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- W2043136773 abstract "This paper shows the effect of self-shadowing on the coupled attitude–orbit dynamics of objects with high area-to-mass ratios (HAMR) in simulating standard multi layer insulation materials (MLI) as tilted single rigid sheets. Efficient and computationally fast self-shadowing methods have been developed. This includes an approximate self-shadowing method and a rapid exact self-shadowing method. Accuracy considerations are made and the effect of a chosen tessellation is shown. The coupled orbit–attitude perturbations of solar radiation pressure and Earth gravity field are taken into account. The results are compared to the attitude–orbit dynamics, when neglecting self-shadowing effects. An averaged physical shadow-map model is developed and compared to the full self-shadowing simulation. The combined effect of solar radiation pressure and self-shadowing leads to a rapid spin-up of the objects, even though they have uniform reflection properties. As a result, the observed brightness of these objects is subject to rapid changes." @default.
- W2043136773 created "2016-06-24" @default.
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- W2043136773 date "2014-02-01" @default.
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- W2043136773 title "Coupled orbit–attitude motion of high area-to-mass ratio (HAMR) objects including efficient self-shadowing" @default.
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- W2043136773 doi "https://doi.org/10.1016/j.actaastro.2013.11.017" @default.
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