Resonant mode coupling for deriving optical resonances in stacked grating structures

2010 ◽  
Author(s):  
Thomas Weiss ◽  
Nikolay A. Gippius ◽  
Richard Taubert ◽  
Gérard Granet ◽  
Sergei G. Tikhodeev ◽  
...  
2010 ◽  
Vol 18 (7) ◽  
pp. 7569 ◽  
Author(s):  
Nikolay A. Gippius ◽  
Thomas Weiss ◽  
Sergei G. Tikhodeev ◽  
Harald Giessen

1987 ◽  
Author(s):  
G. Francis ◽  
A. Bers ◽  
A. K. Ram

1995 ◽  
Vol 155 ◽  
pp. 331-332
Author(s):  
G. Handler ◽  
D. O’Donoghue ◽  
D. A. H. Buckley ◽  
O. Giovannini ◽  
S. O. Kepler ◽  
...  

The variability of CD-24 7599 (V=11.48 mag) was discovered by JCC during observing run XCOV7 of the Whole Earth Telescope (WET, Nather et al. 1990) network in February, 1992. The star was observed as an additional target and 117 hours of high-quality temporal spectroscopic observations were obtained.Our analysis of these data revealed the presence of 7 independent pulsation modes between 27.0 and 38.1 cycles per day (313 – 441 μHz) with semiamplitudes of 2.1 – 10.2 milli-modulation amplitudes (mma). We showed that peaks at linear combination frequencies detected in the power spectra were not due to eigenmodes excited to visible amplitude by resonant mode coupling.


2015 ◽  
Vol 579 ◽  
pp. A133 ◽  
Author(s):  
S. Barceló Forteza ◽  
E. Michel ◽  
T. Roca Cortés ◽  
R. A. García

1977 ◽  
Vol 19 (9) ◽  
pp. 811-816 ◽  
Author(s):  
M Gros ◽  
P Bertrand ◽  
G Baumann

Author(s):  
Thomas Weiss ◽  
Nikolay A. Gippius ◽  
Gérard Granet ◽  
Sergei G. Tikhodeev ◽  
Richard Taubert ◽  
...  

1979 ◽  
Vol 53 ◽  
pp. 359-373 ◽  
Author(s):  
W. Dziembowski

AbstractAttention is focused on those aspects of the theory that may be relevant in understanding the nature of ZZ Ceti-type variable white dwarfs. Recent calculations show that the opacity mechanism can drive a large variety of oscillation modes, including the ones that fit observed periods. An estimate of nonlinear effects shows that resonant mode coupling plays a dominant role in determining the finite amplitude behaviour of oscillations and is also probably responsible for rapid amplitude changes observed in these variables.


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