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BEGIN:VEVENT
UID:20260520T043705-04-1459LBpI1r@https://astronomia.uc.cl/2jucext1/institu
 toastrofisica/
DTSTAMP:20260520T083705Z
DESCRIPTION:It is well known that when a fluid is thermally unstable\, conv
 ection can be the most efficient mechanism for mixing and energy transport
 . However\, the presence of a stable composition gradient can counteract a
 nd inhibit convection\, giving rise to an interesting phenomenon called do
 uble-diffusive convection - or semi-convection - which is characterized by
  layers of convective and diffusive zones. In this seminar\, I will discus
 s some of the main properties of semi-convection and its relevance to gas 
 giant planets. Finally\, I will show 2D hydrodynamical simulations of this
  process. https://astronomia.uc.cl/2jucext1/institutoastrofisica/en/instit
 uto-2/seminars/event/357-hydrodynamics-of-double-diffusive-convection-jose
 -rafael-fuentes-mcgill-university
DTSTART:20190621T171500Z
DTEND:20190621T174500Z
LOCATION:Seminar Room (Instituto de Astrofísica\, Pontificia Universidad Ca
 tólica\, Vicuña Mackenna 4860\, Santiago\, Chile)
SUMMARY:Hydrodynamics of double-diffusive convection (José Rafael Fuentes\;
  McGill University)
URL:https://astronomia.uc.cl/2jucext1/institutoastrofisica/en/instituto-2/s
 eminars/event/357-hydrodynamics-of-double-diffusive-convection-jose-rafael
 -fuentes-mcgill-university
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