410 likes | 665 Views
Breaking of symmetry in atmospheric flows. Enrico Deusebio 1 and Erik Lindborg 2 1 DAMTP, University of Cambridge, Cambridge 2 Linné FLOW Centre, Royal institute of Technology, Stockholm 21th February 2014. Symmetry and asymmetry.
E N D
Breaking of symmetry in atmospheric flows Enrico Deusebio1and Erik Lindborg2 1 DAMTP, University of Cambridge, Cambridge 2 Linné FLOW Centre, Royal institute of Technology, Stockholm 21th February 2014
Symmetry and asymmetry Symmetry often observed in nature and generally thought as a sign of perfection and beauty
Symmetry and asymmetry Symmetry often observed in nature and generally thought as a sign of perfection and beauty Used by mathematicians to simplify their systems
Symmetry and asymmetry Symmetry often observed in nature and generally thought as a sign of perfection and beauty Used by mathematicians to simplify their systems Also used in numerical simulations in order to reduce the computational cost
Asymmetry in atmospheric flows Are atmospheric flows symmetric?
Asymmetry in atmospheric flows Are atmospheric flows symmetric?
Asymmetry in atmospheric flows Are atmospheric flows symmetric?
Asymmetry in atmospheric flows Are atmospheric flows symmetric?
Asymmetry in atmospheric flows Are atmospheric flows symmetric? WHY? Coriolis terms (not symmetry invariant) Can this be observed at small scales?
Helicity (Moffatt & Tsinober, 1992)
Helicity Velocity (Moffatt & Tsinober, 1992)
Helicity Vorticity (Moffatt & Tsinober, 1992)
Helicity (Moffatt & Tsinober, 1992) Invariant of the Euler equations, thus conserved apart from viscous effects
Helicity (Moffatt & Tsinober, 1992) Invariant of the Euler equations, thus conserved apart from viscous effects AS ENERGY
Helicity (Moffatt & Tsinober, 1992) Invariant of the Euler equations, thus conserved apart from viscous effects AS ENERGY Both positive and negative values can be attained
Helicity (Moffatt & Tsinober, 1992) Invariant of the Euler equations, thus conserved apart from viscous effects AS ENERGY Both positive and negative values can be attained DIFFERENTLY FROM ENERGY
Turbulent Ekman boundary layers Recent numerical simulations of turbulent Ekman layers up to Standard numerics using pseudo-spectral codes
Budget equations Energy dissipation Energy injection
Budget equations Energy dissipation Energy injection
Budget equations Energy dissipation Energy injection Helicity dissipation Helicity injection
Budget equations Mean field helicity Turbulent helicity Production Transport Pressure Dissipation Rotation
Budget equations Mean field helicity Turbulent helicity Production Transport Pressure Dissipation Rotation Conversion from mean to turbulent helicity
Budget equations Mean field helicity Turbulent helicity Production Transport Pressure Dissipation Rotation Viscous dissipation of helicity
Budget equations Mean field helicity Turbulent helicity Production Transport Pressure Dissipation Rotation Transport of helicity from one place to another
Budget equations Mean field helicity Turbulent helicity Production Transport Pressure Dissipation Rotation Transport of helicity due to the pressure terms
Budget equations Mean field helicity Turbulent helicity Production Transport Pressure Dissipation Rotation Transport of helicity due to rotation
Budget equations Production Transport Pressure Dissipation Rotation
Budget equations Production Transport Pressure Dissipation Rotation
The helicity cascade Injection of helicity Helicity dissipation
Asymmetry in atmospheric flows Are atmospheric flows symmetric? WHY? Coriolis terms (not symmetry invariant) Can this be observed at small scales?
Asymmetry in atmospheric flows Are atmospheric flows symmetric? WHY? Coriolis terms (not symmetry invariant) Can this be observed at small scales? YES, WE CAN!
Ekman boundary layers Balance between viscous and Coriolis terms Geostrophic Wind far from surface
Budget equations In steady conditions the total helicity is determined by a balance between the injection (due to the pressure gradient) and the viscous destruction Total helicity injection
Turbulent Ekman boundary layers Recent numerical simulations of turbulent Ekman layers up to Standard numerics using pseudo-spectral codes