Orbit determination results and space debris test observation of the OWL-Net

Author(s):  
Jin Choi
2012 ◽  
Vol 62 (1) ◽  
pp. 10-22 ◽  
Author(s):  
A. Milani ◽  
D. Farnocchia ◽  
L. Dimare ◽  
A. Rossi ◽  
F. Bernardi

2015 ◽  
Vol 51 (2) ◽  
pp. 1231-1240 ◽  
Author(s):  
Mauro Grassi ◽  
Ediz Cetin ◽  
Andrew G. Dempster

2012 ◽  
Vol 4 (1) ◽  
pp. 39-51 ◽  
Author(s):  
Fran M. Fadrique ◽  
Alberto A. Maté ◽  
Joan J. Grau ◽  
Jaime F. Sánchez ◽  
Laura A. García

Author(s):  
Alessandro Morselli ◽  
Pierluigi Di Lizia ◽  
Germano Bianchi ◽  
Claudio Bortolotti ◽  
Stelio Montebugnoli ◽  
...  

Author(s):  
Paul Wagner ◽  
Tim Clausen

AbstractFor safe operation of active space crafts, the space debris population needs to be continuously scanned, to avoid collisions of active satellites with space debris. Especially the low Earth orbit (LEO) shows higher risks of collisions due to the highest density of orbital debris. Laser ranging stations can deliver highly accurate distance measurements of debris objects allowing precise orbit determination and more effective collision avoidance. However, a laser ranging station needs accurate a priori orbit information to track an orbital object. To detect and track unknown orbital objects in LEO, here, a passive optical staring system is developed for autonomous 24/7 operation. The system is weather-sealed and does not require any service to perform observations. To detect objects, a wide-angle imaging system with 10° field of view equipped with an astronomical CCD camera was designed and set up to continuously observe the sky for LEO objects. The system can monitor and process several passing objects simultaneously without limitations. It automatically starts an observation, processes the images and saves the 2D angular measurements of each object as equatorial coordinates in the TDM standard. This allows subsequent initial orbit determination and handover to a laser tracking system. During campaigns at twilight the system detected up to 36 objects per hour, with high detection efficiencies of LEO objects larger than 1 m3. It is shown that objects as small as 0.1 m3 can be detected and that the estimated precision of the measurements is about 0.05° or 7 × the pixel scale.


2016 ◽  
Vol 45 (2) ◽  
pp. 0229004
Author(s):  
杜建丽 Du Jianli ◽  
李彬 Li Bin ◽  
陈立娟 Chen Lijuan ◽  
雷祥旭 Lei Xiangxu ◽  
吴满意 Wu Manyi ◽  
...  

2016 ◽  
Vol 45 (2) ◽  
pp. 229004
Author(s):  
杜建丽 Du Jianli ◽  
李彬 Li Bin ◽  
陈立娟 Chen Lijuan ◽  
雷祥旭 Lei Xiangxu ◽  
吴满意 Wu Manyi ◽  
...  

2021 ◽  
Vol 13 (23) ◽  
pp. 4878
Author(s):  
Long Chen ◽  
Chengzhi Liu ◽  
Zhenwei Li ◽  
Zhe Kang

A single electro-optical (EO) sensor used in space debris observation provides angle-only information. However, space debris position can be derived using simultaneous optical measurements obtained from two EO sensors located at two separate observation sites, and this is commonly known as triangulation. In this paper, we propose a new triangulation algorithm to determine space debris position, and its analytical expression of Root-Mean-Square (RMS) position error is presented. The simulation of two-site observation is conducted to compare the RMS positioning error of the proposed triangulation algorithm with traditional triangulation algorithms. The results show that the maximum RMS position error of the proposed triangulation algorithm is not more than 200 m, the proposed triangulation algorithm has higher positioning accuracy than traditional triangulation algorithms, and the RMS position error obtained in the simulation is nearly consistent with the analytical expression of RMS position error. In addition, initial orbit determination (IOD) is carried out by using the triangulation positioning data, and the results show that the IOD accuracy of two-site observation is significantly higher than that of the single-site observation.


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