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  • Infrared Detection of Space Debris and the Applicability of Observation Data

    Paper number

    IAC-19,A6,1,9,x50804

    Author

    Mr. Marcel Becker, Germany, TU Braunschweig

    Coauthor

    Prof. Enrico Stoll, Germany, TU Braunschweig, Institute of Space Systems

    Coauthor

    Dr. Carsten Wiedemann, Germany, TU Braunschweig, Institute of Space Systems

    Coauthor

    Mr. Andre Horstmann, Germany, TU Braunschweig

    Coauthor

    Mr. Manuel Schubert, Germany, TU Braunschweig, Institute of Space Systems

    Coauthor

    Mr. Paul Wagner, Germany, German Aerospace Center (DLR)

    Coauthor

    Mr. Wolfgang Riede, Germany, DLR, German Aerospace Center

    Coauthor

    Mr. Lorenz Böttcher, Germany, TU Braunschweig

    Year

    2019

    Abstract
    Detection and observation od low Earth objects are essential for the knowledge of the space situation. Observations can be done by telescopes or radars. Optical telescopes have various advantages over the radar. Such as low acquisition and operating costs at high precision.\\
    
    Thus, a significant disadvantage of optical systems is their limited availability, since they rely on clear skies and operation only during the twilight phase. The latter is due to the fact that objects for optical visibility must be illuminated by the sun while the station is obscure.\\
    
    However, if the optical observations are shifted to the infrared range, it becomes possible to observe objects in the shadow of the earth. Depending on the material properties and trajectory, the object can also emit infrared radiation in the Earth's shadow (reflected radiation from the earth or its own thermal radiation). So the number of optical detections can be increased by additional detections in the IR range. This has been proven in a research study.\\
    
    For this purpose, an IR detection model was developed by the TU Braunschweig in cooperation with the DLR Stuttgart. This model includes:
    
    \begin{itemize}
    \item Emission-Model: To determine the IR signature of objects in space
    \item Disturbance-Model: To calculate the background IR radiation and absorption of Earth atmosphere
    \item Sensor-Model: To simulate specific IR sensors (variant ranges)
    \end{itemize}
    
    With the help of the developed model, it is possible to simulate and evaluate measurement campaigns. To compare the information gain by IR sensors compared to the conventional use of telescopes and radars. 
    
    For the simulation campaigns are the technical properties of the sensor and local conditions varied. So it is possible to make qualitative statements regarding the positioning of an IR sensor. This analysis is based on known locations of relevant existing facilities for the acquisition of the space situation.
    
    
    The results of the simulated campaigns and the IR simulation model shall be presented in this publication
    Abstract document

    IAC-19,A6,1,9,x50804.brief.pdf

    Manuscript document

    IAC-19,A6,1,9,x50804.pdf (🔒 authorized access only).

    To get the manuscript, please contact IAF Secretariat.