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Solar radiation pressure model for the relay satellite of SELENE

机译:SELENE中继卫星的太阳辐射压力模型

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A new radiation pressure model of the relay satellite of SELENE has been developed. The shape of the satellite was assumed to be a combination of a regular octagonal pillar and a column. Radiation forces acting on each part of the spacecraft were calculated independently and summed vectorially to obtain the mean acceleration of the satellite center of mass. We incorporated this new radiation pressure model into the orbit analysis software GEODYN-II and simulated the tracking data reduction process of the relay satellite. We compared two models: one is the new radiation pressure model developed in this work and the other a so-called "cannonball model" where the shape of the satellite is assumed to be a sphere. By the analysis of simulated two-way Doppler tracking data, we found that the new radiation pressure model reduces the observation residuals compared to the cannonball model. Moreover, we can decrease errors in the estimated lunar gravity field coefficients significantly by use of the new radiation pressure model.
机译:已经开发了SELENE中继卫星的新辐射压力模型。假定卫星的形状是正八角形柱和圆柱的组合。分别计算作用在航天器各部分上的辐射力,并进行矢量求和,以获得卫星质心的平均加速度。我们将此新的辐射压力模型整合到轨道分析软件GEODYN-II中,并模拟了中继卫星的跟踪数据缩减过程。我们比较了两种模型:一种是在这项工作中开发的新的辐射压力模型,另一种是所谓的“炮弹模型”,其中假定卫星的形状为球形。通过分析模拟的双向多普勒跟踪数据,我们发现与炮弹模型相比,新的辐射压力模型减少了观测残差。此外,通过使用新的辐射压力模型,我们可以显着减少估计的月球重力场系数中的误差。

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