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  2. Atmospheric instability - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_instability

    Atmospheric instability is a condition where the Earth's atmosphere is considered to be unstable and as a result local weather is highly variable through distance and time. [ clarification needed ] [ 1 ] Atmospheric instability encourages vertical motion, which is directly correlated to different types of weather systems and their severity.

  3. Convective available potential energy - Wikipedia

    en.wikipedia.org/wiki/Convective_available...

    Positive CAPE will cause the air parcel to rise, while negative CAPE will cause the air parcel to sink. Nonzero CAPE is an indicator of atmospheric instability in any given atmospheric sounding, a necessary condition for the development of cumulus and cumulonimbus clouds with attendant severe weather hazards.

  4. Eady model - Wikipedia

    en.wikipedia.org/wiki/Eady_model

    First, the model assumes the atmosphere is composed of fluid obeying quasi-geostrophic motion. Second, the model assumes a constant Coriolis parameter . The model also assumes a constant static stability parameter and that fluctuations in the density of the air are small (obeys the Boussinesq approximation ).

  5. Baroclinic instabilities in the ocean - Wikipedia

    en.wikipedia.org/wiki/Baroclinic_instabilities...

    A baroclinic instability is a fluid dynamical instability of fundamental importance in the atmosphere and ocean. It can lead to the formation of transient mesoscale eddies, with a horizontal scale of 10-100 km. [1] [2] In contrast, flows on the largest scale in the ocean are described as ocean currents, the largest scale eddies are mostly created by shearing of two ocean currents and static ...

  6. Kelvin–Helmholtz instability - Wikipedia

    en.wikipedia.org/wiki/Kelvin–Helmholtz_instability

    A KH instability rendered visible by clouds, known as fluctus, [2] over Mount Duval in Australia A KH instability on the planet Saturn, formed at the interaction of two bands of the planet's atmosphere Kelvin-Helmholtz billows 500m deep in the Atlantic Ocean Animation of the KH instability, using a second order 2D finite volume scheme

  7. Hydrodynamic stability - Wikipedia

    en.wikipedia.org/wiki/Hydrodynamic_stability

    In fluid dynamics, hydrodynamic stability is the field which analyses the stability and the onset of instability of fluid flows. The study of hydrodynamic stability aims to find out if a given flow is stable or unstable, and if so, how these instabilities will cause the development of turbulence . [ 1 ]

  8. Geophysical Fluid Dynamics Laboratory Coupled Model

    en.wikipedia.org/wiki/Geophysical_Fluid_Dynamics...

    Atmosphere The atmospheric component of the CM2.X models employs a 24-level atmosphere with horizontal resolution of 2° in east–west and 2.5° in north–south directions. This resolution is sufficient to resolve the large mid-latitude cyclones responsible for weather variability.

  9. Brunt–Väisälä frequency - Wikipedia

    en.wikipedia.org/wiki/Brunt–Väisälä_frequency

    In atmospheric dynamics, oceanography, asteroseismology and geophysics, the Brunt–Väisälä frequency, or buoyancy frequency, is a measure of the stability of a fluid to vertical displacements such as those caused by convection. More precisely it is the frequency at which a vertically displaced parcel will oscillate within a statically ...