1. Gravity Waves, Scale Asymptotics, and the Pseudo-Incompressible Equations Ulrich Achatz Goethe-Universität Frankfurt am Main Rupert Klein (FU Berlin) and Fabian Senf (IAP Kühlungsborn) 13.9.10

2. Gravity waves in the middle atmosphere

3. Gravity Waves in the Middle Atmosphere Becker und Schmitz (2003)

4. Gravity Waves in the Middle Atmosphere Becker und Schmitz (2003)

5. Gravity Waves in the Middle Atmosphere Becker und Schmitz (2003) Without GW parameterization

6. linear GWs in the Euler equations no heat sources, friction, … no rotation

7. linear GWs in the Euler equations no heat sources, friction, … no rotation are equivalent to

8. linear GWs in the Euler equations linearization about atmosphere at rest:

9. linear GWs in the Euler equations linearization about atmosphere at rest:

10. linear GWs in the Euler equations conservation of wave energy: linear equations satisfy

11. linear GWs in the Euler equations conservation of wave energy: linear equations satisfy conservation suggests:

12. linear GWs in the Euler equations isothermal atmosphere:

13. linear GWs in the Euler equations isothermal atmosphere: gravity waves sound waves

14. linear GWs in the Euler equations isothermal atmosphere: gravity waves sound waves GW polarization relations:

15. GW breaking in the atmosphere Conservation Instabilität in großen Höhen Impulsdeposition … Rapp et al. (priv. comm.)

16. GW breaking in the atmosphere Conservation Instability at large altitudes Impulsdeposition … Rapp et al. (priv. comm.)

17. GW breaking in the atmosphere Conservation Instability at large altitudes Turbulence Momentum deposition… Rapp et al. (priv. comm.)

18. GW Parameterizations multitude of parameterization approaches (Lindzen 1981, Medvedev und Klaassen 1995, Hines 1997, Alexander and Dunkerton 1999, Warner and McIntyre 2001) too many free parameters reasons : –…–… –insufficent knowledge: conditions of wave breaking basic paradigm: breaking of a single wave –Stability analyses (NMs, SVs) –Direct numerical simulations (DNS)

19. GW breaking

20. GW stability in the Boussinesq theory

21. Basic GW types Dispersionsrelation: Trägheitsschwerewellen (TSW): Hochfrequente Schwerewellen (HSW):

22. Basic GW types Dispersion relation: Inertia-gravity waves (IGW): High-frequent GWs (HGW): Coriolis parameter Stability

23. Basic GW types Dispersion relation: Inertia-gravity waves (IGW): High-frequent gravity waves (HGW): Coriolis parameter Stability

24. Basic GW types Dispersion relation: Inertia-gravity waves (IGW): High-frequent GWs (HGW): Coriolis parameter Stability

25. Traditional Instability Concepts static (convective) instability: amplitude reference (a>1) dynamic instability limited applicability to HGW breaking

26. Traditional Instability Concepts static (convective) instability: amplitude reference (a>1) dynamic instability limited applicability to HGW breaking

27. Traditional Instability Concepts static (convective) instability: amplitude reference (a>1) dynamic instability BUT: limited applicability to GW breaking

28. NM analysis, 2.5D-DNS

29. NMs: Growth Rates  = 70°) Achatz (2005, 2007b)

30. GW amplitude after a perturbation by a NM (DNS): Achatz (2005, 2007b)

31. Energetics not the gradients in z matter, but those in  ! instantaneous growth rate:

32. Energetics not the gradients in z matter, but those in  ! instantaneous growth rate:

33. Energetics not the gradients in z matter, but those in  ! instantaneous growth rate:

34. Energetics of a Breaking HGW with a 0 < 1 Strong growth perturbation energy: buoyancy instability Achatz (2007b)

35. Singular Vectors: normal modes: Exponential energy growth singular vectors: optimal growth over a finite time  (Farrell 1988, Trefethen et al. 1993) characteristic perturbations in a linear initial value problem:

36. NMs and SVs of an IGW (Ri > ¼!): growth within 5min Achatz (2005) Achatz and Schmitz (2006a,b)

37. Dissipation rate breaking IGW (a ¼): Measured dissipation rates 1…1000 mW/kg (Lübken 1997, Müllemann et al. 2003) Achatz (2007a)

38. Summary GW breaking In comparison to assumptions in GW parameterizations: GW breaking sets in at lower amplitudes, i.e. it sets in earlier (at lower altitudes)

39. Summary GW breaking In comparison to assumptions in GW parameterizations: GW breaking sets in at lower amplitudes, i.e. it sets in earlier (at lower altitudes) GW dissipation stronger than assumed, i.e. more momentum deposition

40. Soundproof Modelling and Multi-Scale Asymptotics Achatz, Klein, and Senf (2010)

41. GW breaking in the middle atmosphere Conservation Instability at large altitudes Momentum deposition… Rapp et al. (priv. comm.)

42. GW breaking in the middle atmosphere Conservation Instability at large altitudes Momentum deposition… Competition between wave growth and dissipation: –not in Boussinesq theory Rapp et al. (priv. comm.)

43. GW breaking in the middle atmosphere Conservation Instability at large altitudes Momentum deposition… Competition between wave growth and dissipation: –not in Boussinesq theory –Soundproof candidates: –Anelastic (Ogura and Philips 1962, Lipps and Hemler 1982) –Pseudo-incompressible (Durran 1989) Rapp et al. (priv. comm.)

44. GW breaking in the middle atmosphere Conservation Instability at large altitudes Momentum deposition… Competition between wave growth and dissipation: –not in Boussinesq theory –Soundproof candidates: –Anelastic (Ogura and Philips 1962, Lipps and Hemler 1982) –Pseudo-incompressible (Durran 1989) Rapp et al. (priv. comm.) Which soundproof model should be used?

45. Scales: time and space for simplicity from now on: 2D non-hydrostatic GWs: same spatial scale in horizontal and vertical characteristic wave number time scale set by GW frequency characteristic frequency dispersion relation for

46. Scales: time and space for simplicity from now on: 2D non-hydrostatic GWs: same spatial scale in horizontal and vertical characteristic length scale time scale set by GW frequency characteristic frequency dispersion relation for

47. Scales: time and space for simplicity from now on: 2D non-hydrostatic GWs: same spatial scale in horizontal and vertical characteristic length scale time scale set by GW frequency characteristic time scale dispersion relation for

48. Scales: time and space for simplicity from now on: 2D non-hydrostatic GWs: same spatial scale in horizontal and vertical characteristic length scale time scale set by GW frequency characteristic time scale dispersion relation for

49. Scales: velocities winds determined by polarization relations: what is ? most interesting dynamics when GWs are close to breaking, i.e. locally

50. Scales: velocities winds determined by polarization relations: what is ? most interesting dynamics when GWs are close to breaking, i.e. locally

51. Non-dimensional Euler equations using: yields

52. Non-dimensional Euler equations using: yields isothermal potential- temperature scale height

53. Scales: thermodynamic wave fields potential temperature:

54. Scales: thermodynamic wave fields potential temperature: Exner pressure:

55. Multi-Scale Asymptotics Additional vertical scale needed: and have vertical scale scale of wave growth is Therefore: Multi-scale-asymptotic ansatz also assumed:

56. Multi-Scale Asymptotics Additional vertical scale needed: and have vertical scale scale of wave growth is Therefore: Multi-scale-asymptotic ansatz also assumed:

57. Multi-Scale Asymptotics Additional vertical scale needed: and have vertical scale scale of wave growth is Therefore: Multi-scale-asymptotic ansatz also assumed:

58. Multi-Scale Asymptotics Additional vertical scale needed: and have vertical scale scale of wave growth is Therefore: Multi-scale-asymptotic ansatz also assumed:

59. Scale asymptotics Euler: results Hydrostatic, large-scale, background

60. Scale asymptotics Euler: results Hydrostatic, large-scale, background Momentum equations and entropy equations as in Boussinesq or anelastic theory

61. Scale asymptotics Euler: results Hydrostatic, large-scale, background Momentum equations and entropy equations as in Boussinesq or anelastic theory Exner-pressure equation: leading order incompressibility (Boussinesq) next order yields density effect on amplitude

62. Scale asymptotics: pseudo-incompressible equations scale-asymptotic analysis of

63. Scale asymptotics: pseudo-incompressible equations scale-asymptotic analysis of results:

64. Scale asymptotics: pseudo-incompressible equations scale-asymptotic analysis of results: same scale asymptotics as Euler such a result cannot be obtained from the anelastic equations

65. Scale asymptotics: anelastic equations scale-asymptotic analysis of

66. Scale asymptotics: anelastic equations results: scale-asymptotic analysis of

67. Scale asymptotics: anelastic equations results: scale-asymptotic analysis of

68. Scale asymptotics: anelastic equations results: scale-asymptotic analysis of anelastic equations only consistent if: i.e. potential-temperature scale >> Exner-pressure scale

69. Large-Amplitude WKB Achatz, Klein, and Senf (2010)

70. Large-amplitude WKB

73. Mean flow with only large-scale dependence

74. Large-amplitude WKB Wavepacket with large-scale amplitude wavenumber and frequency with large-scale dependence

75. Large-amplitude WKB

76. Wave induced mean flow

77. Large-amplitude WKB Harmonics of the wavepacket due to nonlinear interactions

78. Large-amplitude WKB collect equal powers in no linearization!

79. Large-amplitude WKB: leading order

80. dispersion relation and structure as from Boussinesq

81. Large-amplitude WKB: 1st order

82. Solvability condition leads to wave-action conservation (Bretherton 1966, Grimshaw 1975, Müller 1976)

83. Large-amplitude WKB: 1st order Solvability condition leads to wave-action conservation (Bretherton 1966, Grimshaw 1975, Müller 1976) Pseudo- incompressible divergence needed!

84. Large-amplitude WKB: 1st order, 2nd harmonics

86. 2nd harmonics are slaved

87. Large-amplitude WKB: 1st order, higher harmonics

89. higher harmonics vanish (nonlinearity is weak)

90. Large-amplitude WKB: mean flow

91. Horizontal flow horizontally homogeneous (non-divergent)

92. Large-amplitude WKB: mean flow No zero-order vertical flow

93. Large-amplitude WKB: mean flow No first-order potential temperature

94. Large-amplitude WKB: mean flow acceleration by GW- momentum-flux divergence

95. Large-amplitude WKB: mean flow acceleration by GW- momentum-flux divergence GWs induce lower- order potential temperature variations

96. Large-amplitude WKB: mean flow acceleration by GW- momentum-flux divergence GWs induce lower- order potential temperature variations p.-i. wave-correction not appearing in anelastic dynamics

97. Large-amplitude WKB: mean flow Wave-induced lower- order vertical flow vanishes

98. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and pseudo-incompressible equations no such result for anelastic theory conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

99. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and pseudo-incompressible equations no such result for anelastic theory conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

100. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and pseudo-incompressible equations no such result for anelastic theory conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

101. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and pseudo-incompressible equations no such result for anelastic theory conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

102. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and p.-i. equations no such result for anelastic theory conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

103. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and p.-i. equations no such result for anelastic theory conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

104. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and p.-i. equations no such result for anelastic theory large-amplitude WKB (consistent with p.i. equations) conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude

105. Summary multi-scale asymptotics: nonlinear dynamics of GWs near breaking linear theory used for obtaining scale estimates velocity thermodynamic wave fields unique small parameter: result: same asymptotics for Euler equations and p.-i. equations no such result for anelastic theory large-amplitude WKB (consistent with p.i. equations) conclusion: use pseudo-incompressible equations for studies of GW dynamics with altitude-dependent amplitude