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In this section, we present the results which are obtained by solving numerically the set of basic equations described in Section 2 over a wide range of wind strength, as well as the radial mass distribution parameter γ (see Eq. (1)).
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The sample is subdivided by straw type, and coherent size, type and mass distribution parameters are reported for the entire sample.
The nonlinear model describing the system is used to derive an adaptive fault tolerant control law, based on Lyapunov stability theorem, in the presence of unknown, slow-varying satellite mass distribution and solar parameter.
Our model structure estimates ancestral average body mass and the variance of the ancestral body mass distribution, and allows either parameter to increase or decrease as a function of time.
The resulting aerodynamic parameters and mass distribution allow calculating a realistic 6D re-entry trajectory.
The aim of the present study is to investigate the thermal behavior of the protoplanetary disk exposed to stellar radiation and the stellar wind over a wide range of three principal parameters: the strength of the stellar wind, the parameters describing the mass distribution of the disk, and the velocity law of the stellar wind.
Fig. 12 Loss mass distribution, after the final round of parameter estimation.
We found a strong influence of these parameters on both molecular mass distribution and recombination processes in the plasma volume.
First, we will see in detail the effect of the wind strength under the fixed parameters describing the disk mass distribution and the velocity distribution of the stellar wind.
It suggests that the physical parameters of the body (size, mass distribution, and inertial properties of the body segments) can partly explain the behavior of the postural sway.
Segment circumferences were each collected at 2 locations in order to approximate the segment mass distribution using geometric relationships, and hence the inertial parameters of the segments (30).
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com