EV1005 LECTURE 3 & 4

Atmospheric Pressure and Basic Concepts

  • Atmospheric pressure is the weight of air above a unit area; it decreases with height because density falls off with altitude.
  • Air near the ground is heated → warm air rises, expands, density decreases, and low pressure forms at the surface.
  • As air rises, it cools; cooler air holds less moisture, so condensation and rain can result from rising air; descending air is typically dry and associated with high pressure.
  • Record pressures mentioned:
    • Canadian record low: 940.2 mb (94.02 kPa) at Saint Anthony, NL, Jan 1977.
    • U.S. record low: 882 mb (26.02 in.) Hurricane Wilma, Oct 2005.
    • Earth’s record low: 870 mb (25.69 in.) Typhoon Tip, Oct 1979.
    • Strong high pressures: Canadian record high 1079.6 mb (107.96 kPa) at Dawson, NWT, Feb 1989; Earth’s record high 1084 mb (32.01 in.) Agata, Siberia, Dec 1968.
  • Normal sea-level pressure: ~1013.2 mb (29.92 inHg).
  • Unit conversions:
    • 1.0 inHg = 33.87 mb; 1.0 mb = 0.0295 inHg; 1.0 mb = 0.75 mm Hg; 1 lb/in² = 68.95 mb (approximate conversions vary with exact reference).
  • Fraction of atmospheric mass in the troposphere: about 90% of the mass is within the troposphere.
  • Density and pressure profiles with altitude:
    • Density is higher near the Earth’s surface and decreases with altitude (see density–altitude profile).
    • Temperature and density profiles vary through the atmospheric layers (troposphere, stratosphere, mesosphere, thermosphere, exosphere).

Atmospheric Circulation: Horizontal and Vertical Motion

  • Air moves from regions of high pressure to low pressure; wind strength is determined by the pressure gradient (spacing of isobars):
    • Wide spacing = weak gradient = light winds.
    • Close spacing = steep gradient = strong winds.
  • Isobars are lines of equal pressure; wind generally follows a path roughly parallel to isobars (geostrophic tendency) with a cross-isobar component due to friction.
  • High pressure systems (anticyclones) in the Southern Hemisphere rotate anticlockwise; low pressure systems (cyclones) rotate clockwise.
  • Low pressure systems are associated with uplift, stronger winds, and precipitation; high pressure systems are associated with sinking air and clearer skies.
  • Vertical motion:
    • High pressure: sinking air, dispersing or compressing, leading to clearer conditions.
    • Low pressure: rising air, leading to condensation, clouds, and precipitation.

Coriolis Force and Global Deflection

  • Coriolis force acts on moving air, deflecting its path:
    • Southern Hemisphere: apparent deflection to the left of the motion.
    • Northern Hemisphere: apparent deflection to the right of the motion.
  • Relative magnitudes (illustrative values):
    • Equator: v ≈ 1675 km/h (≈ 465 m/s)
    • 60° latitude: ≈ 838–770 km/h (≈ 232–214 m/s)
    • Poles: deflection tends toward very small circles (negligible relative to equator).
  • Consequences:
    • Air originating at the equator moves poleward into faster-moving atmosphere, causing it to have a west-to-east (westerly) relative motion as it moves poleward.
    • Combined with pressure gradients, this produces prevailing wind patterns and cyclonic/anticyclonic circulations.
  • Important concept: Coriolis causes turning of geostrophic flow and interacts with pressure gradients and surface friction to produce three-dimensional wind fields.

Geostrophic Winds and Upper-Level Flow

  • Geostrophic winds flow approximately parallel to isobars in the upper atmosphere where friction is small.
  • Across-isobar flow is small and results from a balance among pressure gradient force, Coriolis force, and friction (more cross-isobar flow near the surface).
  • In the upper troposphere, winds tend to be faster where isobars are closer together (stronger pressure gradient).
  • World-wide patterns:
    • Trade winds near the equator.
    • Westerlies in mid-latitudes.
    • Subtropical highs and mid-latitude westerlies associated with jet streams.

Synoptic Features: Fronts, Ridges, Troughs, and Pressure Systems

  • Synoptic charts depict MSLP (mean sea level pressure) with isobars and fronts.
  • Ridge: elongated high-pressure region with isobars curving outward; generally associated with clear weather.
  • Trough: elongated low-pressure region with a surge of lower pressure; associated with unsettled weather.
  • Fronts:
    • Cold front: boundary where cold air advances into warmer air; often sharp wind shift and steep ascent, with colder air behind the front.
    • Warm front: boundary where warm air overrides cooler air; ascent is more gradual, widespread, long-lasting rainfall.
    • Stationary front: boundary between air masses that is not moving significantly.
    • Occluded front: when a cold front overtake a warm front; can produce complex weather patterns.
  • Clouds commonly associated with fronts:
    • Nimbostratus, Cirrus, Altostratus, Cirrostratus, etc.
  • Fronts in Australia often show wind shifts around NW ahead of the front to SW behind it.
  • “Geostrophic winds” in synoptic context: winds flow along isobars with some cross-isobar flow caused by friction; strongest winds where isobars are closest.

Air Masses, Uplift, and Precipitation

  • When air masses collide, they do not mix readily; fronts form (air mass boundaries).
  • Uplift mechanisms:
    • Convergent lifting (airflows collide and forced upward).
    • Convectional lifting (buoyancy over warm surfaces).
    • Orographic lifting (air moves over mountains; rain on windward side, rain shadow on leeward side).
    • Front uplifting due to conflicting air masses.
  • Condensation and cloud formation occur when rising air cools and moisture condenses; latent heat release influences cloud development and precipitation intensity.

Adiabatic Processes, Lapse Rates, and Moisture

  • Adiabatic processes describe cooling/heating of air as it rises or descends without exchanging heat with surrounding air.
  • Dry adiabatic lapse rate (unsaturated air): extΓextdry=10C/1000mext{Γ}_{ ext{dry}} \,=\, 10\,^{\circ}\mathrm{C}/1000\mathrm{m}
  • Moist adiabatic lapse rate (saturated air): approximately Γextmoist5C/1000m\Gamma_{ ext{moist}} \approx 5\,^{\circ}\mathrm{C}/1000\mathrm{m}
  • Dew point lapse rate: roughly ΔTdew1.8C/1000m\Delta T_{\text{dew}} \approx 1.8\,^{\circ}\mathrm{C}/1000\mathrm{m}
  • Phase changes and latent heat:
    • Evaporation/vaporization requires energy; latent heat of vaporization: L_v \approx 540\ \text{cal g^{-1}}
    • Condensation releases latent heat: ΔQ=Lv\Delta Q = -L_v per gram condensed
    • Fusion and melting involve latent heats as well: latent heat of fusion ~ +80\ \text{cal g^{-1}} (absorbed) and freezing/solidification release ~ -80\ \text{cal g^{-1}}
  • During uplift, air cools adiabatically; if it cools to its dew point, condensation occurs and latent heat release slows further cooling (wet adiabatic cooling).
  • Through height, temperature and humidity profiles determine cloud types and precipitation potential.

Water, Humidity, and Clouds

  • Water states and energy:
    • Sublimation: solid to gas (absorbs energy).
    • Deposition: gas to solid (releases energy).
    • Evaporation (vaporization): liquid to gas (absorbs energy).
    • Condensation: gas to liquid (releases energy).
    • Freezing: liquid to solid (releases energy).
    • Melting: solid to liquid (absorbs energy).
  • Latent heat values (per gram):
    • Vaporization: L_v \approx 540\ \text{cal g^{-1}} (absorbed)
    • Condensation: -L_v \approx -540\ \text{cal g^{-1}} (released)
    • Melting: L_f \approx +80\ \text{cal g^{-1}} (absorbed)
    • Freezing: -L_f \approx -80\ \text{cal g^{-1}} (released)
  • Water-holding capacity of air:
    • At 30°C, air can hold about 27.5\ \text{g kg^{-1}} of water vapor at saturation.
    • At 10°C, about 7.5\ \text{g kg^{-1}} at saturation.
  • Humidity concepts:
    • Relative Humidity (RH) is the ratio of actual water vapor to the maximum water vapor the air can hold at that temperature.
    • Dew point is the temperature at which air becomes saturated and condensation begins.
    • Condensation leads to cloud formation; dew point decreases with rising altitude if moisture is unchanged.
  • Cloud formation and types (illustrative):
    • Cirrus, Cirrostratus, Cirrocumulus (high clouds).
    • Altostratus, Altocumulus (middle clouds).
    • Stratus, Stratocumulus (low clouds).
    • Cumulus, Cumulonimbus (vertical development; anvil-headed for cumulonimbus).
  • Uplift and cloud development: advantageous vertical growth leads to cumulonimbus and heavy rainfall; stable layers suppress cloud growth.

Clouds and Precipitation: Condensation Processes

  • Condensation occurs when air rises and cools to its dew point; latent heat release can promote further uplift.
  • Cloud types indicate the vertical development and moisture content; Cumulonimbus represents strong uplift and potential storms.
  • The presence of condensing moisture and lifting mechanisms determine precipitation patterns across regions.

Regional Weather Drivers in Australia

  • Monsoon and Madden–Julian Oscillation (MJO) influence rainfall and cyclone activity, especially in northern Australia.
  • Indian Ocean Dipole (IOD) and El Niño/Southern Oscillation (ENSO) shape seasonal patterns.
  • Australian climate features:
    • Monsoon trough and ITCZ location shift seasonally; NW winds in summer vs SE trades in winter.
    • Frontal systems and troughs contribute to mid-latitude weather in southern Australia.
    • Blocking highs can stall movement of weather systems, influencing droughts and heat waves.
  • Tropical cyclones and depressions contribute to extreme rainfall and wind events in northern regions.
  • West Coast dynamics include troughs and upper-level troughs; sea breezes and monsoonal influences play a role in coastal climates.
  • Notable weather drivers listed: Monsoon, Tropical Cyclones, Madden–Julian Oscillation, Indian Ocean Dipole, Tropical Depressions, West Coast troughs, Trade Winds, Northwesterly Cloudbands, Easterly Trough, Subtropical Ridge (winter and summer), Frontal Systems, Cut-off Lows, Blocking Highs, Southern Annular Mode.

ITCZ, Hadley Circulation, and Global Wind Patterns

  • ITCZ (Intertropical Convergence Zone) location shifts seasonally; the convergence of moist air at the equator results in heavy clouds and rainfall.
  • Hadley circulation: rising moist air around the equator, moving poleward aloft, sinking in the subtropics, and returning near the surface as trade winds.
  • Tropical to mid-latitude transitions produce the Hadley-Cell–Ferrel-Polar cell pattern; vertical motion and fronts accompany these cells.
  • Tropical regions exhibit heavy rainfall due to convection and ITCZ activity; subtropics have descending dry air creating high pressure zones.
  • Seasonal ITCZ shifts and associated rainfall patterns influence the Australian climate, particularly the northern monsoon region.

Monsoon System in Australia and Nearby Regions

  • Monsoon: characterized by a seasonal reversal of winds due to differential heating of land and sea; offshore winds in winter and onshore winds in summer.
  • ITCZ follows the sun’s position and the seasonal migration of heating; two major heat lows (Pilbara and Cloncurry) can attract the ITCZ.
  • Summer monsoon features NW winds; winter features SE trades.
  • MJO influence on cyclone activity in Australia: eastward-moving convective pulse that interacts with the monsoon trough; stronger influence to the north of the country.
  • ENSO (El Niño / La Niña) modulates monsoon intensity and rainfall variability.

Severe Weather and Practical Implications in Australia

  • Economic and ecological impacts from heat waves, bushfires, and monsoonal rains.
  • Anticipated weather indicators include NW winds in dry seasons and SE winds in monsoon-active periods.
  • Frontal systems, tropical cyclones, and monsoon troughs contribute to extreme weather events; blocking highs can lead to prolonged weather patterns.
  • Understanding atmospheric processes helps predict rainfall distribution, drought risk, and temperature extremes.

Atmospheric Stability and Cooling/Heating Processes

  • Atmospheric stability affects cloud formation and precipitation patterns; adiabatic processes govern temperature changes with altitude.
  • Adiabatic temperature change with altitude:
    • Dry adiabatic lapse rate: Γdry=10°C/1000m\Gamma_{dry} = 10\,\degree\mathrm{C}/1000\mathrm{m}
    • Wet (moist) adiabatic lapse rate: approximately Γmoist5°C/1000m\Gamma_{moist} \approx 5\,\degree\mathrm{C}/1000\mathrm{m} due to latent heat release slowing cooling.
  • Dew point lapse rate: ΔTdew1.8°C/1000m\Delta T_{dew} \approx 1.8\,\degree\mathrm{C}/1000\mathrm{m}
  • When a parcel of air rises from sea level at 32°C to 1000 m, its temperature changes according to the appropriate lapse rate, affecting condensation potential and humidity.
  • Relative humidity interacts with temperature to determine condensation likelihood; RH can exceed 100% if temperature falls while moisture content remains.

Atmospheric Layers, Profiles, and Measurements

  • Temperature and pressure profiles across the atmosphere show:
    • Troposphere contains ~90% of atmospheric mass.
    • Temperature generally decreases with height in the troposphere; a lapse rate describes this gradient.
    • Stratosphere contains the ozone layer; temperature increases with height in parts of the stratosphere due to ozone absorption of UV radiation.
  • Pressure at sea level is defined as 1013.2 mb (29.92 inHg); variations include deep lows and strong highs.
  • Pressure scales and conversions:
    • 1 mb ≈ 0.0295 inHg; 1013.2 mb corresponds to 29.92 inHg.
    • Severe hurricane/low-pressure events: pressures can dip well below 1000 mb; high-pressure records rise above 1050–1080 mb.
  • Typical cross-sectional views show the relationship between pressure cells, circulation, and tropopause heights (ITCZ and polar front interactions).

Synoptic Charts and Chart Reading

  • Early synoptic charts illustrate pressure systems, fronts, troughs, ridges, and monsoon features; modern charts continue to show MSLP, fronts, troughs, monsoon troughs, fronts, and jet streams.
  • Synoptic interpretation involves:
    • Identifying high and low pressure centers (H and L).
    • Reading isobar spacing to infer wind strength.
    • Recognizing fronts (warm, cold, stationary, occluded) and associated cloud types.
    • Noting troughs and ridges and their movements to predict weather changes.
  • Example: a geostrophic wind diagram demonstrates air flowing around a low pressure center with isobars wrapping clockwise in the Southern Hemisphere (anticyclonic) and anticlockwise around highs.

Key Pointers for Exam Preparation

  • Understand the cause-and-effect chain: differential heating → pressure differences → wind (pressure gradient) → Coriolis deflection → geostrophic balance in upper levels → fronts, troughs, ridges → uplift and precipitation.
  • Be able to explain why ascending air cools and leads to cloud formation and rain, and why descending air leads to dry, stable conditions.
  • Distinguish between dry and moist adiabatic lapse rates and explain how latent heat release modifies vertical temperature profiles.
  • Recognize the main global wind systems and their relation to pressure belts: trade winds, westerlies, polar easterlies, Hadley, Ferrel, and Polar cells.
  • Understand the ITCZ and its seasonal migration and how that affects monsoon systems and rainfall in Australia.
  • Be able to describe how topography (orography) and surface friction modify wind patterns and rainfall distribution (e.g., rain shadows, sea breezes).
  • Recall representative numerical values for quick reference: normal sea-level pressure, record pressures, lapse rates, latent heats, and Coriolis speed estimates.
  • Connect synoptic cues (isobars, fronts, troughs, ridges) to weather outcomes (wind direction/strength, precipitation, temperature changes).
  • Relate atmospheric processes to real-world phenomena in Australia (heat waves, Antarctic outbreaks, monsoon effects in Townsville, and regional rainfall patterns).

Quick Equations and Critical Numbers (LaTeX)

  • Pressure gradient and wind relationship (conceptual):
    • Wind speed V is proportional to the pressure gradient magnitude |∇P| and modulated by Coriolis and friction forces. In the upper atmosphere (minimal friction): VP,V \propto |\nabla P|, with wind directed along isobars in a geostrophic balance.
  • Dry adiabatic lapse rate: Γdry=10°C/1000m.\Gamma_{dry} = 10\,\degree\mathrm{C}/1000\mathrm{m}.
  • Moist adiabatic lapse rate (approximate): Γmoist5°C/1000m.\Gamma_{moist} \approx 5\,\degree\mathrm{C}/1000\mathrm{m}.
  • Dew point lapse rate: ΔTdew1.8°C/1000m.\Delta T_{dew} \approx 1.8\,\degree\mathrm{C}/1000\mathrm{m}.
  • Latent heat values (per gram):
    • Vaporization: Lv540 cal g1L_v \approx 540\ \text{cal g}^{-1}
    • Condensation: Lv540 cal g1-L_v \approx -540\ \text{cal g}^{-1}
    • Fusion: Lf80 cal g1L_f \approx 80\ \text{cal g}^{-1}
    • Freezing: Lf80 cal g1-L_f \approx -80\ \text{cal g}^{-1}
  • Normal sea-level pressure: pSL1013.2 mb=29.92 inHg.p_{SL} \approx 1013.2\ \text{mb} = 29.92\ \text{inHg}.
  • Record low/high pressures (examples):
    • 940.2 mb (Canada, 1977); 882 mb (U.S., 2005); 870 mb (Earth, 1979).
    • 1079.6 mb (Canada, 1989); 1084 mb (Earth, 1968).
  • Magnetic and rotational considerations (Coriolis) (illustrative):
    • Equatorial linear speed: veq1675 km/h(465 m/s).v_{eq} \approx 1675\ \text{km/h} (\approx 465\ \text{m/s}).
    • At 60°N latitude: v60838 km/h(232 m/s).v_{60} \approx 838\ \text{km/h} (\approx 232\ \text{m/s}).

Remember to Review

  • How pressure systems and airmass boundaries influence weather patterns.
  • The roles of fronts, uplift processes, and topography in rainfall distribution.
  • The interplay between energy budgets, wind, and currents in shaping climate patterns.
  • australia-specific weather drivers including monsoon, MJO, ENSO, IOD, blocking highs, and regional fronts.
  • how to read synoptic charts and interpret MSLP, isobars, fronts, troughs, and ridges for practical forecasting.