Moon Image Acquisition for Pointing Calibration of LAPAN-A2 Satellite's High Resolution Camera

R. Madina, A. P. S. Jayani, A. Sarah, M. Mukhayadi
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Abstract

The missions of LAPAN-A2 satellite are Earth observation using an RGB digital camera, maritime traffic monitoring, and amateur radio communications. The satellite carries a digital camera, to support the mission, with ground resolution 4 m and a swath width 7 km. It is necessary to do pointing calibration to measure misalignment between spacecraft's attitude sensors, spacecraft axis, and cameras, to make sure the accuracy of the camera pointing when capture the image. By using the inertial pointing method, that the satellite is controlled in three axis to direct the satellite camera to the Moon. Nevertheless, the field of view (FOV) of high-resolution digital cameras is very narrow, which is only 0.7° for the Moon to be fully visible in the camera frame. During image acquisition, the star sensor should be still able to see the star so the attitude information of spacecraft can be well determined. It means the time period and position for Moon acquisition is limited. By capturing multiple images, LAPAN-A2 satellite success to get the Moon images right in the center of the frame within the offset between camera and spacecraft axis are 0.1232° on the $x$ axis and −0.93° on the $y$ axis.
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用于LAPAN-A2卫星高分辨率相机指向定标的月球图像采集
LAPAN-A2卫星的任务是使用RGB数码相机进行地球观测、海上交通监测和业余无线电通信。这颗卫星携带一架数码相机,以支持该任务,地面分辨率为4米,宽度为7公里。为了保证航天器姿态传感器、航天器轴与相机之间的对准精度,需要对航天器姿态传感器、航天器轴与相机之间的对准误差进行标定。利用惯性指向法,将卫星控制在三轴上,使卫星相机对准月球。然而,高分辨率数码相机的视场(FOV)非常窄,只有0.7°才能在相机框架中完全看到月球。在图像采集过程中,星敏感器应保持对恒星的可见性,这样才能很好地确定航天器的姿态信息。这意味着获取月球的时间和位置是有限的。通过捕获多幅图像,LAPAN-A2卫星成功地在相机与航天器轴之间的x轴偏移量为0.1232°和y轴偏移量为- 0.93°的帧中心位置获得了月球图像。
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