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The Lorenz-Stenflo system is a four-dimensional continuous-time dynamical system, derived to model atmospheric acoustic-gravity waves in a rotating atmosphere.
Laplace proposed that this process was driven by the cooling of the hot, extended, rotating atmosphere of the primitive Sun.
The reasons for this are complex and have to do with the gravitational interactions of Venus, Earth, and the Sun, as well as the effects of Venus's massive rotating atmosphere.
Many physical phenomena, in the purely dispersive limit, are governed by this type of equation, such as the long waves on a thin liquid film [15], the Rossby waves in a rotating atmosphere [16], and the isolated vortex of drift waves in a three-dimensional plasma [17].
Conventional theory of atmospheric acoustic-gravity waves (AGWs) in flat rotating atmosphere (e.g., Gossard and Hooke 1975) provides polarization relations.
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Venus presents unique numerical and physical challenges because of its thick atmosphere, slow underlying solid body rotation, and super-rotating atmosphere.
However, because the planet is rotating underneath the atmosphere, and frictional forces arise as the planetary surface drags some atmosphere with it, the air flow from center to periphery is not direct, but is twisted due to the Coriolis effect, or the merely apparent force that arise when the observer is in a rotating frame of reference.
Laplace's model begins with the Sun already formed and rotating and its atmosphere extending beyond the distance at which the farthest planet would be created.
The coatings were deposited in a mixed Ar/N2 atmosphere rotating the substrate holder, located at the centre of the deposition chamber.
This no longer allows the spacecraft motion to be synchronized to the super-rotating atmosphere and affects the longitudinal coverage and the spatial resolution of images.
Although the latitude bands differ, this phenomenon is common to most rapidly rotating planets with atmospheres, including Venus, Mars, Jupiter and Saturn.
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