Utilizing Poynting vectors to emphasis low-wavenumber information for FWI

2017 ◽  
Author(s):  
Zhiyang Liu ◽  
Jie Zhang
Keyword(s):  
1971 ◽  
Vol 39 (7) ◽  
pp. 837-838 ◽  
Author(s):  
Emerson M. Pugh
Keyword(s):  

Author(s):  
Yuan Bin Liu ◽  
Jun Qiu ◽  
Rong Jin ◽  
Lin Hua Liu

In this work, we investigated the reflection properties of artificial opals composed of submicron silica spheres with diverse structural parameters and under the effect of light in different states. Furthermore, the primary rules how the reflection properties of artificial opals convert as these factors changing have been revealed clearly. These factors can take effects in changing the shape, value, and position of the peak of the hemispherical reflectance of artificial opals. Then we got the distribution and propagation process of the Poynting vectors corresponding to the positions of the diffraction peak and the low reflectance in the artificial opals at normal and oblique incidence of P-polarization. Comparing with the theoretical interpretation which is a little complicated and nonobjective, this paper will provide a visual result to explain the reason why the structure has high reflectance in some spectral ranges.


2008 ◽  
Vol 57 (5) ◽  
pp. 1014-1022 ◽  
Author(s):  
E. Suzuki ◽  
S. Arakawa ◽  
M. Takahashi ◽  
H. Ota ◽  
K.I. Arai ◽  
...  

2002 ◽  
Vol 49 (9) ◽  
pp. 1553-1566 ◽  
Author(s):  
C. ALBERDI ◽  
S. ALFONSO ◽  
M. BERROGUI ◽  
J. M. DIÑEIRO ◽  
C. SÁENZ ◽  
...  

1994 ◽  
Vol 09 (02) ◽  
pp. 167-179 ◽  
Author(s):  
M.D. ROBERTS

Solutions to gravity with quadratic Lagrangians are found for the simple case where the only nonconstant metric component is the lapse N and the Riemann tensor takes the form [Formula: see text] thus these solutions depend on cross terms in the Riemann tensor and therefore complement linearized theory where it is the derivatives of the Riemann tensor that matter. The relationship of this metric to the null gravitational radiation metric of Peres is given. Gravitational energy Poynting vectors are constructed for the solutions and one of these, based on the Lanczos tensor, supports the indication in the linearized theory that nonnull gravitational radiation can occur.


Author(s):  
Yu-Bin Chen ◽  
Chien-Jing Chen

This work numerically investigated the interaction between two resonances: the magnetic polariton (MP) and surface plasmon polariton (SPP). A reflectance contour plot of deep silver slit arrays quantitatively identified the MP mode and the SPP excitation’s dependence on the period. Five arrays were selected for their SPP excitation wavenumber that approached and then diverged from that of an MP mode. Reflectance spectra from arrays showed dips associated with the two resonances between 10000 cm−1 and 25000 cm−1. Both the magnitude and corresponding wavenumber of nearby dips were modified by the interaction. Moreover, a third dip might appear or two dips might merge into a wider valley when two resonance excitation wavenumbers are close enough. The interaction was further elucidated with electromagnetic fields, Poynting vectors, and the energy density corresponding to representative reflectance dips.


1997 ◽  
Vol 44 (1) ◽  
pp. 69-81 ◽  
Author(s):  
Bruce W. Shore ◽  
Lifeng Li ◽  
Michael D. Feit

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