Development of a CubeSat CLIMBing to the Van-Allen belt

V. Eschelmüller, A. Stren, M. Issa, J. Bauer, A. Goswami, E. Vitztum, K. Repän, W. Treberspurg, C. Scharlemann
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引用次数: 1

Abstract

Based on its successful CubeSat mission PEGASUS, the University of Applied Sciences Wiener Neustadt (FHWN) is preparing its new CubeSat mission called CLIMB. CLIMB is a 3U CubeSat that will be launched to a low, circular orbit of about 500 km. Using a Field Emission Electric Propulsion (FEEP) system commercialized by the company ENPULSION, the satellite will be lifted to an elliptical orbit with its apogee around 1000 km – well inside the inner Van Allen belt. During its 1.5 yearlong ascent and its operation in the Van Allen belt, the satellite will continuously monitor the space radiation with a RadFET dosimeter payload and the impact on CLIMB’s subsystems. Comparisons with radiation testing on ground will allow the assessment of the capability of ground tests to predict effects of space radiation on CubeSat subsystems. The operation of the propulsion system will raise the satellite’s apogee on average 16 times a day. A comprehensive analysis has been conducted to assess its collision probability throughout its mission time. Using various tools, provided by ESA (CROC, MASTER and the DRAMA ARES python package), the collision probability for the entire mission duration (~3 years) was calculated to be 3.38 × 10-5, i.e. a magnitude smaller than the requested probability of 10-4. The second payload of CLIMB is an anisotropic magnetoresistance (AMR) magnetometer with a, for CubeSats high, sensitivity of about 10 nT RMS. The first results of measurements with this COTS based magnetometer are presented as well as experimental assessments of the satellite’s magnetic cleanliness. The benign thermal conditions on CubeSats operating close to Earth are complicated by the relatively high-power propulsion system onboard CLIMB. Detailed numerical analysis (ANSYS, ESATAN) and experimental verifications resulted in the identification of possible methods to deal with up to 18 W of dissipated electric power. The main heat sources are the thruster and the battery unit, during thruster operation
攀爬到范艾伦带的立方体卫星的研制
基于其成功的立方体卫星任务PEGASUS,维也纳新城应用科学大学(FHWN)正在准备其新的立方体卫星任务,称为CLIMB。CLIMB是一颗3U的立方体卫星,将被发射到大约500公里的低圆形轨道上。使用由enpel公司商业化的场发射电力推进(FEEP)系统,卫星将被提升到一个椭圆形轨道,其远地点约为1000公里-完全在范艾伦带内。在其长达1.5年的上升和在范艾伦带的运行期间,卫星将使用RadFET剂量计载荷持续监测空间辐射以及对CLIMB子系统的影响。通过与地面辐射试验的比较,可以评估地面试验预测空间辐射对立方体卫星子系统影响的能力。推进系统的运行将使卫星的远地点平均每天上升16次。对其在整个任务时间内的碰撞概率进行了综合分析。利用欧空局提供的各种工具(CROC、MASTER和DRAMA ARES python包),计算出整个任务期间(~3年)的碰撞概率为3.38 × 10-5,即比要求的10-4的概率小。CLIMB的第二个有效载荷是一个各向异性磁阻(AMR)磁强计,对于CubeSats来说,其灵敏度约为10 nT RMS。介绍了这种基于COTS的磁力计的初步测量结果以及对卫星磁洁净度的实验评估。在靠近地球的立方体卫星上运行的良好的热条件由于相对高功率的推进系统而变得复杂。详细的数值分析(ANSYS, ESATAN)和实验验证确定了处理高达18w耗散电力的可能方法。在推进器运行过程中,主要热源是推进器和电池单元
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