Redigerer Rayleigh-Taylor-ustabilitet

'''Rayleigh–Taylor ustabilitet''', også kalt '''RT ustabilitet''' er en [[ustabilitet]] i et [[Grensesnitt (kjemi)|grensesnitt]] mellom to [[fluid]]er av forskjellig [[tetthet]] som inntreffer når en lettere fluid dytter en tyngre fluid. Ustabiliteten er oppkalt etter [[Lord Rayleigh]] og [[G. I. Taylor]].<ref name=Sharp84>{{Cite journal|
author=Sharp, D.H.|
title=An Overview of Rayleigh–Taylor Instability|
journal=Physica D|
volume=12|
issue=1|
date=1984|
pages=3–18|
doi=10.1016/0167-2789(84)90510-4|bibcode = 1984PhyD...12....3S |
url=https://digital.library.unt.edu/ark:/67531/metadc1104671/}}</ref><ref name=Drazin_50_51>
[[Philip Drazin|Drazin]] (2002) pp. 50–51.</ref><ref>{{Scholarpedia | title=Rayleigh–Taylor instability and mixing | urlname=Rayleigh-Taylor_instability_and_mixing | curator=David Youngs }}</ref> Eksempler er oppførselen til vann som heves over [[Jordens gravitasjonsfelt]],<ref name=Drazin_50_51/> [[soppsky]]er liksom de som stammer fra [[vulkanutbrudd]] og atmosfæriske [[atomeksplosjon]]er,<ref>{{Cite web|url=https://gizmodo.com/why-nuclear-bombs-create-mushroom-clouds-1468107869|title = Why Nuclear Bombs Create Mushroom Clouds| date=20. november 2013 }}</ref> [[supernova]]-eksplosjoner hvor den ekspanderende kjernegassen akselreres innn  i tykkere gass fra skallet,<ref>{{cite journal | author=Wang, C.-Y. | author2= Chevalier R. A. | name-list-style=amp | title=Instabilities and Clumping in Type Ia Supernova Remnants | arxiv=astro-ph/0005105v1 | date=2000 | doi=10.1086/319439 | volume=549 | issue= 2 | journal=The Astrophysical Journal | pages=1119–1134 | bibcode=2001ApJ...549.1119W| s2cid= 15244583 }}</ref><ref>{{Cite book | contribution=Supernova 1987a in the Large Magellanic Cloud | first1=W. | last1=Hillebrandt | first2=P. | last2=Höflich | title=Stellar Astrophysics | editor=R. J. Tayler | publisher=[[CRC Press]] | date=1992 | isbn=978-0-7503-0200-5 | pages=249–302 }}. See page 274.</ref> ustabiliteter i plasmafusjonsraktorer og<ref>{{Cite journal | first1=H. B. | last1=Chen | first2=B. | last2=Hilko | first3=E. | last3=Panarella | title=The Rayleigh–Taylor instability in the spherical pinch | journal=Journal of Fusion Energy | volume=13 | issue=4 | date=1994 | doi=10.1007/BF02215847 | pages=275–280 |bibcode = 1994JFuE...13..275C | s2cid=122223176 }}</ref> innnesluttet treg fusjon.<ref>{{Cite journal | first1=R. | last1=Betti | first2=V.N. | last2=Goncharov | first3=R.L. | last3=McCrory | first4=C.P. | last4=Verdon | title=Growth rates of the ablative Rayleigh–Taylor instability in inertial confinement fusion | journal= Physics of Plasmas | volume=5 | issue=5 | date=1998 | pages=1446–1454 |bibcode = 1998PhPl....5.1446B |doi = 10.1063/1.872802 }}</ref>

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[[Kategori:Fluiddynamikk]]