共查询到20条相似文献,搜索用时 31 毫秒
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E.H. Lemke 《Acta Astronautica》1985,12(3):149-154
The idea of stabilizing the shape of a reflector dish for a space-based radiotelescope by an extensive magnetic field is considered. We outline a construction where the axes of rotational symmetry of the dish lie on the axes of rotational symmetry of a large circular solenoid. Its magnetic field produces a stabilizing pressure by acting on a distribution of dipole moment on the dish. In cosmic regions where the gravity gradient is smaller than the solar radiation pressure, large receiver apertures and large area-to-mass ratios of the dish are attainable. The latter might lead to a higher shape accuracy of the reflecting surface compared to the truss frame stabilization. We calculate the distribution of dipole moment that gives a parabolic surface in the approximation of no dish elasticity and no magnetic dish-dish interaction. A disadvantage is the relative large mass of the solenoid. However, we find that it can be about three times smaller in diameter than the dish. 相似文献
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航天器磁性测量误差因素及精度评估与航天器结构尺寸、磁矩量级、内部磁性分布特征,以及所用的磁测试方法和测试设备等有密切关系。近场分析法是航天器磁偶极矩测定中经典有效的测试方法。文章就该法在航天器磁测试中的系统误差、随机误差因素及精度评估逐一进行详细论述和深入剖析;针对中大尺度航天器正置态磁测试中垂向磁矩测试结果存在的误差,提出提高测试精度和改进误差评估的有效方法和措施;给出航天器磁测试有效性综合评估的基本条件和评判标准,得到不同尺度航天器磁测试误差的预估参考范围。文章所述航天器磁测试误差因素及精度评估技术对于提高航天器磁测试精度、有效控制航天器磁性具有指导意义。 相似文献
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为了对磁偶极子进行高精度的磁性定位,文章从磁偶极子模型出发,推导出磁偶极子的空间坐标与其产生的磁场及磁场梯度之间的关系式;针对模型及关系式,设计了一种全张量磁场梯度传感器,能够一次测量出精确定位所需的9个磁场梯度值和3个磁场强度值;对比仿真结果和实验结果,发现二者具有较好的一致性,证明了该理论模型的有效性。对于磁偶极子,用半径为0.05 m的梯度传感器对磁矩为2 A·m~2的磁偶极子进行定位测量,在0.5~1 m距离内定位误差不大于10%。文章还对定位测量误差的原因进行了分析,包括梯度测量基线距离及传感器半径对定位误差的影响。 相似文献
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E.H. Lemke 《Acta Astronautica》1984,11(9):565-567
A toroidal solenoid in orbit can represent a magnetic trap for bodies carrying dipole moment. We find the dependence of the trap dimensions on the electrical parameters and the orbit height. There is no trap if the solenoid radius exceeds a certain value. Various trap dimensions are calculated for a non-spinning space station in Earth or Sun orbit. The trap dimension is nearly independent of the solenoid orientation so that the solenoid may be fastened to the station rigidly. If the solenoid radius is in the range of some meters, the trap dimension is one order of magnitude greater for a distant Earth orbit and two orders of magnitude for an orbit around the Sun at distances of the order of one AU. The calculations are performed for a non-superconducting solenoid. The trap can be used for simplifying the docking on of maintenance vehicles or building modules, as safety mechanism for crewmembers working in outer space, and for the collection of paramagnetic or ferromagnetic dust stopped by mechanical means. 相似文献
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Griessmeier JM Stadelmann A Motschmann U Belisheva NK Lammer H Biernat HK 《Astrobiology》2005,5(5):587-603
Because of their different origins, cosmic rays can be subdivided into galactic cosmic rays and solar/stellar cosmic rays. The flux of cosmic rays to planetary surfaces is mainly determined by two planetary parameters: the atmospheric density and the strength of the internal magnetic moment. If a planet exhibits an extended magnetosphere, its surface will be protected from high-energy cosmic ray particles. We show that close-in extrasolar planets in the habitable zone of M stars are synchronously rotating with their host star because of the tidal interaction. For gravitationally locked planets the rotation period is equal to the orbital period, which is much longer than the rotation period expected for planets not subject to tidal locking. This results in a relatively small magnetic moment. We found that an Earth-like extrasolar planet, tidally locked in an orbit of 0.2 AU around an M star of 0.5 solar masses, has a rotation rate of 2% of that of the Earth. This results in a magnetic moment of less than 15% of the Earth's current magnetic moment. Therefore, close-in extrasolar planets seem not to be protected by extended Earth-like magnetospheres, and cosmic rays can reach almost the whole surface area of the upper atmosphere. Primary cosmic ray particles that interact with the atmosphere generate secondary energetic particles, a so-called cosmic ray shower. Some of the secondary particles can reach the surface of terrestrial planets when the surface pressure of the atmosphere is on the order of 1 bar or less. We propose that, depending on atmospheric pressure, biological systems on the surface of Earth-like extrasolar planets at close-in orbital distances can be strongly influenced by secondary cosmic rays. 相似文献
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动态环路法磁矩测量技术研究 总被引:3,自引:2,他引:1
文章提出了一种新的航天器磁矩测量方法——动态环路法。首先,利用高斯电势级数公式建立了航天器的磁性偶极-四极模型。然后,针对模型中的8个磁矩分量,基于动态环路法的基本测量原理,设计了5组磁通感应线圈;根据8个磁矩分量的磁感应强度分布以及5组线圈的具体形状和位置,给出了各磁矩分量的磁通量表达式和利用积分法计算各个磁矩分量的公式。最后,对在推导过程中由于简化带来的近似误差和利用积分法计算公式理论计算误差进行了初步分析。当线圈间隔L为半径r的5%时,近似误差和积分法理论计算误差分别不超过2%和0.17%。结果表明,该方法不但能够获得航天器的磁矩大小并计算出其磁心坐标,而且还具有测量过程简单、测量速度较快以及测量精度高的优点。 相似文献
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利用地磁场测量的小卫星自主导航设计 总被引:2,自引:1,他引:2
地磁场矢量是卫星所在位置的函数 ,通过对地磁场的测量 ,即可实现对近地小卫星的自主导航。本文采用卡尔曼滤波技术设计了小卫星基于地磁场测量的导航方法 ,在采用地磁场模型时选取磁偶极子模型 ,以此使设计算法的计算量大大减少。最后利用数字仿真验证了系统性能。 相似文献
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针对因双超平台姿态控制引入非接触磁浮机构这一关键执行机构,而可能引起的卫星平台新的电磁兼容问题,开展了非接触磁浮机构的电磁干扰特性研究。首先,介绍了非接触磁浮机构及其驱动器的工作原理;其次,分别对非接触磁浮机构驱动器的脉冲宽度调制(PWM)控制信号高频干扰特性和传导电磁干扰特性进行了理论和仿真分析,并将其频率特性与星上其他典型单机的工作频率进行了比对。对比分析结果表明:非接触磁浮机构的电磁干扰频率与星上其他典型单机之间间隔较大,其相互之间产生的电磁干扰可忽略,磁浮机构的引入不会产生新的电磁兼容问题。 相似文献
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E.H. Lemke 《Acta Astronautica》1983,10(7):517-520
We examine the motion of a superconducting dipole in the field of a large flat solenoid. It is found that ratios of about 1 MJ per kilogramme of dipole can be reached for an effective current density of about 400 A/mm2 in the dipole if the diameter of the dipole and solenoid are of the order of 6 and 30 m, respectively. The values will be less critical if the dipole passes the field of two solenoids. We propose a mechanical lever-rope method for stabilization of the dipole axis and determine the deflection of the dipole's path from the vertical under small perturbations of the initial co-ordinates. 相似文献
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为了解决无陀螺磁控小卫星的姿态稳定和捕获问题,本文针对偏置稳定的主动磁控小卫星姿态控制平台,基于磁控力矩的时间累积作用效果等效卫星角动量增量的规律,设计了一种仅利用角度反馈的卫星大角度磁捕获控制律。通过仿真和卫星在轨实测的验证,证明该方法具有良好的收敛效果和鲁棒性,工程实现简单,可靠性高,适用于中低轨道的通信小卫星。 相似文献
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The behavior of small-scale irregularities of the electron density, which can exist in the near-Earth plasma at the ionospheric and magnetospheric heights is studied. They can be of both natural and artificial origin. The kinetic approach is used, and the Vlasov-Poisson system of equations is numerically solved using the method of large particles. In the plane perpendicular to the magnetic field, the evolution of a single irregularity having a circular cross-section at the initial moment is calculated. The influence of the transverse dimension of the irregularity and the value of deviation from electro-neutrality at the initial moment on the parameters characterizing the process of irregularity evolution is studied. 相似文献
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Magnetism, iron minerals, and life on Mars 总被引:1,自引:0,他引:1
Rochette P Gattacceca J Chevrier V Mathé PE Menvielle M;Mappa Science Team 《Astrobiology》2006,6(3):423-436
A short critical review is provided on two questions linking magnetism and possible early life on Mars: (1) Did Mars have an Earth-like internal magnetic field, and, if so, during which period and was it a requisite for life? (2) Is there a connection between iron minerals in the martian regolith and life? We also discuss the possible astrobiological implications of magnetic measurements at the surface of Mars using two proposed instruments. A magnetic remanence device based on magnetic field measurements can be used to identify Noachian age rocks and lightning impacts. A contact magnetic susceptibility probe can be used to investigate weathering rinds on martian rocks and identify meteorites among the small regolith rocks. Both materials are considered possible specific niches for microorganisms and, thus, potential astrobiological targets. Experimental results on analogues are presented to support the suitability of such in situ measurements. 相似文献
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对地磁场中卫星不倒置状态下分离卫星Z分量磁矩的测试及数据处理方法进行了研究。利用地球磁场方向特征、卫星剩磁矩与感磁矩在不同测量状态和测量过程中的变化,确定卫星Z分量磁矩含地磁垂直向感磁影响与不含地磁垂直向感磁影响的比例关系,基于积累的不同卫星水平和垂直向的磁测试数据,用近场法计算,获得了卫星Z分量的感磁系数。试验表明:用该法测得的Z分量磁矩测量相对误差不大于30%,工程上有较高的实用价值。 相似文献
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为了提高无人机航空磁探测精度,文章利用大疆六旋翼无人机作为飞行平台,搭载三轴磁通门传感器及相应的数据采集子系统,组建了旋翼无人机磁场测量系统;分析和测量了六旋翼无人机本底磁性分布特征,优化了无磁伸杆的安装位置;采用综合系数法修正了三轴磁通门传感器的误差;最后进行了野外飞行试验,对旋翼无人机磁测系统的整体性能进行验证。结果表明,系统可持续飞行15 min,可有效完成低空磁场探测和磁矩计算,且飞行稳定性能高。文章进一步提出了技术改进方向。该研究可为无人机磁探技术和工程应用提供参考。 相似文献