roa激光站:从人造卫星到空间碎片跟踪

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Revista Mexicana de Astronomia y Astrofisica Pub Date : 2021-09-01 DOI:10.22201/ia.14052059p.2021.53.33
M. Catalán, M. Sánchez-piedra, M. Larrán, A. Vera, F. della Prugna, J. Marin, J. Relinque
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引用次数: 0

摘要

自太空竞赛开始以来,西班牙海军皇家天文台(ROA)一直是空间大地测量学方面的专家。1975年,在与法国CERGA合作的情况下,在非洲区域研究所安装了一个激光站。自1980年以来,ROA一直自己运营这个空间站。这种设备经常跟踪装有反光镜的人造卫星。2014年,ROA开辟了一个新的研究领域:跟踪目前没有活动并配备了反射器的人造卫星。这个新区域是一个挑战,因为这些物体的轨道精度很差,因为它们没有被常规跟踪。这是我们实现最终目标的一种方法:严格监控空间碎片,即任何类型的不受控制的人造轨道物体。为了实现这一目标,自2017年以来,我们对激光设备进行了重大改变。最重要的是用两个新的激光台替换了旧的激光台。一台发射500毫瓦脉冲,另一台发射功率为25毫瓦。后期激光装置的研究由欧盟(EU) H2020基金资助,并由西班牙工业技术发展中心(CDTI)批准。虽然它允许跟踪协作对象,但它也非常适合跟踪非协作对象。跟踪活动将于2017年11月开始。从那时起,非协作对象将被定期监视。这项工作显示了已经进行的修改,以及直到2019年才获得的结果。
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THE ROA LASER STATION: FROM ARTIFICIAL SATELLITES TO SPACE DEBRIS TRACKING
The Royal Observatory of the Spanish Navy (ROA) is specialist in space geodesy since the beginning of the space race. In 1975 a laser station was installed at ROA in collaboration with the French CERGA (Centre de Recherches en Géodynamique et Astrométrie). Since 1980, ROA has operated that station by their own. This equipment routinely tracks artificial satellites equipped with retro-reflectors. In 2014 ROA opened a new field of research: tracking of artificial satellites currently not active and equipped with retroreflectors. This new area was a challenge given the poor orbital accuracies that are available for these objects as they were not tracked on a routine basis. This served as an approach to our final goal: to strictly monitor space debris, this is, any type of uncontrolled man-made orbiting objects. To fulfill the objective, since 2017, we made significant changes to our laser installation. The most important was the replacement of the old laser bench with two new ones. One transmitting 500 mW-pulses, and another laser bench with 25 W transmission power. The study for the installation of the later laser was financed through European Union (EU) H2020 fundings and granted by the Spanish Centre for Industrial Technological Development (CDTI). Although it allows the tracking of collaborative objects, it is ideal for tracking non-collaborative too. Tracking activities begin in November 2017. From then onward, non-collaborative objects are monitored on a regular basis. This work shows the modifications already made, and the results obtained until 2019.
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来源期刊
Revista Mexicana de Astronomia y Astrofisica
Revista Mexicana de Astronomia y Astrofisica 地学天文-天文与天体物理
CiteScore
1.30
自引率
10.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: The Revista Mexicana de Astronomía y Astrofísica, founded in 1974, publishes original research papers in all branches of astronomy, astrophysics and closely related fields. Two numbers per year are issued and are distributed free of charge to all institutions engaged in the fields covered by the RMxAA.
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