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Bottom panel: mass density distribution obtained with ADER-Cons.
Top panel: mass density distribution obtained with ADER-Prim.
It is assumed that mass density distribution in the medium follows a power law of the radial distance from the point of explosion.
The solution to the tails problem can only derive from abandoning completely the probabilistic interpretation and from adopting a more physical and realistic interpretation relating 'what is out there' to, e.g., the mass density distribution over the whole universe.
Adding a correction calculated from the empirical relation to the NRLMSISE-00 model reference leads to a better prediction of storm-time thermospheric mass density distribution.
The difference between the converged 1D solution and the relaxed 2D solutions with (N_{r}=800) (dotted lines) and (N_{r}=1600) (dashed lines) is illustrated in Figure 6 which shows the mass density distribution.
With the help of STAR (Spatial Triaxial Accelerometer for Research) accelerometer measurements on board CHAMP (Challenging Minisatellite Payload), the global distributions of total mass density changes at about 400 km height during major magnetic storms are studied, aiming to improve the capability of current thermospheric model for predicting the storm-time mass density distribution.
Figure 22 shows the rest-mass density distribution on the ((x,y)) plane for this test.
Two-dimensional rest-mass density distribution relative to the initial data maximum value on the equatorial ((x,y)) plane at time (t=1text167~M_{odot}) for the migration test.
Two-dimensional rest-mass density distribution relative to the initial data maximum value on the equatorial ((x,y)) plane at time (t=4text485~M_{odot}) for the dynamical TOV test.
Two-dimensional rest-mass density distribution relative to the initial data maximum value on the equatorial ((x,y)) plane at time (t=4text300~M_{odot}) for the rotating star test.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com