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Atmospheric Solitary Waves

Physica Scripta, 1975
We show that the hydrodynamic equations which govern the propagation of acoustic gravity waves can have shock-like solutions.
Dysthe, K. B., Stenflo, L.
openaire   +1 more source

Mirages with Atmospheric Gravity Waves

Light and Color in the Open Air, 1993
Mirages observed over an interval of time occasionally display slow variations that seem to be periodic.
W H, Lehn, W K, Silvester, D M, Fraser
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Waves in Atmospheres

1989
The flow of air in the atmosphere is neither steady in time nor constant in space, but rather is continually disturbed by wave-like motions occurring on spatial scales ranging from millimeters to thousands of kilometers, and on temporal scales ranging from seconds to weeks. Three basic types of waves can occur in the earth’s atmosphere: acoustic waves,
Alison F. C. Bridger, Richard E. Young
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Rogue wave in Titan’s atmosphere

Astrophysics and Space Science, 2011
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
El-Labany, S. K.   +4 more
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Are There Alfvén Waves in the Solar Atmosphere?

Science, 2007
The Sun's outer coronal layer exists at a temperature of millions of kelvins, much hotter than the solar surface we observe. How this high temperature is maintained and what energy sources are involved continue to puzzle and fascinate solar researchers.
Erdélyi, Róbert, Fedun, V.
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Submillimeter wave spectroscopy of the atmosphere

Journal of the Optical Society of America, 1976
The paper which will be read at this conference will be a review paper in the sense that it will discuss recent and current research in submillimetre atmospheric spectroscopy within an historical framework. This Digest is intended as a guide to the topics which will be considered in the paper.
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Nonlinear waves in the solar atmosphere

Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2005
In this paper, we give a brief review of the contemporary theory of nonlinear waves in the solar atmosphere. The choice of topics reflects personal interests of the author. Historically the theory of nonlinear waves was first applied to the solar atmosphere to explain the chromospheric and coronal heating.
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Waves in the Atmosphere

2001
In the previous chapters, we have already found wavelike dynamical manifestations in the atmosphere such as Rossby waves. These waves are a consequence of the conservation of absolute vorticity in the sense that we have considered the effect of Earth’s rotation but not the presence of gravity.
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Atmospheric interfacial waves

Physics of Fluids A: Fluid Dynamics, 1992
Waves at the interface of a two-layer fluid are considered. The fluid in the lower layer is incompressible with constant density and is flowing irrotationally. In the upper layer, the fluid is stationary but compressible, and corresponds to an isothermal atmosphere with a density profile that decreases exponentially with height.
Forbes L.K., Belward S.R.
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Atmospheric and lithospheric wave guides

1990
Norman A. Haskell was basically interested in understanding the physical processes observed on the earth. He tried to keep the essential structure of the atmosphere and earth in his models. For that reason he modified the atmosphere with gradients and the upper portion of the solid earth with homogeneous layers, which was then the commonly accepted ...
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