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The method in particular allows a good simulation of transverse non-linearities, of field fall-offs and possible merging fields in configurations of neighboring magnets, while using realistic models of magnetic fields.
Theoretical models of magnetic reconnection have been traditionally developed within the framework of magnetohydrodynamics (MHD).
One- and two-dimensional models of magnetic field fluctuations and turbulence are widely used in space-, androphysicalaboratoryoratory contexts.
This article summarizes recent advances in this field that have resulted from the use of more realistic models of magnetic turbulence in space.
We believe that future physical models of magnetic activity and spectral emissions in the solar chromosphere and transition region may make quantitative predictions of temporal relationships among full-disk solar indices for comparison with analyses such as ours.
The implications of these observations for models of magnetic activity in late-type stars, of wind emission in early-type stars, and of X-ray production in the early stages of stellar evolution are briefly discussed.
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However, on the one hand, complex structure of the magnetically suspended gimbal introduces parametric uncertainties into modeling of magnetic suspension force, and the disturbance of magnetic fields brings the unmodeled force into dynamics of magnetically suspended gimbal.
Xie spent six years developing a kind of unified model of magnetic animal navigation.
This work focuses on the accurate thermal modeling of magnetic components for power converters.
In this class we will discuss the design and modeling of magnetic components, which are essential tasks in the development of high performance converters and study advanced applications.
These observations have important implications for the modeling of magnetic reconnection and particle acceleration.
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