排序方式: 共有8条查询结果,搜索用时 187 毫秒
1
1.
Karl-Heinz Glassmeier Ingo Richter Andrea Diedrich Günter Musmann Uli Auster Uwe Motschmann Andre Balogh Chris Carr Emanuele Cupido Andrew Coates Martin Rother Konrad Schwingenschuh Karoly Szegö Bruce Tsurutani 《Space Science Reviews》2007,128(1-4):649-670
The fluxgate magnetometer experiment onboard the ROSETTA spacecraft aims to measure the magnetic field in the interaction
region of the solar wind plasma with comet 67P/Churyumov-Gerasimenko. It consists of a system of two ultra light (about 28
g each ) triaxial fluxgate magnetometer sensors, mounted on the 1.5 m long spacecraft boom. The measurement range of each
sensor is ±16384 nT with quantization steps of 31 pT. The magnetometer sensors are operated with a time resolution of up to
0.05 s, corresponding to a bandwidth of 0–10 Hz. This performance of the RPC-MAG sensors allows detailed analyses of magnetic
field variations in the cometary environment. RPC-MAG furthermore is designed to study possible remnant magnetic fields of
the nucleus, measurements which will be done in close cooperation with the ROSETTA lander magnetometer experiment ROMAP. 相似文献
2.
3.
4.
三轴磁通门传感器在军事和民用领域应用广泛,但由于其存在三轴非正交、零偏和标度系数不一致的问题,导致其存在转向差,影响了其磁测精度。首先,分析了转向差的产生机理,建立了误差模型,通过最小二乘法估算出了误差参数,进而对磁测数据进行了转向差校正。仿真计算表明,该算法对误差参数估算准确,对磁场分量和总场模值均有较好的校正效果,证明了算法的有效性。在磁场测量实验中,利用该算法估算出了传感器的误差参数,并对实测磁场数据进行了校正。校正后,数据的转向差得到了明显抑制,提高了三轴磁通门传感器的测量精度。 相似文献
5.
6.
火星磁场测量是国际火星探测任务的焦点之一,中国首次火星磁测任务通过在巡视器(即火星车)和环绕器上同时搭载磁强计,实现对火星磁场的火–空联合观测。巡视器磁强计载荷选用双探头三轴磁通门磁强计,采用亥姆霍兹补偿线圈型探头技术和全数字闭环反馈电路技术,实现空间磁场的高精度同点测量。单机在设计上考虑了可靠性安全性设计和空间环境适应性设计。经地面标定,单机量程可达到±6.5万nT,噪声水平优于0.01 nT/√Hz,分辨率达到了0.01 nT。 相似文献
7.
H. U. Auster I. Apathy G. Berghofer A. Remizov R. Roll K. H. Fornacon K. H. Glassmeier G. Haerendel I. Hejja E. Kührt W. Magnes D. Moehlmann U. Motschmann I. Richter H. Rosenbauer C. T. Russell J. Rustenbach K. Sauer K. Schwingenschuh I. Szemerey R. Waesch 《Space Science Reviews》2007,128(1-4):221-240
The scientific objectives, design and capabilities of the Rosetta Lander’s ROMAP instrument are presented. ROMAP’s main scientific
goals are longterm magnetic field and plasma measurements of the surface of Comet 67P/Churyumov-Gerasimenko in order to study
cometary activity as a function of heliocentric distance, and measurements during the Lander’s descent to investigate the
structure of the comet’s remanent magnetisation. The ROMAP fluxgate magnetometer, electrostatic analyser and Faraday cup measure
the magnetic field from 0 to 32 Hz, ions of up to 8000 keV and electrons of up to 4200 keV. Additional two types of pressure
sensors – Penning and Minipirani – cover a pressure range from 10−8 to 101 mbar. ROMAP’s sensors and electronics are highly integrated, as required by a combined field/plasma instrument with less
than 1 W power consumption and 1 kg mass. 相似文献
8.
磁场测量是深空探测的重要任务之一,通过磁场可以遥感行星内部、研究行星演化历史、认知太阳系天体空间环境。基于法拉第电磁感应原理的磁通门磁强计,因空间适应性强、技术成熟度高、可靠性高等特点,是深空磁场测量最为常用的载荷。简要描述了磁通门磁强计的基本测量原理,探讨了地面和在轨标定的原理和实施方法,并介绍了磁强计在空间任务中的应用方式。目前,我国已经具备了星载高精度磁通门磁强计的研制能力。在不久的将来,磁通门磁强计有望在深空探测任务中发挥重要作用。 相似文献
1