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  • Tacking the association and tracking problems using directional statistics to model uncertainty

    Paper number

    IAC-18,A6,IP,9,x45085

    Author

    Mr. Shambo Bhattacharjee, United Kingdom, University of Leeds

    Coauthor

    Prof. John T Kent, United Kingdom, University of Leeds

    Coauthor

    Mr. Weston Faber, United States, Applied Defense Solutions, Inc.

    Coauthor

    Dr. Islam Hussein, United States, Applied Defense Solutions, Inc.

    Coauthor

    Prof. Moriba Jah, United States, The University of Texas at Austin

    Year

    2018

    Abstract
    One of the main concerns in space situational awareness is to keep
    track of the large number of resident space objects (RSOs), both
    satellites and debris, orbiting the earth.  Observations typically
    take the form of angles-only measurements from ground-based
    telescopes.  Two specific tasks are the identification of objects and
    the tracking of objects.  Ideas from directional statistics have been
    developed recently to help tackle both of these problems.  The first
    contribution is a new ``Fisher-Bingham-Kent (FBK)'' distribution on the unit sphere, which often can be used to describe the predicted angular
    position and its uncertainty at a specific time of an RSO.  A key
    property of the distribution is that it can describe uncertainty
    tightly spread along an arc of a great circle.  The FBK distribution
    has proved very useful for the association problem in which an
    observation at a particular time might be compatible with the
    predicted positions (plus uncertainties) of two or more objects in a
    catalog or library.  It is desired, if possible, to associate the
    observation with just one of the objects.
    
    A second problem is tracking or filtering.  The objective is to update
    successively the prediction of the state (plus uncertainty) of an RSO
    as new observations are made.  Under an assumption of Gaussianity, the
    problem can be tackled using Kalman filter ideas.  Unfortunately, the
    Gaussianity assumption can fail badly using standard coordinate
    systems in astrodynamics (such as earth-centered inertial, Keplerian
    and equinoctial).  A new ``Adapted STructural (AST)'' coordinate system
    has been developed, under which approximate Gaussianity hold under a
    wide range of circumstances.  An unscented Kalman filter in AST
    coordinates (UKF-AST) has been successfully implemented. Further, the AST-UKF is computationally much faster than particle filters.
    Abstract document

    IAC-18,A6,IP,9,x45085.brief.pdf

    Manuscript document

    IAC-18,A6,IP,9,x45085.pdf (🔒 authorized access only).

    To get the manuscript, please contact IAF Secretariat.