Chapter 16: Problem 4
Make a concept map of the global circulation system, using at least 10 of the following terms and others of your own choosing, with no more than 15 terms total. \(\begin{array}{lll}\text { convection cell } & \text { Hadley cell } & \text { rising air } \\ \text { Coriolis effect } & \text { hot deserts } & \text { solar radiation } \\ \text { descending air } & \text { jet stream } & \text { subtropical high } \\ \text { equatorial low } & \text { polar front } & \text { trade winds } \\ \text { Ferrel cell } & \text { precipitation } & \text { westerlies }\end{array}\)
Short Answer
Step by step solution
Understand the Key Concepts
Define Core Elements
Identify Air Movements and Forces
Connect Climate Impacts
Construct the Concept Map
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Convection Cell
These convection cells help regulate global climates and are significant drivers behind weather patterns. Understanding convection is essential because it connects diverse climate zones through its continuous movement.
In summary, convection cells can be visualized as giant loops of airflow. They encompass large areas, helping to explain the global distribution of heat and moisture.
Coriolis Effect
As the Earth rotates, different parts move at different speeds. This rotation affects how air moves in the atmosphere. In the Northern Hemisphere, the Coriolis effect deflects moving air to the right, while in the Southern Hemisphere, it deflects left.
Without the Coriolis effect, we wouldn't see the characteristic swirls of cyclones or the predictable patterns of trade winds. It helps transform straightforward airflow into complex and dynamic climate systems.
Solar Radiation
This uneven distribution causes temperature gradients, leading to air movement. Areas receiving more sunlight warm up, causing the air to rise, whereas cooler regions see descending air. This primarily drives convection cells, forming the backbone of atmospheric circulation.
Solar radiation affects weather, climates, and ocean currents, making it a cornerstone concept in understanding how our planet's climate systems operate.
Trade Winds
These winds occur as a part of the Hadley cell structure, where air rises near the equator, moves towards the poles, descends at about 30 degrees latitude, and returns towards the equator as these easterly winds.
Historically, trade winds have been critical for navigation. They are also important for ocean currents and play a role in weather, particularly in the tropics and subtropics.
Hadley Cell
Here, air rises at the equator due to intense solar heating, creating low pressure and leading to high rainfall areas. The air then travels poleward at high altitudes, cools down, and descends in the subtropics, forming high-pressure zones known as the subtropical highs.
The descending air in these zones is dry, contributing to the formation of deserts like the Sahara or the Australian Outback. The movement of air within this cell is balanced and continuous, forming a loop that is crucial for global heat distribution.
Ferrel Cell
In this zone, air movements are more complex. Descending air from the higher latitudes moves toward the poles at the surface, while rising air near 60 degrees latitude influences weather systems in the mid-latitudes.
Ferrel Cells help transfer warm equatorial air towards the poles and cold polar air towards the equator. This exchange supports temperate climates and drives westerly prevailing winds, which impact weather in regions like North America and Europe.
Polar Cell
In this cell, cold dense air descends at the poles, creating high pressure. This air then moves towards the equator at the surface, where it warms and rises around 60 degrees latitude, completing the polar convection loop.
Polar Cells play a key role in driving polar easterlies, which are winds that influence polar climate and, indirectly, global climate patterns by affecting ocean currents and energy exchanges.