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Details of Grant 

EPSRC Reference: GR/M05706/01
Title: DIRECT MONTE CARLO SIMULATION OF MICRO DEBRIS
Principal Investigator: Stark, Professor JPW
Other Investigators:
Researcher Co-Investigators:
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Department: School of Engineering & Materials Scienc
Organisation: Queen Mary University of London
Scheme: Standard Research (Pre-FEC)
Starts: 01 December 1998 Ends: 30 November 2000 Value (£): 97,742
EPSRC Research Topic Classifications:
Eng. Dynamics & Tribology
EPSRC Industrial Sector Classifications:
No relevance to Underpinning Sectors
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Panel History:  
Summary on Grant Application Form
Our Direct Simulation Monte Carlo (DSMC) model, originally developed under SERC grant GR/J 73636 describing the evolution of space debris will be extended to incorporate micro debris particles in the range 10 microns to 1mm. This extension will enhance risk assessment capabilities for future satellite systems with particular improvement in describing non-catastrophic collisions and the general deterioration of satellite exposed surfaces. The current interest in developing more robust thermal control blankets, could benefit from improved prediction methods of risk assessment, given that existing models of the environment underestimate collision rates between micro-particles and surfaces, and thus under-predict the replacement frequency for shuttle windows caused by such collisions. We will adopt the results of our ongoing programme of micro-debris generation mechanisms (partly funded by DERA), to provide a statistical description of micro-particles for inclusion in the DSMC model. Validation of this new model will be achieved by comparison with data derived from returned surfaces. We will use the model to examine the orbital lifetime of micro debris wakes, and the consequential influence these have on the further production of debris via collisions with solar arrays. We will seek to define appropriate design requirements covering micro-particle fluences, which could be adopted for surfaces exposed in specific LEO orbits.
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