共查询到19条相似文献,搜索用时 171 毫秒
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微弱磁场测量是研究物质特性和探索未知世界的重要手段之一。实现高精度的微弱磁场信号测量需要设计高精度的信号采集系统,而以模拟量输出的磁强计通常需要数字采集系统进行模/数转换。为此,文章设计开发基于Σ-Δ型模/数转换器(ADC)的高精度微弱磁场信号采集系统,包括系统硬件电路设计和系统核心控制器FPGA的功能设计,实现了FPGA对ADC的读写控制,以及ADC输出数据的接收和发送等。性能测试结果表明,该系统的有效采样位数可接近理论值(21位),输出噪声RMS值为1.9μV,磁场测量精度满足0.1 nT要求。 相似文献
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磁场重联是空间等离子体环境中的重要物理过程。对磁场重联进行深入研究,于空间灾害预报以及各种空间探测活动而言都有重要意义。文章首先回顾磁场重联研究史中的几个重要模型;然后介绍国际上进行磁场重联地面实验的主要等离子体装置及有关实验研究;最后介绍国内磁场重联实验研究的现状,重点介绍中国科学技术大学的KLMP装置和最新实验结果,以及在建中的KRX等离子体装置。地面实验作为磁场重联的重要研究手段,还需要拓展装置尺寸及对不同条件下重联特征的研究。 相似文献
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针对某新型气象卫星的在轨微振动测量需求,分析微振动对于卫星及其精密载荷的影响,提出一种具有可切换量程和较高故障容错能力的卫星微振动测量单元设计方案.通过地面试验数据与在轨数据的对比,证明该系统能够准确辨识整星及高精度载荷在不同工况下的微振动力学数据.该系统功能的成功实现为进一步优化星体结构、改善高精度载荷工作环境提拱了... 相似文献
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地磁环境下卫星磁试验中的外干扰磁场控制补偿方法 总被引:1,自引:1,他引:0
针对地磁环境下外干扰磁场影响卫星磁试验精度问题,综合分析外干扰源场和卫星近场特性;通过合理布局(包括位置和方式)外干扰磁场监测传感器和卫星磁场采集传感器,增设动态磁场采集的A/D取样扫描频率循环控制、信号统计、滤波、数据拟合等信号处理功能,解决了监测传感器和采集传感器所得到的干扰信号的同步性、等效性、一致性,以及采集传感器信号中卫星真实磁场与干扰磁场之间的不相干性;实现了卫星磁试验的外干扰磁场有效闭环控制、自动跟踪、补偿和修正。通过24 h实时监测,外干扰磁场波动控制在0.5~1.0 n T范围内,获得地磁环境下卫星24 h"准零磁"环境磁试验条件,满足卫星磁试验对磁环境的技术要求。 相似文献
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面向空间应用的高精度磁阻磁强计设计及性能测试 总被引:1,自引:0,他引:1
文章基于磁阻磁强计的工作原理,提出了高精度磁阻磁强计三分量探头和电子电路设计方案:改进磁强计三分量探头结构,以消除三分量磁畴间的相互干扰所引起的测量误差;采用交流耦合和闭环控制工作模式,以消除磁畴排列紊乱带来的影响,稳定磁强计的工作状态。关键性能指标的测试结果表明,磁阻磁强计在1 Hz点处的频谱噪声达到38 pT/(Hz)~(1/2),其噪声性能显著提高。另外,该磁阻磁强计采用微型化结构设计,便于安装,满足微小卫星的空间磁场探测的需求。 相似文献
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星载激光测高技术是对地观测系统中最为核心和前沿的信息获取技术之一,因其具有探测方向性好、测距精度高等特点,在地球科学领域中体现出了巨大的应用潜力。在ICESat/GLAS测高地面数据处理系统的基础上,针对将于今年发射的高分七号卫星的载荷特点,设计了一套星载激光测高地面数据处理系统软件。该软件可实现对星载激光测高数据的地面处理并生成3级数据产品,包含激光能量计算、波形分解和激光脚点定位等,以及相应各级产品的数据质量控制处理。利用高分七号仿真数据对该软件进行相应的性能测试,测试结果表明:该系统软件基本满足需求,已初步具备星载激光测高地面数据处理能力。 相似文献
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目前航天测绘相机几何参数的在轨标定通常经由地面检校场数据处理完成。然而,由于一次摄影中难以保证获取的地面检校场影像完整,使得在轨标定周期较长,进而导致实时监测与标定非常困难。“高分十四号”卫星搭载了一种新的姿态测定系统,利用高精度的相机光轴监测实现对相机几何参数的在轨实时标定。文章在此基础上对高分卫星星地相机间夹角在轨解算方案进行了优化,并基于数值仿真和在轨实测数据进行了分析,结果显示优化算法可以进一步提高影像内定向稳定度和最终的定位精度,未来有望在高精度立体测绘应用中发挥重要作用。 相似文献
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《Acta Astronautica》2007,60(10-11):880-888
The Korea Sounding Rocket-III (KSR-III) was successfully launched on November 28, 2002 from the west coast of the Korean Peninsula. The science payload onboard the KSR-III included an ozone detector and two magnetometers along with other various sensors installed to measure physical characteristics such as temperature, pressure, strain, and acceleration. The main objective of KSR-III was to evaluate the liquid propulsion engine system which has been newly adopted in the KSR series. In addition to this main objective, the science payload conducted atmospheric soundings. The payload data were transmitted to the ground station in real time by an onboard telemetry system. The UV radiometer measured the direct solar UV radiation and during the ascending phase the vertical ozone density profile was obtained. This result was compared with coincident measurements taken by other satellites, a ground station, and an ozonesonde. A fluxgate-type magnetometer was onboard the KSR-III to observe the Earth's DC magnetic field and for AC field measurements, a search-coil magnetometer was installed. This was the first Korean mission to use magnetometers on a rocket-borne platform to measure the Earth's magnetic field. Using the telemetry magnetometer data, a study on the rocket attitude was carried out. This paper will give an overview of the design, calibration, and test results of the science payload onboard the KSR-III. 相似文献
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FY-2C星辐射定标及其结果分析 总被引:2,自引:0,他引:2
介绍了风云二号(FY-2)C星发射前后红外与水汽波段的地面真空辐射定标、星上黑体定标和地面辐射校正场定标,以及可见光波段的地面太阳定标、积分球定标、地面辐射校正场定标和太阳像的原理与方法.给出了C星不同波段不同定标法的结果.分析表明,C星采用的定标方法均有效,并互为补充和验证.为进一步提高定标精度,还可对环境温度模拟、二次曲线拟合、减小积分球定标误差和光谱响应等作相应的改进. 相似文献
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This paper analyzes superconducting (SC) coils technology to improve satellite electric propulsion. SC magnets can generate very high magnetic fields with extremely low ohmic losses, low electric power and PCU weight. Moreover, the weight of SC magnet coils is quite low compared with conventional or permanent magnets capable of producing the same field strength. For instance, to obtain a 0.4 T magnetic field strength, typical of applied field magnetoplasmadynamic thrusters (AF-MPD), based on the Lorentz force, and with thrust in the range of 1 N, this paper shows that only a 40 g coil SC weight is needed, whereas an equivalent field copper winding would weigh about 36 kg. Using SC technology it is shown that the limited magnetic induction provided by a permanent magnet may be raised and also that it is possible to obtain high magnetic fields (of order of several Tesla) with fewer turns, drastically reducing coil volume, weight and complexity compared to conventional winding.
Superconductivity at low temperature (LTSC) requires liquid helium at 4.2 K to produce very high current densities: the thermal analysis in this paper shows that, depending on satellite and thruster, high temperature superconductors (HTSC) wires are sometimes better than LTSC because these can support lower current densities but with a critical superconductivity temperature higher than for LHe, requiring LN2 at 77 K, easier to maintain during the whole mission.
Finally, this paper shows that implementing SC cryogenic technology on a satellite can be achieved with current active coolers technology. 相似文献