admissible region
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Sensors ◽  
2021 ◽  
Vol 21 (11) ◽  
pp. 3684
Author(s):  
Leonardo Cament ◽  
Martin Adams ◽  
Pablo Barrios

This paper presents a Bayesian filter based solution to the Space Object (SO) tracking problem using simulated optical telescopic observations. The presented solution utilizes the Probabilistic Admissible Region (PAR) approach, which is an orbital admissible region that adheres to the assumption of independence between newborn targets and surviving SOs. These SOs obey physical energy constraints in terms of orbital semi-major axis length and eccentricity within a range of orbits of interest. In this article, Low Earth Orbit (LEO) SOs are considered. The solution also adopts the Partially Uniform Birth (PUB) intensity, which generates uniformly distributed births in the sensor field of view. The measurement update then generates a particle SO distribution. In this work, a Poisson Labeled Multi-Bernoulli (PLMB) multi-target tracking filter is proposed, using the PUB intensity model for the multi-target birth density, and a PAR for the spatial density to determine the initial orbits of SOs. Experiments are demonstrated using simulated SO trajectories created from real Two-Line Element data, with simulated measurements from twelve telescopes located in observatories, which form part of the Falcon telescope network. Optimal Sub-Pattern Assignment (OSPA) and CLEAR MOT metrics demonstrate encouraging multi-SO tracking results even under very low numbers of observations per SO pass.


2020 ◽  
Vol 177 ◽  
pp. 246-257
Author(s):  
Han Cai ◽  
Islam Hussein ◽  
Moriba Jah

2020 ◽  
Vol 43 (10) ◽  
pp. 1927-1934
Author(s):  
John A. Gaebler ◽  
Penina Axelrad ◽  
Paul W. Schumacher

2020 ◽  
Vol 132 (10) ◽  
Author(s):  
Alessio Del Vigna

AbstractWhen an asteroid has a few observations over a short time span the information contained in the observational arc could be so little that a full orbit determination may be not possible. One of the methods developed in recent years to overcome this problem is based on the systematic ranging and combined with the Admissible Region theory to constrain the poorly-determined topocentric range and range-rate. The result is a set of orbits compatible with the observations, the Manifold Of Variations, a two-dimensional compact manifold parametrised over the Admissible Region. Such a set of orbits represents the asteroid confidence region and is used for short-term hazard predictions. In this paper we present the Manifold Of Variations method and make a detailed analysis of the related probabilistic formalism.


2019 ◽  
Vol 1247 ◽  
pp. 012038
Author(s):  
Daniela Espitia Mosquera ◽  
Edwin Andrés Quintero Salazar
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