1.4 thermal wind balance ug plug (2) into (1) ug ug=0 y

Slides:



Advertisements
Similar presentations
Chapter 1: What is the Mesoscale? Mesoscale energy sources.
Advertisements

The Quasi-Geostrophic Omega Equation (without friction and diabatic terms) We will now develop the Trenberth (1978)* modification to the QG Omega equation.
What Makes the Wind Blow?
Midlatitude Cyclones Equator-to-pole temperature gradient tilts pressure surfaces and produces westerly jets in midlatitudes Waves in the jet induce divergence.
Chapter 10 Mid-latitude Cyclones Chapter 10 Mid-latitude Cyclones.
Extratropical Cyclones – Genesis, Development, and Decay Xiangdong Zhang International Arctic Research Center.
Lackmann, Chapter 1: Basics of atmospheric motion.
Chapter 15 Global Circulation: Big Picture: Idealized View Ferrel cell Polar cell.
Leila M. V. Carvalho Dept. Geography, UCSB
Vorticity.
Next Week: QUIZ One question from each of week: –9 normal lectures + global warming lecture –Over main topic of lecture and homework Multiple choice,
ATM S 542 Synoptic Meteorology Overview Gregory J. Hakim University of Washington, Seattle, USA Vertical structure of the.
MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 12 Midlatitude Cyclones Dr. Eugene Cordero San Jose State University.
Why do we have storms in atmosphere?. Mid-atmosphere (500 hPa) DJF temperature map What are the features of the mean state on which storms grow?
Chapter 1: What is the Mesoscale? Mesoscale energy sources.
AOS 100: Weather and Climate Instructor: Nick Bassill Class TA: Courtney Obergfell.
AOSS 321, Winter 2009 Earth Systems Dynamics Lecture 12 2/17/2009
Lessons 22,23,24 Upper Level Winds
Atms 4320 / 7320 – Lab 7 The Thermal Wind: Forecasting Problems and the Analysis of Fronts.
The General Circulation of the Atmosphere Tapio Schneider.
Lecture 9: Atmospheric pressure and wind (Ch 4) we’ve covered a number of concepts from Ch4 already… next: scales of motion pressure gradient force Coriolis.
Chapter 8 Wind and Weather. Wind –The local motion of air relative to the rotating Earth Wind is measured using 2 characteristics –Direction (wind sock)
Class #13 Monday, September 27, 2010 Class #13: Monday, September 27 Chapter 7 Global Winds 1.
General Circulation & Thermal Wind
Things to look for on the weather maps Visible and IR satellite images (& radar too): Look at cloud movements and locations - do they correlate with what.
The simplifed momentum equations
Potential Vorticity and its application to mid-latitude weather systems We have developed the following tools necessary to diagnose the processes that.
ATS/ESS 452: Synoptic Meteorology Friday 09/26/2014 Continue Review Material Geopotential Thickness Thermal Wind.
AOSS 401, Fall 2006 Lecture 19 October 26, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
The simplest theoretical basis for understanding the location of significant vertical motions in an Eulerian framework is QUASI-GEOSTROPHIC THEORY QG Theory:
PRECIPITATION PROCESSES AT FRONTS. POSSIBLE CONDITIONS PRESENT AT FRONT 1.Air ahead of the front is stable to all forms of instability Forcing mechanism.
A&OS C110/C227: Review of thermodynamics and dynamics IV
Dynamics: Nov. 11. Which are non-divergent, irrational ??
ADVENTURE IN SYNOPTIC DYNAMICS HISTORY
Thickness and Thermal Wind /aos101/wk12.html /aos101/wk12.html.
Class #18 Wednesday, February 18, Class #18: Wednesday, February 18 Waves aloft Introduction to Oceanography Ocean Currents.
FLUID ROTATION Circulation and Vorticity. Arbitrary blob of fluid rotating in a horizontal plane Circulation: A measure of the rotation within a finite.
METR March Review Hydrostatic balance Ideal gas law p = ρ R d T v, ρ = p / R d T v Take layer average virtual temperature, R and g as constants.
AOSS 401, Fall 2006 Lecture 9 September 26, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
ATS/ESS 452: Synoptic Meteorology
Synoptic Scale Balance Equations Using scale analysis (to identify the dominant ‘forces at work’) and manipulating the equations of motion we can arrive.
METR February Why use Temp. Advection? The temperature at a location may change in two ways: –The air parcel which is being sampled might.
Section 8 Vertical Circulation at Fronts
Jets Dynamics Weather Systems – Fall 2015 Outline: a.Why, when and where? b.What is a jet streak? c.Ageostrophic flow associated with jet streaks.
ATS/ESS 452: Synoptic Meteorology Friday 08 January 2016 Review Material Overview of Maps Equations of Motion Advection Continuity.
Potential vorticity and the invertibility principle (pp ) To a first approximation, the atmospheric structure may be regarded as a superposition.
ATS/ESS 452: Synoptic Meteorology Monday 12 January 2015 (Short?) Weather Discussion Review Material Equations of Motion Advection Continuity.
1 This is the footer Midlatitude Weather systems Geraint Vaughan University of Manchester NCAS Director of Observations.
Atmospheric Dynamics Suzanne Gray (University of Reading) With thanks to Alan Gadian and Geraint Vaughan. Basic dynamical concepts.
Class #17 Monday, February 16, Class #17: Monday, February 16 Surface pressure and winds Vertical motions Jet streams aloft.
SO254 - Advection.
ATM S 542 Synoptic Meteorology Overview
Synoptic Scale Balance Equations
Temperature Advection
Vorticity Vertical component of vorticity: i.e., the rotation about the local vertical There are three types of vorticity used in geophysical fluid dynamics.
Thickness and Thermal Wind
A jet stream (or jet) is a narrow current of strong winds.
Thermal Wind, Temperature Advection, and Doppler
Midlatitude Weather Systems ATMS 301
A jet stream (or jet) is a narrow current of strong winds.
The Course of Synoptic Meteorology
Thermal Wind, Temperature Advection, and Doppler
Mesoscale Dynamics Introduction.
Richard B. Rood (Room 2525, SRB)
Richard B. Rood (Room 2525, SRB)
Richard B. Rood (Room 2525, SRB)
The Course of Synoptic Meteorology
AIR MASS SOURCE REGIONS
Presentation transcript:

1.4 thermal wind balance ug plug (2) into (1) ug ug=0 y geostrophic wind hypsometric eqn ug plug (2) into (1) ug greater thickness ug=0 lower thickness y finite difference expression: this is the thermal wind: an increase in wind with height due to a temperature gradient The thermal wind blows ccw around cold pools in the same way as the geostrophic wind blows ccw around lows. The thermal wind is proportional to the T gradient, while the geostrophic wind is proportional to the pressure (or height) gradient.

Let’s verify qualitatively that climatological temperature and wind fields are roughly in thermal wind balance. For instance, look at the meridional variation of temperature with height (in Jan)

Around 30-45 ºN, temperature drops northward, therefore westerly winds increase in strength with height.

thermal wind The meridional temperature gradient is large between 30-50ºN and 1000-300 hPa Therefore the zonal wind increases rapidly from 1000 hPa up to 300 hPa.

Question: Why, if it is colder at higher latitude, doesn’t the wind continue to get stronger with altitude ?

There is definitively a jet ...

Answer: above 300 hPa, it is no longer colder at higher latitudes... tropopause

Z500

Z500-Z1000

baroclinicity The atmosphere is baroclinic if a horizontal temperature gradient is present The atmosphere is barotropic if NO horizontal temperature gradient exists the mid-latitude belt typically is baroclinic, the tropical belt barotropic The atmosphere is equivalent barotropic if the temperature gradient is aligned with the pressure (height Z) gradient in this case, the wind increases in strength with height, but it does not change direction equivalent barotropic baroclinic geostrophic wind at various levels cold cold warm warm height gradient temperature gradient

1.4.2 Geostrophic T advection: cold air advection (CAA) & warm air advection (WAA)

highlight areas of cold air advection (CAA) & warm air advection (WAA)

WAA & CAA

geostrophic temperature advection: the solenoid method geostrophic wind: fatter arrow: larger T gradient cold lower height Z greater Z warm geo. temperature advection is: greater Z the magnitude is: lower Z cold warm the smaller the box, the stronger the temp advection

Thermal wind and geostrophic temperature advection Let us use the natural coordinate and choose the s direction along the thermal wind (along the isotherms) and n towards the cold air. Rotating the x-axis to the s direction, the advection equation is: local T change T advection where is the average wind speed perpendicular to the thermal wind. The sign of      + - VT warm cold

Thermal wind and temperature advection WARM VT VT COLD - + COLD WARM WAA CAA If the wind veers with height,      is positive and there is warm advection. If the wind is back with height,      is negative and there is cold advection.

thermal wind and temperature advection Procedure to estimate the temperature advection in a layer: On the hodograph showing the upper- and low-level wind, draw the thermal wind vector. Apply the rule that the thermal wind blows ccw around cold pools, to determine the temperature gradient, and the unit vector n (points to cold air) 3. Plot the mean wind      , perpendicular to the thermal wind. Note that      is positive if it points in the same direction as n. Then the wind veers with height, and you have warm air advection. If there is warm advection in the lower layer, or cold advection in the upper layer, or both, the environment will become less stable.

example COLD WARM y 5°C n s 10°C x veering wind  warm air advection between 1000-850 hPa

friction-induced near-surface convergence into lows/trofs

1.5 vorticity shear and curvature vorticity

Hovmoller diagrams (Fig. 1.20)

time scales of atmospheric variability Lovejoy 2013, EOS “what is climate”: Dynamics and types of scaling variability: representative temperature series from weather (space scales and timescales), macroweather, and climate scales (bottom to top, respectively). Each sample is 720 points long and was normalized by its overall range (bottom to top: 2.86 K, 27.8 K, 16.84 K, and 7.27 K; dashed lines indicate means). The resolutions are 280 meters, 1 hour, 20 days, and 1 century, and the data are from an aircraft at 200 mbar (north Pacific); Lander, Wyoming; the twentieth century reanalysis (20CR, 75°N, 100°W); and Vostok (Antarctica). Lovejoy 2013, EOS

time scales of atmospheric variability Temperature standard deviations S(Δt). (top left) Grid point scale (2° × 2°) daily fluctuations globally averaged from the 20CR. (bottom left) The same fluctuations, but for the global average (brown line), and the average of the three in situ global surface series (red line) as well as S(Δt) from three multiproxy Northern Hemisphere reconstructions (green line) [see Lovejoy and Schertzer, 2012a]. (right) The European Project for Ice Coring in Antarctica (EPICA) Antarctic series at a 50-year resolution. Also shown is the interglacial window (rectangle) and reference slopes H = −0.4, +0.4, −0.1, and −0.5 (Gaussian white noise). Lovejoy 2013, EOS

(1) Scales of atmospheric motion Note two spectral extremes: (a) A maximum at about 2000 km (b) A minimum at about 500 km [shifted x10 to right] inertial subrange 1000 100 10 1 wavelength [km] Gage and Nastrom (1985)

Energy cascade synoptic scale FA=free atmos. BL=bound. layer Big whirls have little whirls that feed on their velocity; and little whirls have lesser whirls, and so on to viscosity.                   -Lewis Fry Richardson FA=free atmos. BL=bound. layer L = long waves WC = wave cyclones TC=tropical cyclones cb=cumulonimbus cu=cumulus CAT=clear air turbulence From Ludlam (1973)

Scales of atmospheric motion Markowski & Richardson 2010, Fig. 1.1

Scales of atmospheric motion Air motions at all scales from planetary-scale to microscale explain weather: planetary scale: low-frequency (10 days – intraseasonal) e.g. blocking highs (~10,000 km) – explains low-frequency anomalies size such that planetary vort adv > relative vort adv hydrostatic balance applies synoptic scale: cyclonic storms and planetary-wave features: baroclinic instability (~3000 km) – deep stratiform clouds smaller features, whose relative vort adv > planetary vort adv size controlled by b=df/dy mesoscale: waves, fronts, thermal circulations, terrain interactions, mesoscale instabilities, upright convection & its mesoscale organization: various instabilities – synergies (100-500 km) – stratiform & convective clouds time scale between 2p/N and 2p/f hydrostatic balance usually applies microscale: cumuli, thermals, K-H billows, turbulence: static instability (1-5 km) – convective clouds Size controlled by entrainment and perturbation pressures no hydrostatic balance 2p/N ~ 2p/10-2 ~ 10 minutes 2p/f = 12 hours/sin(latitude) = 12 hrs at 90°, 24 hrs at 30°