continued to expand equatorward after onset due to the continued presence of strong southward IMF, such that growth and expansion phase features were simultaneously present. Clear indications of closure of open flux were not observed until a subsequent substorm intensification 25 min after the initial onset. After this time, the substorm auroral bulge in the nightside hours propagated well poleward of the pre-existing convection reversal boundary, and strong flow perturbations were observed by the Goose Bay radar, indicative of flows driven by reconnection in the tail. 相似文献
18.
A flux transfer event observed at the magnetopause by the Equator-S spacecraft and in the ionosphere by the CUTLASS HF radar 总被引：2，自引：0，他引：2
D. A. Neudegg T. K. Yeoman S. W. H. Cowley G. Provan G. Haerendel W. Baumjohann U. Auster K.-H. Fornacon E. Georgescu C. J. Owen 《Annales Geophysicae》1999,17(6):707-711
Observations of a flux transfer event (FTE) have been made simultaneously by the Equator-S spacecraft near the dayside magnetopause whilst corresponding transient plasma flows were seen in the near-conjugate polar ionosphere by the CUTLASS Finland HF radar. Prior to the occurrence of the FTE, the magnetometer on the WIND spacecraft ≈226 RE upstream of the Earth in the solar wind detected a southward turning of the interplanetary magnetic field (IMF) which is estimated to have reached the subsolar magnetopause ≈77 min later. Shortly afterwards the Equator-S magnetometer observed a typical bipolar FTE signature in the magnetic field component normal to the magnetopause, just inside the magnetosphere. Almost simultaneously the CUTLASS Finland radar observed a strong transient flow in the F region plasma between 78° and 83° magnetic latitude, near the ionospheric region predicted to map along geomagnetic field lines to the spacecraft. The flow signature (and the data set as a whole) is found to be fully consistent with the view that the FTE was formed by a burst of magnetopause reconnection. 相似文献