The sea-breeze circulation Part II: Effect of Earth’s rotation Reference: Rotunno (1983, J. Atmos. Sci.)

Slides:



Advertisements
Similar presentations
Section 2: The Planetary Boundary Layer
Advertisements

Unit 9: Circulation Patterns of the Atmosphere
Section 5: Kelvin waves 1.Introduction 2.Shallow water theory 3.Observation 4.Representation in GCM 5.Summary.
The sea-breeze circulation Part II: Effect of Earth’s rotation Reference: Rotunno (1983, J. Atmos. Sci.)
The sea/land-breeze circulation Part I: Development w/o Earth rotation.
Günther Zängl, DWD1 Improvements for idealized simulations with the COSMO model Günther Zängl Deutscher Wetterdienst, Offenbach, Germany.
Horizontal Convective Rolls Asai papers & Simulations w/ ARPS.
Atmospheric Motion ENVI 1400: Lecture 3.
Wind.
Natural Environments: The Atmosphere
Rossby wave propagation. Propagation… Three basic concepts: Propagation in the vertical Propagation in the y-z plane Propagation in the x-y plan.
Dynamics and Thermodynamics Demonstration Model (DTDM)
Atmospheric Circulation
A few summary slides AOS C115/228 - Spring Thermals: buoyancy pressure dynamic pressure decomposition of pdyn.
The General Circulation of the Atmosphere Background and Theory.
The General Circulation of the Atmosphere Tapio Schneider.
Atmospheric temperature
Define Current decreases exponentially with depth. At the same time, its direction changes clockwise with depth (The Ekman spiral). we have,. and At the.
Chapter 12 Section 6 Wind.
Friday 2/14 – Inv. Science Warm-up 1. In what direction does the Earth rotate? (think sunrise and sunset) 2. What is the degree we tilt at? 3. What was.
Basic Meteorology Concepts. Spheres of the Earth.
Chapter 6 Atmospheric Forces and Wind
Lecture 14 4 February 2005 Atmospheric and Oceanic Circulations (continued) Chapter 6.
Upper ocean currents, Coriolis force, and Ekman Transport Gaspard-Gustave de Coriolis Walfrid Ekman.
Richard Rotunno National Center for Atmospheric Research, USA Fluid Dynamics for Coastal Meteorology.
On the Linear Theory of the Land and Sea Breeze MPO 663 project, Falko Judt based on Rotunno, 1983 Sun and Orlanski, 1981.
Session 3, Unit 5 Dispersion Modeling. The Box Model Description and assumption Box model For line source with line strength of Q L Example.
What set the atmosphere in motion?
Internal Wave Interactions with Time-Dependent Critical Levels Brian Casaday and J. C. Vanderhoff Department of Mechanical Engineering Brigham Young University,
Atmospheric Circulation
Atmospheric Motion SOEE1400: Lecture 7. Plan of lecture 1.Forces on the air 2.Pressure gradient force 3.Coriolis force 4.Geostrophic wind 5.Effects of.
Marine Physics Chapters 8, 9, 10 JUST COPY WHAT IS UNDERLINED!!!!!!
NATS 101 Section 13: Lecture 16 Why does the wind blow? Part II.
Model Task 5: Implementing the 2D model ATM 562 Fall 2015 Fovell (see updated course notes, Chapter 13) 1.
Adjoint models: Examples ATM 569 Fovell Fall 2015 (See course notes, Chapter 16) 1.
Composition/Characterstics of the Atmosphere 80% Nitrogen, 20% Oxygen- treated as a perfect gas Lower atmosphere extends up to  50 km. Lower atmosphere.
The Atmosphere in Motion
The sea-breeze circulation Part I: Development w/o Earth rotation.
Chapter 17 continued  The horizontal movement of air from high pressure to low pressure  Moderates surface temperatures  Distributes moisture 
The Sun’s Path. Summer Solstice (approximately June 20-21) North Pole: The North Pole (90 degrees north latitude) receives 24 hours of daylight, as it.
The TEKS Know that climatic interactions exist among Earth, ocean, and weather systems (A) recognize that the Sun provides the energy that drives.
Atmospheric Pressure Ch The atmosphere has weight (14.7 lb/sq in.) 2.We don’t notice b/c we have air and water inside us (blood, tissue, and cells)
Rapid Intensification of Tropical Cyclones by Organized Deep Convection Chanh Q. Kieu, and Da-Lin Zhang Department of Atmospheric and Oceanic Science University.
Aim: How do the intensity and angle of insolation relate?
Define and we have • At the sea surface (z=0), the surface current flows at 45o to the right of the wind direction Depends on constant Az => • Current.
Lesson 1 Earth’s Atmosphere Lesson 2 Energy Transfer in the Atmosphere
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS
Ben Green Group meeting, 9/13/2013
The linear sea-breeze circulation and effect of Earth’s rotation
Global Circulation and Winds (Stewart Cap. 4)
Air Masses and fronts An air mass is a large body of air that has similar temperature and moisture properties throughout. A front is defined as the transition.
Coupled atmosphere-ocean simulation on hurricane forecast
Atmospheric Circulation
Dynamics and Thermodynamics Demonstration Model (DTDM)
Read each slide, some slides have information to record on your organizer. Some slides have numbers that go with the question or red and underlined to.
Is air moving away or towards each of these pressure centers?
The Subtropical Sea Breeze
Local and Global Wind Systems
WINDS.
Weather & Climate – MTDI 1200OL Plymouth State University
Chapter 10 Wind: Global Systems.
Atmospheric Forces Wind Relationships.
Wind.
Aim: What are global winds and ocean currents?
The linear sea-breeze circulation and effect of Earth’s rotation (and Experiment #1) ATM 419/563 Spring 2019 Fovell Reference: Rotunno (1983, J. Atmos.
Aim: What are global winds and ocean currents?
Circulation in the atmosphere
Local and Global Wind Systems
World Geography 3202 Unit 2 Climate Patterns.
Aim: What are global winds and ocean currents?
Presentation transcript:

The sea-breeze circulation Part II: Effect of Earth’s rotation Reference: Rotunno (1983, J. Atmos. Sci.)

Rotunno (1983) Quasi-2D analytic linear model Heating function specified over land –Becomes cooling function after sunset –Equinox conditions Cross-shore flow u, along-shore v Two crucial frequencies –Heating  = 2  /day (period 24h) –Coriolis f = 2  sin  (inertial period 45˚N) One special latitude… where f =  (30˚N)

Heating function Rotunno’s analytic model lacks diffusion so horizontal, vertical spreading built into function

Streamfunction 

Circulation C Integrate CCW as shown Take w ~ 0; u top ~ 0 Integrate from ± infinity, from sfc to top of atmosphere

Rotunno’s analytic solution

If f >  (poleward of 30˚) equation is elliptic sea-breeze circulation spatially confined circulation in phase with heating circulation, onshore flow strongest at noon circulation amplitude decreases poleward If f <  (equatorward of 30˚) equation is hyperbolic sea-breeze circulation is extensive circulation, heating out of phase f = 0 onshore flow strongest at sunset f = 0 circulation strongest at midnight

Rotunno’s analytic solution If f =  (30˚N) equation is singular some friction or diffusion is needed circulation max at sunset onshore flow strongest at noon

Summary LatitudeOnshore maxCirculation max  > 30˚ Noon  = 30˚ NoonSunset  = 0˚ SunsetMidnight

f >  (poleward of 30˚) at noon Note onshore flow strongest at coastline (x = 0); this is day’s max coast

f <  (equatorward of 30˚)  at three times sunrise noon (reverse sign for midnight) sunset Note coastline onshore flow max at sunset

Paradox? Why is onshore max wind at sunset and circulation max at midnight/noon? –While wind speed at coast strongest at sunset/sunrise, wind integrated along surface larger at midnight/noon Max |C| noon & midnight

Effect of linear friction midnight noon sunset friction coefficient Time of circulation maximum As friction increases, tropical circulation max becomes earlier, poleward circulation max becomes later

DTDM long-term sea-breeze strategy Incorporate Rotunno’s heat source, mimicking effect of surface heating + vertical mixing Make model linear Dramatically reduce vertical diffusion Simulations start at sunrise One use: to investigate effect of latitude and/or linearity on onshore flow, timing and circulation strength

input_seabreeze.txt &rotunno_seabreeze section c=================================================================== c c The rotunno_seabreeze namelist implements a lower tropospheric c heat source following Rotunno (1983), useful for long-term c integrations of the sea-land-breeze circulation c c iseabreeze (1 = turn Rotunno heat source on; default is 0) c sb_ampl - amplitude of heat source (K/s; default = ) c sb_x0 - controls heat source shape at coastline (m; default = 1000.) c sb_z0 - controls heat source shape at coastline (m; default = 1000.) c sb_period - period of heating, in days (default = 1.0) c sb_latitude - latitude for experiment (degrees; default = 60.) c sb_linear (1 = linearize model; default = 1) c c===================================================================

input_seabreeze.txt &rotunno_seabreeze section &rotunno_seabreeze iseabreeze = 1, sb_ampl = , sb_x0 = 1000., sb_z0 = 1000., sb_period = 1.0, sb_latitude = 30., sb_linear = 1, $ sb_latitude ≠ 0 activates Coriolis sb_linear = 1 linearizes the model Other settings include: timend = sec dx = 2000 m, dz = 250 m, dt = 1 sec dkx = dkz = 5 m 2 /s (since linear)

Caution Don’t make model anelastic for now –Make sure ianelastic = 0 and ipressure = 0 –Didn’t finish the code for anelastic linear model –iseabreeze = 1 should be used alone (I.e., no thermal, surface flux, etc., activated)

Solution strategy Model starts at sunrise (6 am) Equinox presumed (sunset 6 pm) Heating max at noon, zero at sunset Cooling at night, absolute max at midnight

Heat source sb_hsrc set mproj off set lev 0 4 set lon [or set x ] d sb_hsrc

Heating function vs. time

Time series using GrADS > open seabreeze.rotunno.30deg > set t > set z 1 > set x 100 > set vrange > set xaxis > d sb_hsrc > draw xlab hour > draw ylab heating function at surface > draw title heating function vs. time

30˚N linear case (5 m 2 /s diffusion) seabreeze.gs Shaded: vertical velocity; contoured: cross-shore velocity

30˚N linear case set t set z 1 set xaxis d sum(u,x=1,x=199) Circulation Sunset Note non-zero 24h… should run several days to spin-up

30˚N linear case Onshore flow max ~ 4pm Note non-calm 24h… should run several days to spin-up sunset

Variation with latitude

Cross-shore flow and vertical motion at noon (on 1 st day) (seabreeze.gs) set t 72

Cross-shore flow and vertical motion at sunset (on 1 st day)

Cross-shore flow and vertical motion at midnight (on 1 st day)

Cross-shore near-surface wind at coastline (linear model)

Circulation vs. time Eq 30N 60N 90N sunset Circ magnitude decreases w/ latitude (expected) 30N circ max at sunset (expected) Poleward circ max later than expected (noon) Equator circ max earlier than expected (midnite) Consistent w/ existence of some friction? midnight

Recall: linear friction effect midnight noon sunset friction coefficient Time of circulation maximum As friction increases, tropical circulation max shifts earlier, poleward circulation max becomes later

Hovmoller diagrams (seabreeze_hov.gs) What is missing? x (across-coast) t (h after sunrise)

Questions to ponder Why is the onshore flow at 30N strongest in midafternoon? (Heating max was noon) Why does onshore max occur earlier at 60N? Why does onshore flow magnitude decrease poleward? Why does friction shift circulation max time? Note no offshore flow at equator at all. Why? How does linear assumption affect results?

Further exploration Run model longer… how long until statistically steady? Make model nonlinear Compare to data –Collect surface data along N-S coastline –Compare to “data” from more sophisticated model

Tips for nonlinear runs Set sb_linear = 0 Increase dkx, dkz to avoid computational instability Example with dkx = 500, dkz = 50 m 2 /s (probably excessive)

Cross-shore wind at coastline linear vs. nonlinear Why are they different?

Linear vs. nonlinear at noon

Linear vs. nonlinear at sunset