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    • 1. 发明申请
    • ATTITUDE-ACQUISITION METHODS AND SYSTEMS FOR CONTROLLED SPACECRAFT ATTITUDE
    • 用于控制的空间姿态的姿态采集方法和系统
    • US20040098177A1
    • 2004-05-20
    • US10300454
    • 2002-11-19
    • The Boeing Company
    • David D. NeedelmanYeong-Wei A. WuRongsheng Li
    • G06F017/00
    • G01C21/025B64G1/26B64G1/285B64G1/288B64G1/361G05D1/0883
    • Attitude acquisition methods and systems are provided which reduce the time generally required to acquire spacecraft attitude estimates and enhance the probability of realizing such estimates. The methods and systems receive, over a time span nullt, successive frames of star-sensor signals that correspond to successive stellar fields-of-view, estimate spacecraft rotation nullr throughout at least a portion of the time span nullt, and, in response to the spacecraft rotation nullr, process the star-sensor signals into a processed set of star-sensor signals that denote star positions across an expanded field-of-view that exceeds any of the successive fields-of-view. The expanded field-of-view facilitates identification of the stars that generated the processed set of star-sensor signals to thereby acquire an initial attitude estimate.
    • 提供了姿态获取方法和系统,减少了获取航天器态度估计所需的时间,并提高了实现此类估计的可能性。 方法和系统在时间跨度Deltat中接收对应于连续的恒星视场的星形传感器信号的连续帧,在至少一部分时间段Deltat中估计航天器旋转Deltar,并响应于 航天器旋转Deltar,将星形传感器信号处理成一组经过处理的恒星传感器信号,它们表示超过任何连续视场的扩展视场中的星形位置。 扩展的视野有助于识别产生经处理的星形传感器信号集合的恒星,从而获得初始姿态估计。
    • 2. 发明申请
    • Satellite methods and structures for improved antenna pointing and wide field-of-view attitude acquisition
    • 用于改善天线指向和广视野姿态采集的卫星方法和结构
    • US20030222816A1
    • 2003-12-04
    • US10162465
    • 2002-06-03
    • The Boeing Company
    • Ketao LiuRichard FowellYeong-Wei A. WuRongsheng Li
    • H04B007/185H01Q003/00
    • H01Q3/005
    • Methods and structures are provided for reducing pointing errors null of satellite antennas and for generating broad field-of-view satellite attitude acquisition patterns. In one method embodiment, satellite transmit beams have estimated pointing attitudes null and are transmitted to overlap on a ground-based receiving terminal which has a known terminal location null and which measures received signal strengths null. Pointing errors null of the transmit beams are then determined from the estimated pointing attitudes null, the terminal location null and the signal strengths null and the pointing errors null are subsequently reduced by revising the pointing attitudes null. Other method embodiments utilize known signal-strength functions and antenna signals with known signal parameters such as frequencies and/or modulations.
    • 提供了用于减少卫星天线的指向误差zeta和产生广泛的视野卫星姿态采集模式的方法和结构。 在一个方法实施例中,卫星发射波束具有估计的指向姿态β,并且在具有已知终端位置λ并且测量接收信号强度α的基于地面的接收终端上被发送以重叠。 然后从估计的指向态度β确定发射波束的指向误差zeta,随后通过修正指向态度β来减少终端位置λ和信号强度α和指向误差zeta。 其他方法实施例利用具有已知信号参数(例如频率和/或调制)的已知信号强度函数和天线信号。
    • 4. 发明申请
    • SPACECRAFT METHODS AND STRUCTURES WITH ENHANCED ATTITUDE CONTROL THAT FACILITATES GYROSCOPE SUBSTITUTIONS
    • 具有增强姿态控制的补充方法和结构,有助于取代GYROSCOPE
    • US20030171855A1
    • 2003-09-11
    • US10039488
    • 2001-10-28
    • BOEING COMPANY
    • Rongsheng LiJeffrey A. KurlandAlec M. DawsonYeong-Wei A. WuDavid S. Uetrecht
    • G05D001/00G06F007/00
    • G05D1/0883B64G1/26B64G1/28B64G1/285B64G1/288B64G1/32B64G1/36G05B13/024
    • Methods and structures are provided that enhance attitude control during gyroscope substitutions by insuring that a spacecraft's attitude control system does not drive its absolute-attitude sensors out of their capture ranges. In a method embodiment, an operational process-noise covariance Q of a Kalman filter is temporarily replaced with a substantially greater interim process-noise covariance Q. This replacement increases the weight given to the most recent attitude measurements and hastens the reduction of attitude errors and gyroscope bias errors. The error effect of the substituted gyroscopes is reduced and the absolute-attitude sensors are not driven out of their capture range. In another method embodiment, this replacement is preceded by the temporary replacement of an operational measurement-noise variance R with a substantially larger interim measurement-noise variance R to reduce transients during the gyroscope substitutions.
    • 提供了通过确保航天器的姿态控制系统不将其绝对姿态传感器驱动到其捕获范围之外来增强陀螺仪替换期间的姿态控制的方法和结构。 在方法实施例中,卡尔曼滤波器的操作过程 - 噪声协方差Q被临时过程噪声协方差Q临时替换。该替换增加了给予最近姿态测量的重量并加速了姿态误差的降低,并且 陀螺偏置误差。 取代陀螺仪的误差效应降低,绝对姿态传感器不会被驱赶出其捕获范围。 在另一方法实施例中,该替换之前是临时替换具有相当大的临时测量噪声方差R的操作测量噪声方差R,以减少在陀螺仪替换期间的瞬变。
    • 7. 发明申请
    • SPACECRAFT METHODS AND SYSTEMS FOR AUTONOMOUS CORRECTION OF STAR TRACKER CHARGE-TRANSFER-EFFICIENCY ERRORS
    • 用于自动校正星形跟踪器充电传输效率错误的方法和系统
    • US20020125375A1
    • 2002-09-12
    • US09769637
    • 2001-01-25
    • THE BOEING COMPANY
    • Yeong-Wei WuRongsheng LiJames H. Green
    • B64G001/24B64G001/36
    • G05D1/0883B64G1/26B64G1/288B64G1/361B64G2001/245
    • Structures and methods are provided for deriving corrected star coordinates Ccrctd from measured star coordinates Cms that include star tracker charge transfer efficiency (CTE) errors. The structures and methods are based on a recognition that measured star coordinates Cms of star image centroids include CTE errors which are functions of the CCD path lengths over which the associated electrical charges traveled. In particular, the errors are substantially a product of a respective path length and a star-coordinate error factor null which, in turn, is a function of the star image magnitudes msi. Information contained in different measured star coordinates Cms is organized to facilitate the derivation of an estimate null* of the star-coordinate error factor null with conventional estimation processes. The measured star coordinates Cms are then corrected with the error factor estimate null* to realize the corrected star coordinates Ccrctd and, thereby, improve the accuracy of spacecraft attitude control.
    • 提供了结构和方法,用于从包括星形跟踪器电荷转移效率(CTE)误差的测量的星座坐标Cms导出校正星座标Ccrctd。 结构和方法基于识别,星形图像质心的测量星座坐标Cms包括作为相关电荷行进的CCD路径长度的函数的CTE误差。 特别地,误差基本上是相应的路径长度和星坐标误差因子&xgr的乘积; 这又是星形图像幅度msi的函数。 包含在不同测量星座坐标Cms中的信息被组织以便于推导星坐标误差因子&xgr的估计&xgr * 与传统的估计过程。 然后用误差因子估计&xgr *来校正测量的星座Cms,以实现校正的星座Ccrctd,从而提高航天器姿态控制的精度。