METEORITES ORBITS RECONSTRUCTION BY OPTICAL IMAGING (MOROI) NETWORK

被引:0
作者
Nedelcu, D. A. [1 ,2 ]
Birlan, M. [1 ,2 ]
Turcu, V [3 ]
Boaca, I [1 ]
Badescu, O. [1 ]
Gornea, A. [1 ]
Sonka, A. B. [1 ,4 ]
Blagoi, O. [1 ]
Danescu, C. [1 ]
Paraschiv, P. [1 ]
机构
[1] Romanian Acad, Astron Inst, Str Cutitul de Argint 5, Bucharest 040557, Romania
[2] PSL Res Univ, Inst Mecan Celeste & Calculs Ephemerides, CNRS UMR8028, Observ Paris, 77 Av Denfert Rochereau, F-75014 Paris, France
[3] Astron Inst Romanian Acad, Astron Observ, Cluj Napoca Str Ciressilor 19, Cluj Napoca 400487, Romania
[4] Univ Bucharest, Fac Phys, 405 Atomistilor, Magurele 077125, Ilfov, Romania
来源
ROMANIAN ASTRONOMICAL JOURNAL | 2018年 / 28卷 / 01期
关键词
meteors; meteorites; asteroids; celestial mechanics; orbits;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An wide range, all-sky camera network is an effective infrastructure for the detection of atmospheric entries of natural (meteoroids) or artificial bodies (space debris). The Meteorites Orbits Reconstruction by Optical Imaging (MOROI) is an all-sky network operated by the Astronomical Institute of the Romanian Academy. Here we present the overall architecture of the network that became operational on mid-2017 and the preliminary results on atmospheric trajectory and orbit reconstruction of multistation events. The 20-station network is expected to be fully operational by the end of 2018.
引用
收藏
页码:55 / 62
页数:8
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