Assessment of possible observation strategy in LEO regime

Paper number

IAC-13,A6,7,2,x19060

Author

Dr. Alessandro Vananti, Astronomical Institute University of Bern (AIUB), Switzerland

Coauthor

Prof. Thomas Schildknecht, Astronomical Institute University of Bern (AIUB), Switzerland

Coauthor

Mr. Gian Maria Pinna, ESA/ESAC, Spain

Coauthor

Dr. Tim Flohrer, European Space Agency (ESA), Germany

Year

2013

Abstract

The European Space Agency (ESA) is developing an independent system for Space Situational Awareness (SSA). One component of the draft architecture of the
system foresees a network of optical telescopes for observations in the GEO/MEO/LEO regions. The telescope network will survey and track objects up to a certain limiting magnitude and will allow the collection of
accurate orbits. Major design drivers are the requirements on coverage of the existing object population, timeliness for detecting particular events, such as, e.g., fragmentations, releases, or orbit maneuvers, and orbit accuracy for cataloguing.
In this work, a possible strategy for covering the upper LEO regime by optical observations is analyzed.
The visibility limitations of LEO objects observed from stations at different latitudes are evaluated. Coverage simulations of the existing LEO population are performed considering different numbers of sites. Using simulated LEO observations of selected test objects, the orbit determination accuracy depending on different observation intervals is examined.

Abstract document

IAC-13,A6,7,2,x19060.brief.pdf

Manuscript document

IAC-13,A6,7,2,x19060.pdf (🔒 authorized access only).

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