Diurnal Energy Budget and Urban Climates

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Flashcards covering key vocabulary related to diurnal energy budgets, global circulation patterns, and urban climates.

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29 Terms

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<p>Diurnal Energy Budget</p>

Diurnal Energy Budget

Balance between incoming solar radiation and outgoing terrestrial radiation during a 24-hour period.

<p>Balance between incoming solar radiation and outgoing terrestrial radiation during a 24-hour period.</p>
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<p>Incoming Solar Radiation (Insolation)</p>

Incoming Solar Radiation (Insolation)

Energy received from the Sun that warms the Earth's surface during the day.

<p>Energy received from the Sun that warms the Earth's surface during the day.</p>
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<p>Outgoing Radiation</p>

Outgoing Radiation

Heat lost by the Earth to the atmosphere and space at night, mostly as infrared radiation.

<p>Heat lost by the Earth to the atmosphere and space at night, mostly as infrared radiation.</p>
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<p>Albedo</p>

Albedo

Reflectivity of a surface; measures how much sunlight is reflected rather than absorbed.

<p>Reflectivity of a surface; measures how much sunlight is reflected rather than absorbed.</p>
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<p>High Albedo Surfaces</p>

High Albedo Surfaces

Light-colored surfaces that reflect most sunlight, resulting in lower temperatures (e.g., ice and snow).

<p>Light-colored surfaces that reflect most sunlight, resulting in lower temperatures (e.g., ice and snow).</p>
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<p>Low Albedo Surfaces</p>

Low Albedo Surfaces

Dark-colored surfaces that absorb more sunlight, warming the surface (e.g., forests or oceans).

<p>Dark-colored surfaces that absorb more sunlight, warming the surface (e.g., forests or oceans).</p>
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Excess Radiation

The Sun's energy is most intense at the equator due to direct overhead sunlight, creating warm temperatures.

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Deficit Radiation

Sunlight is spread over a larger area near the poles and is less intense, leading to colder temperatures.

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<p>Atmospheric Circulation</p>

Atmospheric Circulation

Warm air rises at the equator and moves toward the poles, while cooler air from the poles moves toward the equator, creating global wind patterns.

<p>Warm air rises at the equator and moves toward the poles, while cooler air from the poles moves toward the equator, creating global wind patterns.</p>
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<p>Ocean Currents</p>

Ocean Currents

Transfer heat by moving warm water from the equator towards the poles, and cold water moves from the poles toward the equator.

<p>Transfer heat by moving warm water from the equator towards the poles, and cold water moves from the poles toward the equator.</p>
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<p>Air Pressure</p>

Air Pressure

Weight of the atmosphere pressing down on Earth's surface.

<p>Weight of the atmosphere pressing down on Earth's surface.</p>
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High Pressure Areas

Regions where air is sinking, creating clear skies and calm weather.

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Low Pressure Areas

Regions where air is rising, leading to cloud formation and stormy weather.

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<p>Equatorial Low Pressure Belt</p>

Equatorial Low Pressure Belt

Low pressure at the equator caused by rising warm air; also known as the Intertropical Convergence Zone (ITCZ).

<p>Low pressure at the equator caused by rising warm air; also known as the Intertropical Convergence Zone (ITCZ).</p>
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<p>Subtropical High Pressure Belt</p>

Subtropical High Pressure Belt

High pressure areas around 30° north and south of the equator where air that rose at the equator cools and sinks.

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<p>Subpolar Low Pressure Belt</p>

Subpolar Low Pressure Belt

Low pressure areas at about 60° latitude where warm air from the subtropics meets cold air from the poles.

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<p>Polar High Pressure</p>

Polar High Pressure

High pressure at the poles caused by sinking cold air.

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<p>Trade Winds</p>

Trade Winds

Winds that blow from the subtropical high-pressure areas towards the equator, deflected by the Coriolis effect.

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<p>Westerlies</p>

Westerlies

Winds in the middle latitudes (30°–60°) that blow from the west towards the east, driven by pressure differences.

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<p>Polar Easterlies</p>

Polar Easterlies

Winds near the poles that blow from the east to the west.

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<p>Pressure Gradients</p>

Pressure Gradients

Air moves from areas of high pressure to low pressure; the stronger the difference, the stronger the wind.

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<p>Coriolis Effect</p>

Coriolis Effect

Due to Earth's rotation, moving air is deflected to the right in the Northern Hemisphere and to the left in the Southern Hemisphere.

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<p>General Circulation Model (GCM)</p>

General Circulation Model (GCM)

Simplified model that explains the movement of air around the globe based on temperature, pressure, and wind patterns.

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<p>Hadley Cell</p>

Hadley Cell

Warm air at the equator rises and moves toward the poles, sinking around 30° latitude, creating the trade winds and subtropical high-pressure areas.

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<p>Ferrel Cell</p>

Ferrel Cell

In the middle latitudes (30°–60°), air is forced to rise at low-pressure areas and sinks at high-pressure areas; area where the westerlies occur.

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<p>Polar Cell</p>

Polar Cell

Cold air sinks at the poles and moves toward the equator, creating the polar easterlies.

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<p>Urban Climates</p>

Urban Climates

Climatic characteristics that are different in urban areas compared to surrounding rural areas, influenced by human activities.

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Urban Heat Island (UHI)

Increase in temperature in urban areas compared to surrounding rural areas, caused by human activities such as dense buildings and concrete surfaces.

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Canyon Effect

Tall buildings block wind and create areas of low air movement, preventing heat and pollutants from being dispersed.