首页> 外文会议>ESA Symposium on European Rocket and Balloon Programmes and Related Research >ESTADIUS: A HIGH MOTION 'ONE ARCSEC' DAYTIME ATTITUDE ESTIMATION SYSTEM FOR STRATOSPHERIC APPLICATIONS
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ESTADIUS: A HIGH MOTION 'ONE ARCSEC' DAYTIME ATTITUDE ESTIMATION SYSTEM FOR STRATOSPHERIC APPLICATIONS

机译:ESTADIUS:用于平流层应用的高速“一弧度”白天姿态估计系统

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ESTADIUS is an autonomous, accurate and daytime attitude estimation system, for stratospheric balloons that require a high level of attitude measurement and stability. The system has been developed by CNES. ESTADIUS is based on star sensor and gyrometer data fusion within an extended Kalman filter. The star sensor is composed of a 16 MPixels visible-CCD camera and a large aperture camera lens (focal length of 135mm, aperture f/1.8, 10°×15° field of view or FOV) which provides very accurate stars measurements due to very low pixel angular size. This also allows detecting stars against a bright sky background. The gyrometer is a 0.01°/h performance class Fiber Optic Gyroscope (FOG). The system is adapted to work down to an altitude of ~25km, even under high cinematic conditions. Key elements of ESTADIUS are: daytime conditions use (as well as night time), autonomy (automatic recognition of constellations), high angular rate robustness (a few deg/s thanks to the high performance of attitude propagation), stray-light robustness (thanks to a high performance baffle), high accuracy (<1", 1σ). Four stratospheric qualification flights were very successfully performed in 2010/2011 and 2013/2014 in Kiruna (Sweden) and Timmins (Canada). ESTADIUS will allow long stratospheric flights with a unique attitude estimation system avoiding the restriction of the night/day conditions at launch. The first operational flight of ESTADIUS will be in 2015 for the PILOT scientific missions (led by IRAP and CNES in France). Further balloon missions such as CEDRE will use the system. ESTADIUS is probably the first autonomous, large FOV, daytime stellar attitude measurement system This paper details the technical features and inflight results.
机译:ESTADIUS是一种自动,准确和白天的姿态估计系统,用于需要高水平姿态测量和稳定性的平流层气球。该系统由CNES开发。 ESTADIUS基于扩展的卡尔曼滤波器内的恒星传感器和陀螺仪数据融合。恒星传感器由一个16 MPixels可见CCD相机和一个大光圈相机镜头(焦距为135mm,光圈f / 1.8,10°×15°视场或FOV)组成,由于具有非常高的观测精度低像素角尺寸。这也允许在明亮的天空背景下检测星星。陀螺仪是性能为0.01°/ h的光纤陀螺仪(FOG)。该系统即使在高电影条件下也能在低至25km的高度下工作。 ESTADIUS的关键要素是:白天条件的使用(以及夜间),自治(自动识别星座),高角速率鲁棒性(由于姿态传播的高性能,几度/ s),杂散光鲁棒性(得益于高性能挡板),高精度(<1“,1σ)。在2010/2011年和2013/2014年,在基律纳(瑞典)和蒂明斯(加拿大)成功进行了四次平流层资格飞行。ESTADIUS将允许长平流层飞行带有独特姿态估计系统的飞行,避免了发射时的昼/夜条件的限制,ESTADIUS的首个运行飞行将于2015年进行PILOT科学任务(由法国IRAP和CNES领导)。 ESTADIUS可能是第一个自主的,大型FOV,白天恒星姿态测量系统。

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