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Atmospheric Circulation and Weather Systems

Learning Outcomes

  1. Understand how temperature variations cause pressure differences.
  2. Recognize the key forces influencing the movement of air: Pressure gradient, Coriolis, and Frictional forces.
  3. Identify patterns in global atmospheric circulation.
  4. Learn how air masses form and interact, leading to various weather systems.
  5. Grasp the mechanisms of tropical and extra-tropical cyclones.

Atmospheric pressure plays a crucial role in setting the air in motion. As air expands when heated and contracts when cooled, pressure differences emerge across the Earth’s surface, causing air to move from areas of high pressure to low pressure. This chapter focuses on the forces influencing atmospheric circulation, wind patterns, and the weather phenomena that result from these processes.

Atmospheric Pressure

Atmospheric pressure is the weight of a column of air from sea level to the top of the atmosphere and is measured in millibars (mb). At sea level, the average pressure is 1,013.2 mb. This pressure decreases with elevation and varies depending on the location. Instruments like mercury barometers and aneroid barometers measure atmospheric pressure. Wind is driven by variations in pressure, moving from high-pressure zones to low-pressure zones.

Vertical Variation of Pressure

Pressure in the lower atmosphere decreases rapidly with height, with an approximate drop of 1 mb for every 10 meters increase in elevation. The decrease in pressure varies, as seen in Table 9.1:

LevelPressure (mb)Temperature (°C)
Sea Level1,013.2515.2
1 km898.768.7
5 km540.48-17.3
10 km265.00-49.7

Although the vertical pressure gradient is large, the gravitational force balances it, preventing strong upward winds.

Horizontal Distribution of Pressure

Horizontal pressure variations influence wind direction and velocity. Isobars (lines connecting locations with equal pressure) on weather maps help visualize pressure systems. Low-pressure systems are enclosed by isobars with the lowest pressure at the center, while high-pressure systems have the highest pressure at the center. These systems shift with the sun’s movement, oscillating between hemispheres during different seasons.

Forces Affecting Wind Velocity and Direction

Wind is a result of differences in atmospheric pressure. The combined effects of the pressure gradient force, Coriolis force, and frictional force determine wind movement.

  1. Pressure Gradient Force: It results from the difference in atmospheric pressure. Stronger pressure gradients (closer isobars) result in faster winds.
  2. Frictional Force: Greatest near the Earth’s surface, it slows down wind, especially over land. Its influence reduces with altitude and is minimal over seas.
  3. Coriolis Force: This force, caused by Earth’s rotation, deflects wind direction: right in the northern hemisphere and left in the southern hemisphere. It is stronger at the poles and absent at the equator.

In low-pressure areas, the wind circulates counterclockwise in the northern hemisphere and clockwise in the southern hemisphere. This is reversed in high-pressure areas.

Wind Systems

Geostrophic winds occur when the pressure gradient force and the Coriolis force balance each other, causing wind to flow parallel to isobars. Table 9.2 shows wind patterns in cyclones and anticyclones:

SystemPressure ConditionNorthern Hemisphere DirectionSouthern Hemisphere Direction
CycloneLow pressureAnticlockwiseClockwise
AnticycloneHigh pressureClockwiseAnticlockwise

At the Earth’s surface, air converges over low-pressure areas and rises, while in high-pressure areas, air subsides and diverges.

Note: Coriolis force is zero at the equator, which prevents the formation of tropical cyclones near the equator.

General Circulation of the Atmosphere

Planetary wind patterns are driven by the following:

  1. Latitudinal heating variations
  2. Emergence of pressure belts
  3. Movement of belts with the sun’s path
  4. Distribution of land and oceans
  5. Earth’s rotation

The general atmospheric circulation sets in motion the ocean’s currents, which significantly impact global climates.

Major Wind Cells

Three primary wind cells determine the planet’s general circulation:

  1. Hadley Cell: Near the equator, rising warm air creates low pressure in the Inter-Tropical Convergence Zone (ITCZ), and winds from the subtropics converge here.
  2. Ferrel Cell: Between 30° and 60° latitude, cold polar air meets warm subtropical air, forming westerlies.
  3. Polar Cell: Near the poles, dense cold air sinks, creating polar easterlies.

The interaction between these cells redistributes heat and moisture, maintaining Earth’s temperature balance.

Ocean-Atmosphere Interactions

Oceans play a critical role in atmospheric circulation by influencing the transfer of energy and moisture into the air. One significant phenomenon is the El Niño, which involves the movement of warm water across the Pacific Ocean, replacing the cooler Peruvian current. This disrupts typical weather patterns, causing extreme weather events across the globe.

Important Note: ENSO (El Niño-Southern Oscillation) is a combined phenomenon involving changes in Pacific Ocean temperatures and atmospheric pressures, leading to global weather variations.

Seasonal Winds

Seasonal shifts in temperature and pressure modify wind patterns. The monsoon is the most well-known seasonal wind system, particularly in Southeast Asia. Monsoons are caused by the seasonal movement of pressure belts and maximum heating regions.

Local Winds

Local winds arise due to variations in the heating and cooling of Earth’s surfaces:

  1. Land and Sea Breezes: During the day, land heats up faster than the sea, causing wind to blow from sea to land. At night, this pattern reverses, and land breezes blow from land to sea.
  2. Mountain and Valley Winds: In mountainous regions, valley breezes blow upwards during the day, and mountain winds blow downwards at night.
  3. Katabatic Winds: These are cold winds that descend from high plateaus and ice fields into valleys, such as those found in Antarctica.

Air Masses and Fronts

When air remains over a homogeneous region for a long period, it acquires that region’s characteristics, forming air masses. These air masses are classified based on their source regions:

  1. Maritime Tropical (mT)
  2. Continental Tropical (cT)
  3. Maritime Polar (mP)
  4. Continental Polar (cP)
  5. Continental Arctic (cA)

When two air masses meet, they form a front. The interaction of warm and cold air masses at these fronts leads to weather changes, such as precipitation and storms.

Extra-Tropical Cyclones

Extra-tropical cyclones develop along the polar front, where cold polar air meets warmer air from the subtropics. These cyclones often have well-defined fronts and cause significant weather changes in mid and high latitudes. The interaction of warm fronts and cold fronts generates clouds and precipitation.

Note: Extra-tropical cyclones cover large areas and can form over both land and sea, unlike tropical cyclones, which form exclusively over oceans.

Tropical Cyclones

Tropical cyclones are violent storms that form over tropical oceans. These systems bring heavy rainfall, strong winds, and storm surges, causing widespread destruction. Conditions for tropical cyclone formation include:

  1. Sea surface temperatures above 27°C
  2. Presence of the Coriolis force
  3. Low wind shear
  4. Pre-existing low-pressure systems

Cyclones intensify through the release of energy from condensation in rising moist air. When a cyclone makes landfall, it loses strength due to the cut-off of moisture supply. Landfall is the point where the cyclone crosses the coast.

CharacteristicsTropical CyclonesExtra-Tropical Cyclones
Formation AreaTropical OceansMid and High Latitudes
SizeSmaller (600-1,200 km)Larger
Wind VelocityHigh (up to 250 km/h)Moderate
LifespanShorter (intensifies over the sea)Longer

**Important Note

**: The *eye* of the cyclone is a calm region, surrounded by spiraling winds in the eye wall, where wind speeds are the highest.

Thunderstorms and Tornadoes

Thunderstorms are caused by intense convection on hot, moist days, forming cumulonimbus clouds that produce thunder, lightning, and sometimes hail. Tornadoes, which occur mainly in mid-latitudes, are violent, spiraling winds with extremely low pressure at their center. Tornadoes over the sea are called waterspouts.


Multiple Choice Question
If the surface air pressure is 1,000 mb, the air pressure at 1 km above the surface will be:
a) 700 mb
b) 1,100 mb
c) 900 mb (Correct Answer)
d) 1,300 mb

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