Astrophysics (Index)About

turbulence

(turbulent flow)
(irregular flow of a fluid)

Turbulence (or turbulent flow) is chaotic flow of a fluid. It is characterized by changes in flow velocity and pressure over space and time, and eddies, i.e., circular or swirling flows, often lasting only a short time. In contrast, a laminar flow has the fluid flowing in an organized fashion, potentially continuously. Turbulence in Earth atmosphere is of interest to astronomers because it is a contributor to seeing issues, and is a target of adaptive optics (AO). Turbulence also is a factor within the gas of some astronomical objects e.g., within stars or clouds: one means of detecting it is through analysis of spectral lines.


(physics,fluid dynamics)
Further reading:
https://en.wikipedia.org/wiki/Turbulence
https://glossary.ametsoc.org/wiki/Turbulence
https://www.weather.gov/source/zhu/ZHU_Training_Page/turbulence_stuff/turbulence/turbulence.htm
https://phys.libretexts.org/Bookshelves/University_Physics/Book%3A_University_Physics_(OpenStax)/Book%3A_University_Physics_I_-_Mechanics_Sound_Oscillations_and_Waves_(OpenStax)/14%3A_Fluid_Mechanics/14.09%3A_Viscosity_and_Turbulence

Referenced by pages:
alpha disk
core collapse supernova (CCSN)
Darcy velocity field
dense core
Doppler broadening
dynamo
giant planet formation
gravitational instability model
homopause
interstellar holography
kilometer size barrier
Kolmogorov spectrum
line broadening
Mach number
magnetic switchback
magnetorotational instability (MRI)
mixing length theory
molecular cloud turbulence
quenched galaxy
radio halo
Rayleigh number (Ra)
Reynolds decomposition
Reynolds number (Re)
seeing
spectral line
THEMIS
turbulent pressure
vortex
Wilson-Bappu effect

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