Demonstration of the PADRE spacecraft assessment mode. This analysis simulated the destructive re-entry of a 1000kg component-centric vehicle, modelled as a relatively simple structore comprising approximately 40 components. Re-entry is predicted from a circular sun-synchronous orbit of 130km altitude using the DRAMA v3.0.4 version of SESAM. Uncertainties in the initial true anomaly, atmosphere density, material properties, drag and heating coefficients are considered. A standard Monte-Carlo of between 2000 and 5000 simulations has been executed.
Sensitivity parameters |
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Correlation coefficient: -0.2523012022795629 Slope: -0.011236345667194387 N: 2000 |
Sensitivity parameters |
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Correlation coefficient: 0.044472254523806765 Slope: 0.00593930871716165 N: 2000 |
Sensitivity parameters |
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Correlation coefficient: 0.0035299645357404407 Slope: 0.0002755701627471307 N: 2000 |
Sensitivity parameters |
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Correlation coefficient: -0.3785837352392934 Slope: -0.07980723374249421 N: 2000 |
Sensitivity parameters |
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Correlation coefficient: 0.04223631987385087 Slope: 0.026699760053696574 N: 2000 |
Sensitivity parameters |
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Correlation coefficient: 0.007221390781830842 Slope: 0.0026684387125402473 N: 2000 |
ESA PADRE 2021