2022
DOI: 10.1007/s00376-021-1244-2
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Variations in Amplitudes and Wave Energy along the Energy Dispersion Paths for Rossby Waves in the Quasigeostrophic Barotropic Model

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Cited by 5 publications
(3 citation statements)
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“…The ray demonstrates the propagation of the perturbation energy and differs from the phase propagation. Along the ray, the potential, kinetic, and magnetic energies can be solved, and their interaction with the basic flow and the basic magnetic field can be discussed (e.g., similar studies for Rossby waves can be seen in Li et al 2021b, 2022and Li & Kang 2022. Therefore, we can also apply the energy dispersion of magnetic Rossby waves to interpret the observed events involving the magnetic field.…”
Section: Discussionmentioning
confidence: 99%
“…The ray demonstrates the propagation of the perturbation energy and differs from the phase propagation. Along the ray, the potential, kinetic, and magnetic energies can be solved, and their interaction with the basic flow and the basic magnetic field can be discussed (e.g., similar studies for Rossby waves can be seen in Li et al 2021b, 2022and Li & Kang 2022. Therefore, we can also apply the energy dispersion of magnetic Rossby waves to interpret the observed events involving the magnetic field.…”
Section: Discussionmentioning
confidence: 99%
“…The results show that the variabilities of the East Asian winter and summer monsoon systems are the variablities of circulation seeing from their phenomena, but these variabilities are also the variations of quasi-stationary planetary waves according to their mechanisms. Currently, this theory is developing and expanding, and it has wide applications not only in the study on atmospheric circulation dynamics at middle and high latitudes but also in the study on the dynamics of typhoon genesis and evolution in tropical regions [46][47][48][49][50][51]. Moreover, the nonlinear effects of the energy dispersion of Rossby wave in atmosphere and the nonlinear interactions of different quasi-stationary planetary wave trains also need to be further investigated.…”
Section: Conclusion and Discussionmentioning
confidence: 99%
“…Simultaneously, in the formed X-H• • • Y, stabilized complex forces of the X-H bond and H• • • Y interaction seem to promote the positioning of the X-H bond in the plane and therefore out-of-plane bending modes are more energetically expensive. Since the wavenumber is directly proportional to the energy [109], a shift toward a higher wavenumber is observed for the bending modes upon hydrogen bond formation. The opposing behavior of the stretching and bending modes upon HB formation is shown schematically in Figure 7.…”
Section: Water Influence On Carbonyl Region-ftirmentioning
confidence: 99%