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AMS Weather Studies Introduction to Atmospheric Science, 4 th Edition. Chapter 9 Atmosphere’s Planetary Circulation. Case-in-Point. In the winter of 1997-98, the San Francisco Bay area experienced considerable flooding due to an unusually high sea level and wind-driven waves
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AMS Weather StudiesIntroduction to Atmospheric Science, 4th Edition Chapter 9 Atmosphere’s Planetary Circulation
Case-in-Point • In the winter of 1997-98, the San Francisco Bay area experienced considerable flooding due to an unusually high sea level and wind-driven waves • On one of the worst days of flooding, 3 February 1998, waters from the Bay inundated U.S. Highway 101 to a depth of up to 1.2 m (4 ft) north of the Golden Gate Bridge • Several factors control sea level in San Francisco Bay • The most important are the regular astronomical tides • Two high tides and two low tides per day • Second factor is the slow long-term trend of rising sea level due to global warming • Causes expansion of sea water and melting of land-based glaciers • El Niño is also a major factor • The 1997-98 El Niño, one of the most intense of the 20th century, winter winds blew strongly from the south along the California coast, driving surface water toward the shore and raising sea level
Driving Question • What are the principal features of the planetary-scale atmospheric circulation, and how does the circulation affect weather and climate? • This chapter describes planetary-scale: • Pressure systems • Wind belts • Circulation patterns of middle latitude westerlies • Anomalous variations in the circulation regime that result in El Niño and La Niña
Idealized Circulation Pattern • To start with, assume a non-rotating Earth • Also assume a uniform solid surface • Sun heats the equatorial regions more intensely than the poles; a temperature gradient develops • Convection cell forms when cold, dense air sinks at the poles and flows at the surface toward the equator, where it forces warm, less dense air to rise. Aloft, equatorial air flows toward the poles.
Idealized Circulation Pattern • If the idealized planet starts to rotate from west to east, the Coriolis Effect comes into play • Northern Hemisphere surface winds are diverted to the right and blow toward the southwest • Southern Hemisphere surface winds are diverted to the left and blow toward the northwest • Winds blow counter to planet’s direction of rotation
Idealized Circulation Pattern • Circulation is maintained in the atmosphere of our idealized Earth because the planetary-scale winds split into 3 belts in each hemisphere • 3 belts are: • 0° to 30° • 30° to 60° • 60° to 90° • Now some winds blow with and some blow against the planet’s rotation
Idealized Circulation Pattern • Surface winds converge along the equator and along 60° latitude circles • Convergence leads to rising air, expansional cooling, cloud development and precipitation • Convergence zones are belts of relatively low surface air pressure • Surface winds diverge at the poles and along the 30° latitude circles • Air descends, is compressed and warms, and weather is generally fair • Divergence zones are belts of relatively high surface air pressure
Features of the Planetary-Scale Circulation • Adding continents and ocean basins complicates the picture • Some pressure belts break into separate cells • Important pressure contrasts develop over land versus sea • Maps show mean sea-level air pressure during January (top) and July (bottom); these are semi-permanent features
Features of the Planetary-Scale Circulation • Schematic representation of the planetary-scale surface circulation of the atmosphere
Features of the Planetary-Scale Circulation • Pressure Systems and Wind Belts • Subtropical anticyclones • Form near 30° N and S latitude over oceans • Extend from the ocean surface to the tropopause and exert a major influence on weather and climate over vast areas of the ocean and continents • Subsiding air extends outward from the eastern sides • Compressional warming, low relative humidity, and fair skies are common • Major deserts are located on eastern flanks • The far western portions are characterized by less subsidence, less stable air, and frequent episodes of cloudy, stormy weather
Features of the Planetary-Scale Circulation • Pressure Systems and Wind Belts, cont. • Subtropical anticyclones • Common is a weak horizontal pressure gradient over a large area • Winds are weak and • Horse latitudes (30 to 35 degrees N and S) result • Surface winds poleward of the horse latitudes are the midlatitude westerlies • Winds blowing out of the high pressure cells toward the equatorial lows are called the trade winds • Trade winds from the two hemispheres converge into a broad east-west equatorial belt of light and variable winds called the doldrums. In that belt, ascending air induces cloudiness and rainfall and the most active weather develops along the intertropical convergence zone (ITCZ).
Features of the Planetary-Scale Circulation • Pressure Systems and Wind Belts, cont. • Poleward of subtropical anticyclones: • Surface westerlies flow into regions of low pressure • These are the Aleutian low and the Icelandic low in the Northern Hemisphere • In the Southern Hemisphere, this is a nearly continuous belt of low pressure surrounding Antarctica • Surface westerlies meet and override the polar easterlies along the polar front • In places where the polar front is well-defined, it is a potential site for development of extra-tropical cyclones • Polar highs are shallow, cold anticyclones that develop at high latitudes
Features of the Planetary-Scale Circulation • Winds Aloft • Aloft, winds in the middle and upper troposphere blow away from the ITCZ • These feed into the subtropical highs • Resulting convection cells are called Hadley cells
Features of the Planetary-Scale Circulation • Winds Aloft, continued • Aloft in middle latitudes, winds blow from west to east in a wavelike pattern of ridges and troughs • These winds are responsible for the movement of the synoptic-scale weather systems • Their north/south components contribute to poleward heat transport
Vertical Cross Section of Prevailing Winds in the Troposphere The altitude of the tropopause is directly related to the mean air temperature of the troposphere. The tropopause is found in three segments, occurring at highest altitudes in the tropics and lowest altitudes in the polar regions.
Features of the Planetary-Scale Circulation • Trade Wind Inversion • A persistent and climatically significant feature of the planetary-scale circulation over the eastern portions of tropical ocean basins • Key to formation is the descending branch of the Hadley cell • Descending air is warmed by compression and its relative humidity decreases • This air encounters the marine air layer overlying the ocean surface • Where SST are low, layer is cool, humid, and stable • Where SST are high, layer is warm, more humid, less stable, and well mixed by convection • The trade wind inversion is formed at the altitude where air subsiding from above meets the top of the marine layer, trapping the cool marine layer near the surface • Develops to the east and southeast of the center of a subtropical high • Acts as a cap on the vertical development of clouds and rain
Features of the Planetary-Scale Circulation • Seasonal Shifts • Pressure systems, the polar front, the planetary wind belts, and the ITCZ follow the sun, shifting toward the poles in spring and toward the equator in autumn • Planetary-scale systems in both hemispheres move north and south in tandem • Subtropical anticyclones exert higher surface pressure in summer • Icelandic low deepens in winter and weakens in summer • The Aleutian low disappears in summer • Seasonal reversals of pressure occur over the continents due to the contrast in solar heating of sea versus land • Continents at middle and high latitudes are dominated by relatively high pressure in winter and low pressure in summer • Northward migration of the ITCZ triggers summer monsoon rains in Central America, North Africa, India, and Southeast Asia
Features of the Planetary-Scale Circulation • ITCZ follows the sun • It reaches farthest north in July • It retreats to its most southerly latitudes in January
Features of the Planetary-Scale Circulation • Same latitude, different climates • In summer, San Diego is under the eastern edge of the Hawaiian subtropical high and has a distinct dry season • In summer, Charleston is on the humid, unstable side of the Bermuda high
Features of the Planetary-Scale Circulation • Ocean Surface Currents • Surface ocean currents are wind-driven • Horizontal movement of ocean surface waters to a large extent mirrors the long-term average planetary scale atmospheric circulation • Gyres, large-scale circulation regimes, appear in each of the major ocean basins and are associated with the prevailing winds that help set up the currents • Trades winds and the westerlies associated with the semi-permanent subtropical highs drive the subtropical gyres • The counterclockwise surface winds in the Aleutian and Icelandic sub-polar low pressure systems drive the sub-polar gyres
Features of the Planetary-Scale Circulation Long-term average pattern of wind-driven ocean-surface currents. Gyres in the ocean basin are driven by the planetary-scale atmospheric circulation.
Monsoon Circulation • Seasonal reversal of prevailing winds • Results in wet summers and relatively dry winters • Vigorous monsoon over portions of Africa and Asia, where rains are essential for drinking water and agriculture • Over much of India, monsoon rains account for over 80% of the annual precipitation • Depends on seasonal shifting of global circulation patterns • Also depend on seasonal contrasts in heating and cooling of water and land • Ocean has greater thermal inertia than the land
Surface wind patterns over Asia during • Wet (summer) monsoon • Dry (winter) monson
Monsoon Circulation • In spring, there is relatively cool air over the ocean and relatively warm air over land • Horizontal pressure gradient is directed from sea to land • Produces an onshore flow of humid air • Over land, intense solar heating generates convection • Expansional cooling causes condensation, clouds, and rain • Release of latent heat increases buoyancy and contributes to uplift and instability, triggering even more cloud development and rainfall • Aloft, the air spreads seaward and subsides over the relatively cool ocean surface
Monsoon Circulation • In Autumn, radiational cooling chills the land more than the adjacent ocean surface • Horizontal pressure gradient is directed from land to sea • Produces an offshore flow of air • Over land, air subsides, and dry surface winds sweep seaward • Air rises over the relatively warm ocean surface, completing the monsoon circulation
Topography complicates the monsoon circulation and the geographical distribution of rainfall Monsoon rainfall is neither uniform nor continual Rainy season consists of active and dormant phases The planetary circulation (e.g., ITCZ shifts) and the strength and distribution of convective activity vary from one year to the next Variation affects the intensity and duration of monsoon rains The southwest monsoon affects the American Southwest and brings a dramatic increase in rainfall during July and August Monsoon Circulation
Waves in the Westerlies • Between 2 and 5 waves generally encircle the hemisphere at any one time • These long waves are called Rossby waves, and characterize the westerlies above the 500-mb level • They are measured by: • Wavelength • Distance between successive troughs or ridges • Amplitude • North-south extent • Number of waves • In winter, waves strengthen • Fewer waves • Longer wavelength • Greater amplitude • Seasonal changes stem from variations in the north-south air pressure gradient, which is steeper in winter because of the greater temperature gradient
Waves in the Westerlies • Zonal and Meridional Flow Patterns • Westerlies have 2 components: • North-south airflow is the meridional component • West-to-east airflow is the zonal component • If north-south component is weak, the result is a zonal flow pattern • North-south exchange of air masses is minimal • If flow is in a pattern of deep troughs and sharp ridges, the result is a meridional flow pattern • Greater temperature contrasts develop across the U.S. and southern Canada • Stage is set for development of extra-tropical cyclones • If northern westerlies have a wave configuration differing from the southern westerlies, a complicated split flow pattern may exist
Waves in the Westerlies • Zonal and Meridional Flow • These two images illustrate extremes of zonal and meridional flow • Westerlies generally shift back and forth between zonal and meridional flow • There is no regularity to this shift • The affects long-range weather forecasting accuracy
Waves in the Westerlies • Blocking Systems and Weather Extremes • North American weather is more dramatic when the westerlies are strongly meridional • Undulations may become so dramatic that masses of air separate from the flow • Cutoff highs and lows result • These prevent normal west-to-east circulation, and are called blocking systems • Extremes in weather such as drought or flooding rains or excessive heat or cold can result
Waves in the Westerlies • Blocking Systems and Weather Extremes, cont. • (A) Prevailing circulation pattern in the mid to upper troposphere during the summer of 1988. The blocking warm anticyclone over the central U.S. contributed to severe drought • (B) The long-term average circulation pattern
Waves in the Westerlies • Blocking Systems and Weather Extremes, cont. • The map illustrates principal features of the prevailing atmospheric circulation pattern during the summer of 1993 • A blocking circulation pattern was responsible for record flooding in the Midwest and drought over the Southeast
Waves in the Westerlies • Blocking Systems and Weather Extremes, cont. • The top map illustrates the total rainfall for the period June-August 1993, expressed as a percentage of the long-term average • The bottom picture shows a sign marking the crest of floodwaters at Missouri City, MO • Heavy rains falling on the drainage basins of the Missouri and Upper Mississippi River valleys saturated soils and triggered excessive runoff, all-time record river crests, and severe flooding. Property damage totaled about $26.7 billion (2002 dollars).
Waves in the Westerlies • Short Waves • Ripples superimposed on Rossby long waves • Propogate rapidly through the Rossby waves • 12 or more waves are generally found in a hemisphere at any one time • Westerlies accelerate in ridges and slow in troughs, inducing horizontal speed convergence aloft ahead of ridges and horizontal speed divergence aloft ahead of troughs
Waves in the Westerlies • Short Waves, cont. • The figure is a schematic representation of the relationship between waves in the westerlies and a surface high and low
Jet Streams • Narrow corridors of very strong wind • In middle latitudes, the most prominent jet stream (polar front jet stream) is located above the polar front in the upper troposphere between the midlatitude tropopause and the polar tropopause • Follows the path of the planetary westerly waves • Winds may top 160 km per hr (100 mph) • Eastbound aircraft seek it as a tail wind
Jet Streams • The polar front is a narrow transition zone between relatively cold and warm air masses • Cold air is denser than warm air, so pressure drops more rapidly in a column of cold air than warm air • Even if air pressure is the same at the surface, there is a horizontal pressure gradient aloft (directed from warm to cold air) that increases with increasing altitude
Jet Streams • Coriolis Effect balances the horizontal pressure gradient force • Winds blow parallel to the polar front with cold air to the left of the direction of motion in the Northern Hemisphere • Due to a strengthening horizontal pressure gradient with increasing altitude, wind speed increases with altitude in the troposphere and is highest near the tropopause • Where the polar front is well defined, jet stream winds are stronger and jet streaks may develop • Strongest jet streaks develop in winter along the east coasts of North America and Asia • Great temperature contrast between snow-covered land and ice-free sea surface • Jet streaks may have wind speeds as high as 350 km per hr (217 mph)
Jet Streams • The figure below is a map view of a jet streak with associated regions of horizontal divergence and convergence aloft. The contour lines are isotachs, lines of equal wind speed (in km per hr). In a straight jet streak, the strongest horizontal divergence is in the left-front quadrant, supplying upper-air support for extra-tropical cyclone development.
Jet Streams • Undergoes important seasonal shifts • Strengthens in winter and weakens in summer • Map shows long-term average seasonal locations • When polar front jet stream is south of your location, weather is relatively cold. When it is north, the weather is relatively warm
Jet Streams • Subtropical Jet stream • Found on the poleward side of Hadley cells near the break in the tropopause between tropical and middle latitudes • Strongest in winter • Less variable with latitude than the polar front jet stream • Other jet streams • Tropical easterly jet • Feature of the summer circulation at about 15 degrees N over North Africa and south of India and Southeast Asia • Low-level jet stream • Several hundred meters above Earth’s surface • Surges up Mississippi River valley • Contributes to the development of nocturnal thunderstorms
El Niño, La Niña, and the Southern Oscillation • In El Niño, • Trade winds weaken • SST rise well above long-term averages over the central and eastern tropical Pacific • Areas of heavy rainfall shift from the western into the central tropical Pacific • La Niña is a period of exceptionally strong trade winds across the tropical Pacific with lower than usual SST in the central and eastern tropical Pacific • El Niño is the warm phase and La Niña is the cold phase of the tropical atmosphere/ocean interaction • El Niño and La Niña influence the prevailing circulation of the atmosphere in middle latitudes, especially in winter • Weather extremes that may accompany El Niño are opposite those associated with La Niña
El Niño, La Niña, and the Southern Oscillation • Historical Perspective • Originally was the name given by fisherman to the seasonal occurrence of an unusually warm southward flowing ocean current and poor fishing off the coast of Peru and Ecuador during the Christmas season • Warm weather episodes are relatively brief (1-2 months) and then SST and fisheries return to normal levels • Now, scientists reserve the term El Niño for long-lasting atmosphere/ocean anomalies • Occurs every 3-7 years • Persists for 12-18 months or longer • Accompanied by significant Pacific SST changes, major changes in atmosphere and ocean circulation patterns, and collapse of important South American fisheries
El Niño, La Niña, and the Southern Oscillation • Historical Perspective • An important step in understanding El Niño was the discovery of the southern oscillation in 1924 by Sir Gilbert Walker • Seesaw variation in air pressure across the tropical Indian and Pacific Oceans • Influences monsoon rains in India • In 1966, Jacob Bjerknes demonstrated a relationship between El Niño and the southern oscillation (ENSO) • An El Niño episode begins when the air pressure gradient across the tropical Pacific begins to weaken, heralding the slackening of the trade winds • Intense El Niño of 1982-83 brought attention to weather impacts worldwide
Historical Perspective Today, the southern oscillation index is computed by subtracting the Darwin pressure from the Tahiti pressure divided by the standard deviation of that quantity Strong positive values indicate La Niña conditions Strong negative values indicate El Niño conditions El Niño, La Niña, and the Southern Oscillation
El Niño, La Niña, and the Southern Oscillation • Neutral Conditions in the Tropical Pacific • If Earth did not rotate, frictional coupling between the wind and the ocean surface would push a thin layer of water in the same direction of the wind, and the surface layer would drag the layer beneath it • Because Earth rotates, the shallow layer of surface water set in motion by the wind is deflected to the right of the wind direction in the Northern Hemisphere and to the left in the Southern Hemisphere • Except at the equator, each layer of water put into motion by the layer above shifts direction because of the Coriolis Effect • The model to plot the direction and speed of water layers is known as the Ekman spiral • The net water movement of 90° to the wind direction due to the coupling between wind and surface water is known as Ekman transport
Ekman Spiral and Ekman Transport In the Northern Hemisphere, the surface layer of water moves at 45 degrees to the right of the wind direction. The net transport of water through the wind driven column is 90 degrees to the right of the wind.
Typically, southerly or southwesterly winds blowing along the west coast of South America drive warm surface waters to the left (westward) via Ekman transport, away from the coast In the process known as upwelling, cold-nutrient-rich waters move upward from depths of 200 to 1000 m (650 to 3300 ft) Abundance of nutrients brought to sunlit surface waters spurs an explosive growth of phytoplankton, which supports a highly productive fishery El Niño, La Niña, and the Southern Oscillation
Average rainfall per day across the tropical Pacific from 1998-2007
El Niño and La Niña • Neutral Conditions in the Tropical Pacific, cont. • Walker Circulation (large convective-type circulation) • High SST in the western tropical Pacific lowers surface air pressure and low SST in the eastern tropical Pacific raises air pressure • During neutral conditions, the east-west SST gradient reinforces the trade winds by strengthening the east-west pressure gradient • Trades become warmer and more humid as they flow over the ocean surface • In the western tropical Pacific warm humid air rises, expands, and cools, leading to thunderstorm formation • Aloft, air flows eastward and sinks over the cooler water of the eastern tropical Pacific