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Modeling Climate Change in the Laboratory Mikls Vincze MTA-ELTE Theoretical Physics Research Group ELTE Institute of Physics, von Krmn Laboratory for Enviromental Flows (HU), BTU Cottbus-Senftenberg, Department of Aerodynamics and Fluid


  1. Modeling Climate Change in the Laboratory Miklós Vincze MTA-ELTE Theoretical Physics Research Group ELTE Institute of Physics, von Kármán Laboratory for Enviromental Flows (HU), BTU Cottbus-Senftenberg, Department of Aerodynamics and Fluid Mechanics (DE) Intl. Conf. On Teaching Physics Innovatively – Budapest, Hungary August, 2015

  2. First of all: What kind of laboratory?  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 1998 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large-scale (atmosphere, ocean) flow structures  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research  Website (www.karman.elte.hu) almost up-to-date …  Video (courtesy index.hu)

  3. First of all: What kind of laboratory?  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 2002 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large- scale (atmosphere, ocean) flow structures  Website (www.karman.elte.hu) almost up-to-date …  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research

  4. First of all: What kind of laboratory?  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 1998 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large-scale (atmosphere, ocean) flow structures  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research  Website (www.karman.elte.hu) almost up-to-date …  Video (courtesy index.hu) LINK: http://index.hu/video/2010/09/26/kutatok_ejszakaja_2010/ [from 02:00 to 04:00]

  5. Hot topics  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 2002 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large-scale (atmosphere, ocean) flow structures  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research  Website (www.karman.elte.hu) almost up-to-date …  Video (courtesy: index.hu)

  6. Hot topics  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 2002 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large-scale (atmosphere, ocean) flow structures  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research  Website (www.karman.elte.hu) almost up-to-date …  Video (courtesy: index.hu)

  7. Hot topics  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 2002 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large-scale (atmosphere, ocean) flow structures  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research  Website (www.karman.elte.hu) almost up-to-date …  Video (courtesy: index.hu)

  8. Hot topics  A Laboratory for environmental flows (aka geophysical fluid dynamics), called Kármán Laboratory of Eötvös University (hidden abbreviation: K.ár.mán . – can also stand for ‚ Environmental Flow maniacs (?)’ in Hungarian)  Founded in 2002 by Imre M. Jánosi, Tamás Tél, Gábor K. Szabó, and Viktor Horváth  The principle of hydrodynamical similarity enables modeling large-scale (atmosphere, ocean) flow structures  Demonstration, teaching (incl. High school groups, Researchers ’ Night, etc.), research  Website (www.karman.elte.hu) almost up-to-date …  Video (courtesy: index.hu)

  9. Why to use such a lab for research purposes nowadays? - #1: Lab experiments as ‚ analog computers ’ “ It alw lways bothers me e tha that, accord rding to the the law laws as s we e under erstand the them today, it it takes a computing mach chine an inf infinite number of f log logical oper erations to fig figure out what goes on in in no matter r how tin tiny a reg region of f spa space, and no matter how tiny a region of time.” - R. P. Feynman (In: The Character of Physical Law, 1967)

  10. Why to use such a lab for research purposes nowadays? - #2: Test-bed for „ Nimitz class ” complex flow models • A som somewhat provocative statement: : The e opera rational numerical methods and models for r wea eather fora rasting and cli climate pre rediction can be e validated only in in the the la lab! ! (if if at t all ll)

  11. So, what can be done? • How to separate parametrization (discretization, etc.) errors from those that originate from our incomplete understanding of the system • Let’s build/find a physical system which behaves like the atmosphere, but still much simpler, and all the governing equations are correctly understood!

  12. A minimal model of mid-latitude weather - A large variety of the typical atmospheric phenomena of the mid- latitudes are primarily driven by two factors only. - Rotation + meridional temperature difference ≈ weather - Let’s use a differentially heated rotating circular tank for method validation!

  13. A minimal model of mid-latitude weather • A dif ifferentia ially ly heated cyli cylindrical l tan ank, mounted on on a a turntable tu le. “Rotating annulus” Geometrical parameters (Cottbus): a = 45 mm b = 120 mm d = 135 mm

  14. A minimal model of mid-latitude weather • A dif ifferentia ially ly heated cyli cylindrical l tan ank, mounted on on a a turntable tu le. “Rotating annulus” Geometrical parameters (Cottbus): a = 45 mm b = 120 mm d = 135 mm

  15. A minimal model of mid-latitude weather • A dif ifferentia ially ly heated cyli cylindrical l tan ank, mounted on on a a turntable tu le. “Rotating annulus” Geometrical parameters (Budapest): a = 45 mm b = 150 mm d = 40 mm

  16. Basics: baroclinic instability

  17. Basics: baroclinic instability “Sideways convection” – no threshold in Δ T (i.e. No ‘critical Rayleigh number’) Any temperature difference can initiate the flow

  18. Basics: baroclinic instability “Sideways convection” – no threshold in Δ T (i.e. No ‘critical Rayleigh number’) Any temperature difference can initiate the flow

  19. Basics: baroclinic instability

  20. Basics: baroclinic instability Rotation!

  21. Baroclinic instability Rotation! Zonal flow (thermal wind) Geostrophic theory: Tilted density surfaces

  22. Baroclinic instability Rotation! Zonal flow (thermal wind) Geostrophic theory: Tilted density surfaces

  23. Baroclinic instability Baroclinic instability! Rotation! Zonal flow (thermal wind) Geostrophic theory: Tilted density surfaces

  24. Baroclinic waves - control parameters: • rotation rate, radial temperature difference - Different planetary atmospheres can be modelled • Venus: slow rotation, zonal flow • Earth: fast rotation  Coriolis effect  cyclones (“weather”)

  25. Baroclinic waves, planetary analogies - control parameters: • rotation rate, radial temperature difference - Different planetary atmospheres can be modelled • Venus: slow rotation, zonal flow • Earth: fast rotation  Coriolis effect  cyclones (“weather”)

  26. The regime diagram (after Fultz)

  27. The regime diagram (after Fultz)

  28. The regime diagram (after Fultz)

  29. The regime diagram (after Fultz)

  30. Preliminary results

  31. Preliminary results

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