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The size dependence is well interpreted by a model of radial energy distribution in the ion track.
Considering the contact area of the APPLEs on the FW and the radial energy transport between the APPLEs, FW heat load profile can be analyzed.
However, when disk luminosity is close to or exceeds the Eddington luminosity, the standard disk model breaks, and we have to consider the "slim disk" solution in which radial energy advection is dominant.
Figure 5 Radial energy influx profile of an APS source.
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In this work, we achieve a unique separation by assuming the orthogonality of the two parts in terms of the radial SV energy at the CMB.
We have avoided the non-uniqueness in decomposing the SV into two parts violating and satisfying the necessary condition, by assuming the orthogonality of the two parts in terms of radial SV energy integrated over the CMB.
Figure 5 illustrates the change in variation of the radial confinement energy across the length of the nanowire (depicted in Fig. 1) as the magnetic field strength is increased.
In the absence of the magnetic field, the sinusoidal deformity affects the radial confinement energies drastically.
The solvation free energy, radial distribution functions (RDFs) and water structures are investigated to study the swelling process.
It consists of two basic components: an inducer like an axial-flow rotor, and the radial blades where energy is imparted by centrifugal force.
During the dipolarisation phase the importance of electric fields has been emphasized with the Salammbô 4D model (latitude, longitude, radial distance and energy) (Bourdarie et al.; 1997a).
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