共查询到18条相似文献,搜索用时 359 毫秒
1.
2.
3.
为获取航空磁探中水下铁磁性目标的空间磁场分布,通过三维积分方程法的基本原理推导出空间磁场的解析式,根据矢量恒等式和高斯散度定理简化空间磁场计算式,建立水下铁磁性目标空间磁场预测模型。通过铁磁性长方体对模型进行理论验证,使用铯光泵磁力仪测量铁磁性长旋转椭球体的高空磁场;然后,基于预测模型推算铁磁性长旋转椭球体的磁场,根据实际测量的磁场数据和预测值进行比较。结果表明,预测模型的推算精度较高,平均绝对误差为0.320 5 nT,平均相对误差为12.368%。 相似文献
4.
在空间探测过程中,采用高灵敏无自旋交换弛豫(SERF)原子磁强计在行星表面进行磁场测量是原位物质成分分析的有效手段之一。为了提高SERF原子磁强计的磁场测量灵敏度,必须减小外界磁场扰动对其原子自旋SERF态质量的影响,基于SERF原子磁强计的测量原理,设计了一套主动磁补偿系统。首先,通过测量驱动激光光强获得3个方向的磁场信息;在此基础上,控制电流源和线圈主动产生一个与外界磁场扰动大小相同、方向相反的磁场来补偿扰动,以提高原子自旋SERF态的质量;最后,结合现有的SERF原子磁强计实验平台进行了实验验证。实验结果表明,与手动补偿方式相比,采用本文所述的主动磁补偿系统,可以实时跟踪磁场补偿点,降低系统信号的噪声,补偿了外界磁场的扰动,验证了磁强计主动磁补偿技术的有效性,为后续样机的研制奠定了技术基础。 相似文献
5.
固定翼无人机航磁探测系统的磁补偿模型分析 总被引:1,自引:0,他引:1
近年来,无人机的应用日益广泛,逐渐用于航空物探。在使用固定翼无人机搭载磁力仪进行航磁测量时,必然引入飞行平台干扰,包括与机动无关的干扰和与机动有关的干扰。去除和飞机机动有关的磁干扰,即为磁补偿工作。航磁补偿的经典TOLLES-LAWSON模型将磁干扰分为剩余磁场、感应磁场和涡流磁场。对于固定翼无人机,涡流磁场可以不考虑,将剩余磁场和感应磁场合称为稳态干扰场。主要对飞机干扰的来源和性质进行分析,并在地面设计实验验证铁磁性材料的性质,以加深对磁补偿模型的假设和推导过程的理解。最后,在地面实验平台上测量了飞机磁干扰场的平面分布图,指导航空磁力仪的安装。在将TOLLES-LAWSON模型应用于固定翼无人机航磁探测系统的磁补偿工作时,无人机与有人机相比,在结构和材料方面都有较大差异,因此对模型的物理意义和假设条件的深入理解至关重要,此即本文所述工作成果的出发点。 相似文献
6.
7.
8.
9.
环形磁铁空间磁场的解析计算与仿真 总被引:1,自引:0,他引:1
从永磁体的磁荷模型出发,运用标量磁位法、广义二项式定理、矢量叠加原理等建立了环形磁铁在磁体外部空间磁场分布的解析表达式,并在MATLAB仿真软件中进行了计算。利用三维数字式特斯拉计实际测量了两种规格的永磁体的磁场分布,利用Ansoft Maxwell电磁场分析软件建立了两种永磁体在磁体外部空间的磁场分布,通过对比解析计算结果、实际测量结果和Ansoft Maxwell仿真结果发现解析表达式很好地反映了永磁环空间磁场的分布规律,误差不超过7%,从而验证了解析表达式的正确性。 相似文献
10.
11.
12.
13.
14.
The Magnetostatic Cleanliness Program for the Cassini Spacecraft 总被引:3,自引:0,他引:3
The Cassini spacecraft, launched in October 1997 and expected to reach Saturn in 2004, carries two magnetometer experiments on a 10-m boom, one at the mid-section of the boom and the other situated at the end of the boom. In order to gather valid scientific magnetic field data and avoid electromagnetic interference, the spacecraft had to comply with stringent magnetostatic cleanliness requirements. This paper describes the results of the Cassini magnetics cleanliness program that achieved the goal of minimizing the magnetic field interference with Cassini’s DC magnetic field science instruments.This revised version was published online in July 2005 with a corrected cover date. 相似文献
15.
16.
17.
Lohr D. A. Zanetti L. J. Anderson B. J. Potemra T. A. Hayes J. R. Gold R. E. Henshaw R. M. Mobley F. F. Holland D. B. Acuña M. H. Scheifele J. L. 《Space Science Reviews》1997,82(1-2):255-281
The primary objective of the investigation is the search for a body-wide magnetic field of the near Earth asteroid Eros. The Near Earth Asteroid Rendezvous (NEAR) 3-axis fluxgate magnetometer includes a sensor mounted on the high-gain antenna feed structure. The NEAR Magnetic Facility Instrument (MFI) is a joint hardware effort between GSFC and APL. The design and magnetics approach achieved by the NEAR MFI effort entailed low-cost, up-front attention to engineering solutions which did not impact the schedule. The goal of the magnetometer is reliable magnetic field measurements within 5 nT, which necessitates the use of an extensive spacecraft magnetic interference model but is achievable with the full year's orbital data set. Such a goal has been shown viable with recent in-flight calibration data and comparisons to the WIND magnetometer data. The NEAR MFI effort has succeeded in providing magnetic field measurements for the first flight in NASA's Discovery line. 相似文献
18.
Direct measurements of the geomagnetic field have been made for more than 400 years, beginning with individual determinations of the angle between geographic and magnetic North. This was followed by the start of continuous time series of full vector measurements at geomagnetic observatories and the beginning of geomagnetic repeat stations surveys in the 19th century. In the second half of the 20th century, true global coverage with geomagnetic field measurements was accomplished by magnetometer payloads on low-Earth-orbiting satellites. This article describes the procedures and instruments for magnetic field measurements on ground and in space and covers geomagnetic observatories, repeat stations, automatic observatories, satellites and historic observations. Special emphasis is laid on the global network of geomagnetic observatories. 相似文献