On the interaction of gravity waves and thermal tides in the middle atmosphere Fabian Senf, Erich Becker Leibniz Institute for Atmospheric Physics, Kühlungsborn.

Slides:



Advertisements
Similar presentations
INTROTHE MODELTHE DATATHE COMPARISONOUTLOOK 1 Atmospheric waves workshop 9-10 November, 2011 ESTEC, Noordwijk (NL)E 2011 Manuela Sornig [1] RIU – Department.
Advertisements

Atmospheric waves from the point of view of a modeler Alexander Medvedev.
F.Nimmo EART164 Spring 11 EART164: PLANETARY ATMOSPHERES Francis Nimmo.
REFERENCES Alexander et al (2008): Global Estimates of Gravity Wave Momentum Flux from HIRDLS Observations. JGR 113 D15S18 Ern et al (2004): Absolute Values.
The role of the mean flow and gravity wave forcing in the observed seasonal variability of the migrating diurnal tide. David A. Ortland NorthWest Research.
The Problem of Parameterization in Numerical Models METEO 6030 Xuanli Li University of Utah Department of Meteorology Spring 2005.
Doppler signatures of the atmospheric circulation of hot Jupiters Adam Showman University of Arizona Jonathan Fortney (UCSC), Nikole Lewis (Univ. Arizona),
The Atmospheric Boundary Layer (ABL) over Mesoscale Surface Heterogeneity 25 June 2009 Song-Lak Kang Research Review.
Observations of High Frequency GWs observed in mesospheric airglow, and the implication to the GW imposed zonal stress and the residual circulation Gary.
Modeling the quasi-biennial oscillations Modeling the quasi-biennial oscillations of the zonal wind in the equatorial stratosphere. Kulyamin D.V. MIPT,
By studying the case with QBO signal only, the model reproduces the previous observation that QBO signal of column ozone at equator is anti-correlated.
Atmospheric Analysis Lecture 3.
How to move the gravity-wave parameterization problem forward? Some thoughts Ted Shepherd Department of Physics University of Toronto NCAR TIIMES Gravity-Wave.
Convection in Neutron Stars Department of Physics National Tsing Hua University G.T. Chen 2004/5/20 Convection in the surface layers of neutron stars Juan.
An introduction to the Inter-tropical Convergence Zone (ITCZ) Chia-chi Wang Dept. Atmospheric Sciences Chinese Culture University Acknowledgment: Prof.
Solar Forcing on Climate Through Stratospheric Ozone Change Le Kuai.
THE HADLEY CIRCULATION (1735): global sea breeze HOT COLD Explains: Intertropical Convergence Zone (ITCZ) Wet tropics, dry poles Problem: does not account.
Suggested components of a GW parameterization design that includes the major sources and modifying influences: 1. individual source spectra in amplitude,
Determination of upper atmospheric properties on Mars and other bodies using satellite drag/aerobraking measurements Paul Withers Boston University, USA.
The General Circulation of the Atmosphere Background and Theory.
The General Circulation of the Atmosphere Tapio Schneider.
Warning! In this unit, we switch from thinking in 1-D to 3-D on a rotating sphere Intuition from daily life doesn’t work nearly as well for this material!
Gravity Waves Geraint Vaughan University of Manchester, UK
Solar Variability and Climate: From Mechanisms to Models
The Air-Sea Momentum Exchange R.W. Stewart; 1973 Dahai Jeong - AMP.
How do gravity waves determine the global distributions of winds, temperature, density and turbulence within a planetary atmosphere? What is the fundamental.
F.Nimmo EART164 Spring 11 EART164: PLANETARY ATMOSPHERES Francis Nimmo.
© Imperial College LondonPage 1 Solar Influence on Stratosphere-Troposphere Dynamical Coupling Isla Simpson, Joanna D. Haigh, Space and Atmospheric Physics,
AOSS 401, Fall 2006 Lecture 8 September 24, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
General Circulation of the Atmosphere Lisa Goddard 19 September 2006.
Observations and model data Fig. 1 Location of used meteor radar sites in the subtropical region: Learmonth at ° E, 22.2 °S (117.2 °E, 20 °S), Rarotonga.
*K. Ikeda (CCSR, Univ. of Tokyo) M. Yamamoto (RIAM, Kyushu Univ.)
Gravity Waves, Scale Asymptotics, and the Pseudo-Incompressible Equations Ulrich Achatz Goethe-Universität Frankfurt am Main Rupert Klein (FU Berlin) and.
Using GPS data to study the tropical tropopause Bill Randel National Center for Atmospheric Research Boulder, Colorado “You can observe a lot by just watching”
Momentum Equations in a Fluid (PD) Pressure difference (Co) Coriolis Force (Fr) Friction Total Force acting on a body = mass times its acceleration (W)
Vertical Wavenumber Spectrum of Gravity Waves at the Northern High Latitude Region in the Martian Atmosphere Hiroki Ando.
Modeling the Atmospheric Boundary Layer (2). Review of last lecture Reynolds averaging: Separation of mean and turbulent components u = U + u’, = 0 Intensity.
Neutral Winds in the Upper Atmosphere Qian Wu National Center for Atmospheric Research.
Richard Rotunno National Center for Atmospheric Research, USA Fluid Dynamics for Coastal Meteorology.
REFERENCES Alexander et al (2008): Global Estimates of Gravity Wave Momentum Flux from HIRDLS Observations. JGR 113 D15S18 Ern et al (2004): Absolute Values.
MESOSPHERE COUPLING THE ROLE OF WAVES AND TIDES. Spectra show that waves & tides of large amplitude dominate the MLT region A typical power spectrum of.
Sound speed in air: C S ∝ [T] 1/2 T[K] C S [m/s] Conv. Div. tendency of pressure & density >0
The Linear and Non-linear Evolution Mechanism of Mesoscale Vortex Disturbances in Winter Over Western Japan Sea Yasumitsu MAEJIMA and Keita IGA (Ocean.
Internal Wave Interactions with Time-Dependent Critical Levels Brian Casaday and J. C. Vanderhoff Department of Mechanical Engineering Brigham Young University,
Vertical Wavenumber Spectra of Gravity Waves in the Venus and Mars Atmosphere *Hiroki Ando, Takeshi Imamura, Bernd Häusler, Martin Pätzold.
Lecture Guidelines for GEOF110 Chapter 5 ( 2 hours) Chapter 6 (2 Hours) Ilker Fer Guiding for blackboard presentation. Following Pond & Pickard, Introductory.
Gravity waves generated by thunderstorms E. Blanc 1, T. Farges 1, J. Marty 1, A. Le Pichon 1, P. Herry 1 1 Commissariat Energie Atomique DASE/LDG Bruyères.
CITES 2005, Novosibirsk Modeling and Simulation of Global Structure of Urban Boundary Layer Kurbatskiy A. F. Institute of Theoretical and Applied Mechanics.
Kelvin Waves as Observed by the SABER Instrument on the TIMED Spacecraft Jeffrey M. Forbes, Xiaoli Zhang, Saburo Miyahara, Scott E. Palo, James Russell,
GITM and Non-hydrostatic processes Yue Deng Department of Physics University of Texas, Arlington.
中央大學大氣科學系 1 Transient Mountain Waves in an Evolving Synoptic-Scale Flow and Their Interaction with Large Scales Chih-Chieh (Jack) Chen, Climate and Global.
Richard Rotunno National Center for Atmospheric Research, USA Dynamical Mesoscale Mountain Meteorology.
NCAR Advanced Study Program (ASP) Seminar, February 13, Solar Semidiurnal Tide in the Atmosphere Jeff Forbes Department of Aerospace Engineering.
Class 8. Oceans Figure: Ocean Depth (mean = 3.7 km)
Inertia-Gravity waves and their role in mixing Geraint Vaughan University of Manchester, UK.
Atmospheric Circulation of hot Jupiters Adam Showman LPL Collaborators: J. Fortney, N. Lewis, L. Polvani, D. Perez-Becker, Y. Lian, M. Marley, H. Knutson.
Page 1© Crown copyright Cloud-resolving simulations of the tropics and the tropical tropopause layer Glenn Shutts June
Interannual to decadal variability of circulation in the northern Japan/East Sea, Dmitry Stepanov 1, Victoriia Stepanova 1 and Anatoly Gusev.
Results We first best-fit the zonal wind and temperature simulated in the 3D PlanetWRF using the semi- analytic 2D model with,,, and. See Fig 2. The similarity.
Dynamical Constraints on the Gravity Wave Source Spectrum Used in a Parameterization of Gravity Wave Forcing David Ortland NorthWest Research Associates.
May 2005 ICAM - MAP 1 Mountain-Wave Momentum Flux in an Evolving Synoptic-Scale Flow Chih-Chieh Chen, Dale R. Durran and Gregory J. Hakim Department of.
Atmospheric Gravity Waves
Gravity-wave breaking beyond traditional instability concepts U. Achatz Goethe-Universität Frankfurt am Main, Germany
AOSS 401, Fall 2006 Lecture 7 September 21, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
Impact of midnight thermosphere dynamics on the equatorial ionospheric vertical drifts Tzu-Wei Fang 1,2 R. Akmaev 2, R. Stoneback 3, T. Fuller-Rowell 1,2,
Using the Mars climate Database for aerobraking ( km)
Hurricane Vortex X L Converging Spin up Diverging Spin down Ekman
AOSS 321, Winter 2009 Earth System Dynamics Lecture 11 2/12/2009
Baroclinic and barotropic annular modes
Ling Wang and M. Joan Alexander
Presentation transcript:

On the interaction of gravity waves and thermal tides in the middle atmosphere Fabian Senf, Erich Becker Leibniz Institute for Atmospheric Physics, Kühlungsborn Ulrich Achatz Goethe University, Frankfurt (Main)

Introduction - Gravity waves and thermal tides in the middle atmosphere - On gravity – tidal wave interaction studies Model - Ray tracing method - Experiments of different complexity Results - modulation of gravity-wave frequencies and phase velocities - refraction of horizontal wave vector - amplitude of gravity-wave force - equivalent friction coefficients Overview: Fabian

zonally averaged HAMMONIA zonal wind and temperature for north winter dynamics of middle atmosphere Introduction: latitude altitude [km] latitude

zonally averaged HAMMONIA zonal wind and temperature for north winter dynamics of middle atmosphere Introduction: latitude altitude [km] latitudeBreite tropospheric sources gravity wave force meridional circulation adiabatic cooling adiabatic warming Fabian drives

Meso-scale gravity waves are essential for large-scale dynamics, but hardly resolved in complex circulation models! parameterizations with crude assumptions high-resolution, mechanistic modelling Fabian dynamics of middle atmosphere Introduction:

thermal tides planetary-scale buoyancy oscillations induced by solar heating sun heating tides north pole earth Introduction: Fabian

zonal wind amplitude meridional wind amplitude HAMMONIA diurnal tides as background (from Hauke Schmidt) Introduction: latitude altitude [km] total altitude [km] migratingnon-migrating

Introduction: Thermal tides induce extreme changes in the conditions for gravity wave propagation in the middle atmosphere. Fabian thermal tides interaction between gravity waves and thermal tides is not deeply understood and also not sufficiently investigated because most studies focus on the interaction between thermal tides and gravity-wave parameterizations!

Fabian Past Studies of the interaction between thermal tides and gravity-wave parameterizations: highly idealized models: Fritts & Vincent (1987), Lu & Fritts (1993) linear modeling: Forbes et. al. (1991); Miyahara & Forbes (1991,1994), McLandress (1997), Meyer (1997), Ortland & Alexander (2006) non-linear GCM results: Mayr et. al. (1998,2001), Akmaev (2001), McLandress (2002) Main outcome: shrinking of vertical phase structure but different effects on tidal amplitude (different source and turbulence parameterization seem to be responsible) But, with crude assumptions: gravity wave parameterizations in vertical columns assumed: stationarity of background flow and instantaneous adjustment Introduction:

Fabian Our strategy: relaxing of the assumptions made for gravity wave propagation successively including temporal and horizontal dependence of the background flow BUT, keeping other aspects as simple as possible!  highly simplified lower boundary conditions (or GW sources)  saturation at convective instability threshold to estimate turbulent diffusion coefficients Introduction: ray tracing of gravity waves

Ray tracing in thermal tidesModel: Fabian wave parcel group velocity c g ray tracing and wave parcel concept t = 1 h t = 6 ht = 10 h zonal wind profile altitude longitude c wave parcel: small volume of GW field ray tracing: following the path of wave parcel

Ray tracing in thermal tidesModel: Fabian ray tracing and wave parcel concept zonal wind profile c wave parcel: small volume of GW field ray tracing: following the path of wave parcel

Ray tracing equations and symmetries of WKB theory: transience  frequency modulation horizontal gradients  refraction vertical gradients Model: Fabian

Conventional GW Parametrization: transience  frequency modulation horizontal gradients  refraction vertical gradients Model: Fabian

RAPAGI – RAy PArametrization of Gravity wave Impacts: global ray tracing model for time-dependent flows conservation of wave action and diffusion according to simple saturation theory (Lindzen, 1981) Model: Fabian

gravity wave spectrum in use: 14 gravity wave fields in different directions: - horizontal wave length with about 400 km to 600 km - periods in the range of hours - momentum fluxes between 0.3 to 0.5 mPa c = 33 m/s c = 10 m/s Model: extremely simple, but reproduces average gravity wave forces

Ray tracing experiments: Model: Fabian full complex ray tracing simulation noREF simple ray tracing – simulation TS conventional vertical column transience included no transience, instantaneously adjusting horizontal refraction and propagation included no horizontal refraction and propagation increasing complexity

Vertical column thinking 15°S latitude (TS) expected height of strongest gravity wave forcing moves downward with tidal phase transient critical layers? Fabian Results: phase velocity altitude [km] velocity [m/s]

Fabian Results: Vertical column thinking is NOT appropriate for tides due to frequency modulation! less critical layer filtering! 15°S latitude (TS) phase velocity altitude [km] velocity [m/s] 15°S latitude (TS) altitude [km] velocity [m/s]

Understanding frequency modulation: simplified equations: Results: Fabian local positive tendency of wind leads to increase of phase speed local negative tendency of wind leads to decrease of phase speed t = 1 h t = 4 h

Fabian horizontal phase velocity follows the shape of the background (BG) wind (Contours: BG Wind) longitudinal variations of phase velocity longitude altitude [km] [m/s] Results:

Fabian meridional gradients of the zonal wind induce refraction of gravity waves into the jet maximum in which their travel time is minimized longitude latitude refraction of horizontal wave vectors Results:

latitude altitude [km] latitude average gravity wave flow arrows:average group velocity, colors:initial meridional position, contours:wind in wave direction Fabian Results: O W N S O W N S

latitude altitude [km] latitude Fabian O W N S O W N S average gravity wave flow arrows:average group velocity, colors:initial meridional position, contours:wind in wave direction Results:

meridional displacement displacements of 50° in latitude occur often! displacements larger than 100° in latitude are possible! Fabian Results:

Fabian amplitude of zonal diurnal gravity wave force latitude altitude [km] [m/s per day] conventional GW parameterizations extremely overestimate zonal GW drag amplitude simulations without horizontal refraction slightly overestimate zonal GW drag amplitude

Fabian tidal wind force e.g.180° phase shift projection on tidal wind force on tidal amplitude Results: phase relation between force and tides tidal wind e.g. 90° phase shift projection on tidal acceleration advancing of tide force on phase structure force

projections of the diurnal gravity wave force on - tidal wind  real part of equivalent friction coefficient if positive: local decrease of tidal amplitude - tidal acceleration  imaginary part of equivalent friction coefficent if negative: local vertical shrinking tidal phase structure Results: Fabian

Fabian conventional parameterizations extremely over-estimate the decrease of tidal amplitude latitude altitude [km] real parts of equivalent friction coefficients [per 10 6 s] Results:

conventional parameterizations mainly over-estimate the decrease of tidal vertical wave length Results: Fabian latitude altitude [km] imaginary parts of equivalent friction coefficients [per 10 6 s]

Summary: WKB theory and ray tracing has been used describing propagation and dissipation of a spectrum of GWs monthly averaged data + diurnal tides from HAMMONIA as background for GW propagation comparison with conventional GW parameterizations show:  overestimation of GW drag frequency modulation reduces diurnal gravity wave forces horizontal refraction leads to formation of wave guides and large meridional displacements GW drag induces decrease of tidal vertical wave length and amplitude Fabian Thank you for your attention!

Fabian THE END!

Breite Höhe [km] Fabian Ergebnisse: Refraktion des horizontalen Wellenvektors Westwind-Jet Ostwind-Jet NP / Winter SP / Sommer EQ u0u0 Schnitt in Stratopause

Fabian Ergebnisse: Refraktion des horizontalen Wellenvektors Westwind-Jet Ostwind-Jet NP / Winter SP / Sommer EQ u0u0