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At frequencies below the transition frequency, infragravity waves continuously radiate acoustic-gravity waves into the upper atmosphere.
At frequencies below the transition frequency, IGWs continuously radiate their energy into the upper atmosphere in the form of acoustic-gravity waves (AGWs).
In the first domain, below the transition frequency or for low frequencies, the orthotropic sandwich panel has a classical isotropic plate behavior.
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The lines in this figure assume the lasers are detuned by one linewidth below the bare-atom transition frequency.The ground-state polarizability of the Ca (Rb) atom is larger (smaller) than the excited state, leading to blue-shifting (red-shifting) of the transition frequency as the ion approaches.
Importantly, alterations in the transition frequency patterns were also observed.
We show that, at frequencies below a certain transition frequency of about 3 mHz, infragravity waves continuously radiate their energy into the upper atmosphere in the form of acoustic-gravity waves.
These waves cease to be surface ones and become leaky waves at frequencies below a certain depth-dependent transition frequency of the order of 3 mHz.
The measured transition frequencies differ substantially from simple theoretical predictions.
Transition frequency was calculated by subtracting the start from the end frequency of the call stem (fig. 1).
We can then compute the significance-weighted transition frequencies by multiplying each transition frequency with its significance.
To test a transition frequency for statistical significance, we use the Monte Carlo sampling method described below.
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