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As a result, to quantitatively determine the D major of the NW arrays, leaky mode resonance is initially adopted to calculate the respective resonant wavelengths for different diameters of NWs [2].
The results show that flexural mode resonance is largely avoided for the considered design topology.
These radial properties of amplitude and cross-phase imply that the fundamental cavity mode resonance is excited in the plasmasphere.
Currently, plasmaspheric cavity mode resonance is the most popular source mechanism for Pi2 pulsations observed at low to mid latitudes.
Another key feature for harmonic cavity mode resonance is the radial (latitudinal) profile of the cross-phase.
An qualitative understanding of such broadband enhanced absorption effect, which is attributed to the guided mode resonance, is presented.
Similar(54)
In Fig. 12, which was adapted from Figure 1 of Takahashi et al. (2003b), a two-dimensional box-shaped magnetosphere for the cavity mode resonance was considered wherein the magnetic field was (i) straight and uniform, (ii) directed along the z-axis, and (iii) fixed to the northern and southern boundaries (ionosphere) of the box.
The radial profile of the harmonic cavity mode resonance was shown by Luo et al. (2011) who used data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) multisatellite observations and low-latitude ground observations, which were performed at approximately the same longitude on the nightside.
A qualitative physical explanation of this broadband absorption enhancement, which results from the leaky waveguide modes resonance, is presented.
The first mode resonances are found between 16 and 52 kHz with response amplitudes ranging from 62.5 to 420 μm.
Guided mode resonances are experimentally demonstrated in fabricated III-nitride gratings, opening the possibility to achieve the interaction between the excited light and the grating structure through guided mode resonance.
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