Chapter 2 Flashcards

1
Q

A measure of the average kinetic energy of the molecules in a substance. Higher temperatures correspond to more energetic molecules.

A

Temperature

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2
Q

The transfer of energy from a warmer object to a cooler one. It is transferred in the atmosphere by:

A

Heat

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3
Q

The direct transfer of heat through a substance, mainly affecting the surface of the Earth.

A

Conduction

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4
Q

The transfer of heat by the movement of fluid (air or water), such as rising warm air and sinking cool air.

A

Convection

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4
Q

The transfer of energy by electromagnetic waves. All objects emit radiation depending on their temperature.

A

Radiation

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5
Q

The heat absorbed or released during a phase change (e.g., from solid to liquid or liquid to gas), without changing temperature. It plays a significant role in atmospheric processes:

A

Latent Heat

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6
Q

Water absorbs latent heat and changes from liquid to vapor, cooling the surroundings.

A

Evaporation

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7
Q

Water vapor releases latent heat and changes back to liquid, warming the surroundings.

A

Condensation

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8
Q

Energy from the sun primarily in the form of shortwave radiation (visible light and UV radiation). It heats Earth’s surface, driving weather patterns.

A

Solar Radiation

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9
Q

Why the Earth Has Seasons

A
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9
Q

Earth emits longwave radiation (infrared) back to space. This energy is what balances the incoming solar radiation.

A

Terrestrial Radiation

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9
Q

The balance between incoming solar energy and outgoing terrestrial radiation, which maintains Earth’s average temperature.

A

Radiative Equilibrium

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9
Q

Around June 21, the Northern Hemisphere is tilted towards the sun, receiving more sunlight and experiencing summer.

A

Summer Solstice

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10
Q

Gases such as water vapor, carbon dioxide (CO₂), methane (CH₄), and ozone (O₃) that absorb longwave radiation from Earth’s surface and reradiate it back, trapping heat in the atmosphere.

A

Greenhouse Gases

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10
Q

The increase in greenhouse gases, especially due to human activities like burning fossil fuels, leading to additional warming of the Earth.

A

Enhanced Greenhouse Effect

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10
Q

Around March 21 and September 21, day and night are approximately equal because neither hemisphere is tilted towards or away from the sun.

A

Equinoxes

10
Q

Around December 21, the Northern Hemisphere is tilted away from the sun, leading to winter.

A

Winter Solstice

11
Q

Factors Affecting Earth’s Seasonal Variations

A

Sun Angle
Daylight
Distance from the sun

11
Q

Clouds reflect incoming solar radiation, reducing the amount of energy that reaches Earth’s surface and contributing to cooling.

A

Clouds and Solar Radiation

12
Q

Clouds also trap outgoing longwave radiation, contributing to warming at night. This dual effect makes clouds important regulators of temperature.

A

Clouds and Terrestrial Radiation

12
Q

Caused by Earth’s axial tilt and its orbit around the sun, leading to variations in sunlight and day length

A

Seasons

13
Q

Solar radiation, including visible light and ultraviolet, that is absorbed by the Earth’s surface.

A

Shortwave Raadiation

14
Q

The percentage of incoming sunlight reflected by a surface.

A

Albedo

14
Q

Radiation emitted by the Earth, primarily in the form of infrared radiation.

A

Longwave Radiation

15
Q

The rate at which solar energy reaches the Earth, approximately 1367 watts per square meter.

A

Solar Constant