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1.
火星空间环境磁场探测研究——高精度磁强计 总被引:2,自引:0,他引:2
萤火一号卫星将对火星空间环境磁场实施探测。火星磁场对火星弓激波、磁鞘、电离层、大气等绝大多数空间环境效应都具有重要影响,萤火一号对火星磁场的探测是通过搭载于其上的科学载荷磁强计来实现的。此磁强计在工作原理及具体设计上,考虑了火星轨道严酷的工作环境和科学目标所需的测量要求。通过装星前的地面标定测试,验证了萤火一号磁强计可以在-130~75℃温度范围内测量±256nT以内的磁场,分辨率可达到0.01 nT,带宽内总噪声小于0.03 nT,能够满足萤火一号对火星空间环境探测的需求。 相似文献
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萤火一号卫星将对火星空间环境磁场实施探测. 火星磁场对火星弓激波、磁鞘、电离层、大气等绝大多数空间环境效应都具有重要影响, 萤火一号对火星磁场的探测是通过搭载于其上的科学载荷磁强计来实现的. 此磁强计在工作原理及具体设计上, 考虑了火星轨道严酷的工作环境和科学目标所需的测量要求. 通过装星前的地面标定测试, 验证了萤火一号磁强计可以在-130~75°C温度范围内测量±256 nT以内的磁场, 分辨率可达到0.01 nT, 带宽内总噪声小于0.03 nT, 能够满足萤火一号对火星空间环境探测的需求. 相似文献
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以SWARM为代表的高精度地磁测量卫星对地球磁场探测精度经过标定之后优于0.5 nT,对于开展地磁科学研究具有重要意义。地磁测量卫星通过安装在伸展杆上的矢量磁通门磁强计、标量磁强计和高精度星敏感器,获取测量方向的惯性空间姿态的地磁信息,其中高精度标量磁强计主要用于对磁通门矢量磁强计进行标定。针对地磁测量卫星,研究了矢量磁强计在轨测量误差的校正方法。考虑到矢量磁强计非正交角、标度因子以及偏差的影响,建立磁场矢量线性输出模型;结合标量磁强计的测量值分别设计基于小量近似的线性校正算法和基于参数辨识更新的非线性校正算法;校验两种算法的标定精度,并通过Tukey权重函数改善算法的鲁棒性。仿真结果表明,两种算法校正结果相似,磁场三轴误差可校正至0.5 nT以内,在标量磁强计存在异常值时仍具有较好的校正效果。 相似文献
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基于巨磁阻抗效应(GMI)的磁强计是近年来磁强计研究领域的热点. 相比其他类型磁强计, GMI磁强计具有微型化、高灵敏度、快速响应、高温度 稳定性和低功耗的优点. 本文以铁基纳米晶带材为敏感材料, 设计并实现了GMI 磁强计传感器与后续信号处理电路, 组成一台GMI磁强计. 实验结果表明, 该磁 强计在-25000~25000nT量程内灵敏度为0.176mV·nT-1, 满足实际弱磁场测量要求, 并且具有体积小及功耗低的特点, 有望应用于空间 探测等磁测量领域. 相似文献
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电磁监测试验卫星矢量磁场探测方法 总被引:3,自引:0,他引:3
电磁监测试验卫星是中国第一颗近地轨道电磁场科学探测试验卫星, 探测空间背景磁场是其重要任务之一. 空间背景磁场探测需要在卫星平台上对空间矢量磁场进行长期稳定准确探测, 电磁监测试验卫星采用磁通门磁强计和基于CPT效应的绝对磁场校准装置(Coupled Dark State Magnetometer, CDSM)分别探测空间相对矢量磁场以及绝对标量磁场, 通过数据处理, 使最终的矢量磁场探测数据具有准确性. 这种数据处理方法在理想模型下拥有解析解, 实施过程中载荷的噪声、 准确度及稳定性影响模型的准确性, 会产生数据校准误差. 通过对在轨磁场探测的模拟确定了这种数据处理方法的性能, 验证了在载荷设计性能的基础上电磁监测试验卫星的磁场探测可以实现1 nT的准确度. 相似文献
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恒定弱磁标准装置是用来复现高稳定度的恒定弱磁场,并对所复现的弱磁场进行精确测量的装置。恒定弱磁标准装置是由线圈系统、光泵地磁补偿系统、恒流源系统、磁场测量系统等组成。装置采用先进的Cs光泵磁强计补偿技术,在线圈系统的工作区中产生高稳定度的恒定弱磁场,磁场波动均方差小于0.1 nT。通过高稳定度恒流源和线圈系统可以复现1~1.105nT的磁场。通过He-Cs光泵磁共振仪、频率计数器及计算机构成的磁场测量系统可以对所复现的弱磁感应强度量值进行精确的测量,标准测量不确定度为0.07~0.1 nT。 相似文献
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C. Sumners P. Reiff W. Weber 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The Houston Museum of Natural Science, in collaboration with Rice University has an outreach program taking portable digital theaters to schools and community sites for over five years and has conducted research on student learning in this immersive environment. By using an external independent evaluator, the effectiveness of NASA-funded Education and Public Outreach (EPO) projects can be assessed. This paper documents interactive techniques and learning strategies in full-dome digital theaters. The presentation is divided into Evaluation Strategies and Results and Interactivity Strategies and Results. All learners from grades 3–12 showed statistically significant short-term increase in knowledge of basic Earth science concepts after a single 22-min show. Improvements were more significant on items that were taught using more than one modality of instruction: hearing, seeing, discussion, and immersion. Thus immersive theater can be an effective as well as engaging teaching method for Earth and Space science concepts, particularly those that are intrinsically three-dimensional and thus most effectively taught in an immersive environment. The portable system allows taking the educational experience to rural and tribal sites where the underserved students could not afford the time or expense to travel to museums. 相似文献
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Samujjwal Ray Rajdeep Ray Mofazzal Hossain Khondekar Koushik Ghosh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(8):2214-2226
A monthly average solar green coronal index time series for the period from January 1939 to December 2008 collected from NOAA (The National Oceanic and Atmospheric Administration) has been analysed in this paper in perspective of scaling analysis and modelling. Smoothed and de-noising have been done using suitable mother wavelet as a pre-requisite. The Finite Variance Scaling Method (FVSM), Higuchi method, rescaled range (R/S) and a generalized method have been applied to calculate the scaling exponents and fractal dimensions of the time series. Autocorrelation function (ACF) is used to find autoregressive (AR) process and Partial autocorrelation function (PACF) has been used to get the order of AR model. Finally a best fit model has been proposed using Yule-Walker Method with supporting results of goodness of fit and wavelet spectrum. The results reveal an anti-persistent, Short Range Dependent (SRD), self-similar property with signatures of non-causality, non-stationarity and nonlinearity in the data series. The model shows the best fit to the data under observation. 相似文献
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C.H. Jaroschek M. Hoshino H. Lesch R.A. Treumann 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(3):481-490
We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles. 相似文献
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A. Buch R. Sternberg C. Szopa C. Freissinet C. Garnier El J. Bekri C. Rodier R. Navarro-González F. Raulin M. Cabane M. Stambouli D.P. Glavin P.R. Mahaffy 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
In the frame of the 2009 Mars Science Laboratory (MSL) mission a new sample preparation system (SPS) compatible with gas chromatography–mass spectrometry (GC–MS) has been developed for the in situ analysis of complex organic molecules in the Martian soil. The goal is to detect, if they exist, some of the key compounds that play an important role in life on Earth including carboxylic acids, amino acids and nucleobases. 相似文献
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基于LuGre模型的电液加载系统摩擦补偿 总被引:2,自引:2,他引:2
为了提高电液加载系统控制精度,针对摩擦问题提出了基于LuGre摩擦模型的前馈补偿方法.建立了用于摩擦仿真分析和补偿器设计的电液加载系统数学模型;通过实验获取并分析了相关的摩擦数据;基于实验数据进行LuGre模型参数辨识,把LuGre模型和辨识结果引入电液加载系统数学模型,并进行仿真结果与实际摩擦数据的对照,证明了LuGre摩擦模型的准确性.设计前馈补偿器,进行了实验对比,实验结果表明前馈补偿器可将摩擦产生的控制误差有效地降至未补偿时的30%左右. 相似文献
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G.E. Dorrington 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Various aerial platforms intended for long endurance survey of the Titan surface are presented. A few novel concepts are introduced, including a heated methane balloon and a balloon with a tethered wind turbine. All the concept options are predicted to have lower scientific payload fractions than the Huygens probe. It is concluded that the selection of the best aerial platform option depends on more accurate mass estimates and a clear decision on whether, or not, in situ surface composition measurements are required in conjunction with aerial remote sensing. 相似文献
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H. Cottin P. Coll D. Coscia N. Fray Y.Y. Guan F. Macari F. Raulin C. Rivron F. Stalport C. Szopa D. Chaput M. Viso M. Bertrand A. Chabin L. Thirkell F. Westall A. Brack 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
To understand the evolution of organic molecules involved in extraterrestrial environments and with exobiological implications, many experimental programs in the laboratory are devoted to photochemical studies in the gaseous phase as well as in the solid state. The validity of such studies and their applications to extraterrestrial environments can be questioned as long as experiments conducted in space conditions, with the full solar spectrum, especially in the short wavelength domain, have not been implemented. The experiments that are described here will be carried out on a FOTON capsule, using the BIOPAN facility, and on the International Space Station, using the EXPOSE facility. Vented and sealed exposition cells will be used, which will allow us to study the chemical evolution in the gaseous phase as well as heterogeneous processes, such as the degradation of solid compounds and the release of gaseous fragments. 相似文献
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S. Hekker 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars. These data have revolutionized the fields of transiting exoplanets and asteroseismology. In this review some important asteroseismic results obtained using data from the CoRoT and Kepler space missions concerning stars that show solar-like oscillations are discussed. These results comprise, among others, measurements of the location of the base of the convection zone and helium second-ionization zone in main-sequence stars, the presence (or not) of core-helium burning in red-giant stars, as well as differential rotation in these stars. 相似文献
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K. Clark J. Boldt R. Greeley K. Hand I. Jun R. Lock R. Pappalardo T. Van Houten T. Yan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Missions to explore Europa have been imagined ever since the Voyager mission first suggested that Europa was geologically very young. Subsequently, the Galileo spacecraft supplied fascinating new insights into this satellite of Jupiter. Now, an international team is proposing a return to the Jupiter system and Europa with the Europa Jupiter System Mission (EJSM). Currently, NASA and ESA are designing two orbiters that would explore the Jovian system and then each would settle into orbit around one of Jupiter’s icy satellites, Europa and Ganymede. In addition, the Japanese Aerospace eXploration Agency (JAXA) is considering a Jupiter magnetospheric orbiter and the Russian Space Agency is investigating a Europa lander. 相似文献
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R.D. Bentley A. Csillaghy J. Aboudarham C. Jacquey M.A. Hapgood K. Bocchialini M. Messerotti J. Brooke P. Gallagher P. Fox N. Hurlburt D.A. Roberts L. Sanchez Duarte 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations. 相似文献