GEOG110 Midterm 1 - Matthew Winnick

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/116

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 2:00 AM on 3/10/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

117 Terms

1
New cards

Steady-state (Equilibrium)

A system or variable that does not change through time. Requires a steady flow of input and output energy.

2
New cards

Positive Feedback Loop

When the output of a stimulus amplifies the initial stimulus.

3
New cards

Negative Feedback Loop

When the output of a stimulus opposes the initial stimulus.

4
New cards

Transient State

When equilibrium/steady-state is temporarily broken.

5
New cards

Electromagnetic Radiation

A type of energy that travels through space as waves.

6
New cards

Visible EM Radiation

The only part of the electromagnetic spectrum that our eyes can detect. The shortest wavelengths.(Think rainbow colors)

7
New cards

Infrared EM Radiation

Wavelengths longer than visible light, so we can't see it, but we can feel it. (Think warmth- when you can feel the heat from the sun)

8
New cards

Ultraviolet EM Radiation

Shorter wavelengths than visible light = holds the most energy (Think getting a sunburn)

9
New cards

Blackbody Radiation

Objects emit electromagnetic waves whose characteristics depend on the object's temperature (Sun and Earth behave like blackbodies)

10
New cards

Planck's Law

Describes how hot objects emit electromagnetic radiation across different wavelengths based on their temperature

11
New cards

Do hot or cold objects give off more energy (shorter wavelengths)?

Hot

12
New cards

What happens when the Earth emits less energy than it absorbs?

It warms up

13
New cards

What happens when the Earth emits more energy than it absorbs?

It cools down

14
New cards

Albedo

The fraction of light reflected by an object

15
New cards

Do oceans or land have higher albedo?

Land, especially ice.

16
New cards

Why is Earth's albedo decreasing?

Glaciers are melting and turning into ocean water, which has a lower albedo overall.

17
New cards

Radiative Balance

Earth's temperature stays stable when the energy coming in from the sun equals the energy leaving the Earth back to space.

18
New cards

What happens if incoming energy > outgoing energy?

The planet warms.

19
New cards

What happens if incoming energy< outgoing energy?

The planet cools.

20
New cards

Stefan-Boltzmann Constant

A number that tells us how much energy an object radiates as heat based on it's temperature.

21
New cards

Greenhouses Gases

Gases in the atmosphere that absorb and re-emit infrared radiation, which traps heat and warms the earth.

22
New cards

How are greenhouse gases able to absorb infrared energy?

They have an asymmetric molecule shape.

23
New cards

What is the most important greenhouse gas and why?

Water vapor, because it has the largest role in the natural greenhouse effect.

24
New cards

Why is carbon dioxide a notable greenhouse gas?

It is the most human-controlled greenhouse gas.

25
New cards

Greenhouse Effect

Gases absorb and re-emit heat that is emitted from the Earth after sunlight warms the Earth.

26
New cards

What happens to the wavelengths that get trapped by the Greenhouse Effect?

They get sent back to Earth.

27
New cards

Why is the Greenhouse Effect so important?

It is essential to life because it keeps the Earth warm enough for liquid water.

28
New cards

Band Saturation

Greenhouse gases absorb infrared radiation at specific wavelength bands

29
New cards

What happens when you add more gas to the Greenhouse Effect?

Total absorption still increases even if the main band is already mostly full, which means more heat is trapped in the atmosphere.

30
New cards

Heat Capacity

How much energy something can absorb before its temperature changes.

31
New cards

High Heat Capacity

Absorbs lots of heat without temperature changing much.

32
New cards

Low Heat Capacity

Heats up and cools down quickly.

33
New cards

Does water have a high or low heat capacity?

Very high. It buffers temperature changes and keeps climates more stable.

34
New cards

Water Triple Point

The temperature and pressure where water can exist simultaneously as ice, liquid, and vapor. Show how water transitions between it's forms.

35
New cards

Sensible Heat

Heat you can feel as the temperature changes.

36
New cards

How is sensible heat transported in the atmosphere?

Transported via conduction, convection, and advection. All directions.

37
New cards

Latent Heat

Energy absorbed or released when a substance changes form without changing its temperature.

38
New cards

How is latent heat transported in the atmosphere?

Transported via rising and moving water vapor. This is how the Earth redistributes energy.

39
New cards

Troposphere

The lowest layer of Earth's atmosphere. Where weather happens and water vapor is stored. It's behavior controls climate and weather.

40
New cards

Convection Cell

A loop of rising warm air and sinking cool air, moving heat and moisture in the atmosphere and driving weather patterns.

41
New cards

What happens to rising air?

Cools and condenses, forming clouds and precipitation.

42
New cards

What happens to sinking air?

Dries and warms.

43
New cards

Coriolis Effect

Earth's rotation making moving air/water bend, which determines the rotation of storms and the path of winds.

44
New cards

What direction does air move in the Northern Hemisphere?

To the right.

45
New cards

What direction does air move in the Southern Hemisphere?

To the left.

46
New cards

What direction do hurricanes rotate in the Northern Hemisphere?

Counterclockwise.

47
New cards

What directions do hurricanes rotate in the Southern Hemisphere?

Clockwise.

48
New cards

Hadley Cells

A tropical atmospheric circulation cell where warm air rises near the equator, moves toward 30° latitude, cools and sinks, creating trade winds and deserts around 30° N/S.

49
New cards

Ferrel Cells

A mid-latitude circulation cell where air moves poleward near the surface and equatorward aloft, connecting Hadley and Polar cells; responsible for westerlies in 30-60° latitudes.

50
New cards

Polar Cells

A polar atmospheric circulation cell where cold air sinks at the poles, flows toward 60° latitude, rises, and returns poleward aloft; drives polar easterlies.

51
New cards

Orographic Precipitation (Rain Shadows)

Mountains make air rise, causing rain on the windward side and dry conditions on the leeward side.

52
New cards

What happens on the windward side of a mountain (Orographic Precipitation)?

Facing the wind causes rain or snow as air cools and condenses

53
New cards

What happens on the leeward side of a mountain (Orographic Precipitation)?

Air descends, creating a rain shadow as air warms and dries.

54
New cards

Surface Ocean

The top layer of the ocean (top 100-200 meters). Makes up 10% of ocean water.

55
New cards

Deep Ocean

The lawyer below the surface ocean, extending to the ocean floor (deepest parts are 11,000 meters). Makes up 90% of ocean water.

56
New cards

How does wind act as a driver of surface ocean currents?

Pushes water up, creating large global currents.

57
New cards

How do tides act as a driver of surface ocean currents?

Pull water with gravitational forces, creating coastal currents.

58
New cards

Eckman Transport / Eckman Spiral

Wind moves the surface water of the ocean, but the Coriolis effect twists the motion with depth, forming the Ekman Spiral.

59
New cards

Ocean Gyres

Giant circular ocean currents driven by wind and Earth's rotation that move heat around the planet.

60
New cards

What are Ocean Gyres caused by?

Wind, the Coriolis effect, and continents blocking water flow.

61
New cards

What direction do Ocean Gyres rotate in the Northern Hemisphere?

Clockwise.

62
New cards

What direction do Ocean Gyres rotate in the Southern Hemisphere?

Counterclockwise.

63
New cards

Upwelling

When deep, cold water rises to the ocean, bringing nutrients that support marine life.

64
New cards

Causes of upwelling along coastlines

Wind blows along the coast, and Ekman transport pushes water away from the shore, causing deep water to rise and replace it.

65
New cards

Causes of upwelling along the equator

Winds blow west, Coriolis effect pushes surface water away from the equator, and deep water rises to replace it.

66
New cards

Downwelling

Surface water sinks to the deep ocean.

67
New cards

What causes downwelling along coasts?

Wind blows along the coast, Ekman transport pushes surface water toward the shore, and water piles along the coast and sinks downwards.

68
New cards

Thermohaline Circulation

Dense water sinks, less dense water rises, creating deep and surface currents.

69
New cards

Pattern of Thermohaline Circulation

Surface water sinks, deep water moves along the ocean floor, deep water rises (upwelling).

70
New cards

Ocean Heat Transport

Moves heat very slowly, mainly though ocean currents.

71
New cards

Atmospheric Heat Transport

Moves a lot of heat quickly, through winds and convection.

72
New cards

El Niño

Trade winds weaken, warm water spread eastward across the Pacific, causing warmer global temperatures.

73
New cards

La Nina

Trade winds strengthen, pushing warm water westward and more cold water upwells in the east, causing cooler global temperatures.

74
New cards

Short-Term Carbon Cycle (days to decades)

Fast carbon moves between air, plants, animals, and surface ocean.

75
New cards

Long-Term (Thousands to millions of years)

Slow carbon moves through rocks, sediments, and deep ocean, controlling climate over millions of years.

76
New cards

Carbon Reservoirs

Where carbon is stored.

77
New cards

Carbon Fluxes

How carbon moves.

78
New cards

Residence Times

How long carbon stays.

79
New cards

Do small carbon reservoirs have a short or long residence time?

Short.

80
New cards

Do big carbon reservoirs have a short or long residence time?

Long.

81
New cards

Photosynthesis

The process by which plants use sunlight to make energy.

82
New cards

Plant Respiration

Plants use some of the sugar they made in photosynthesis for energy, releasing CO2 back into the atmosphere.

83
New cards

Soil Respiration

Microbes break down dead plant material and organic matter in soil, releasing CO2.

84
New cards

Permafrost

Soil or sediment that remains frozen for at least two consecutive years.

85
New cards

Why does permafrost store so much carbon?

Because plant material cannot fully decompose in the cold.

86
New cards

Does cold or warm water hold more CO2?

Cold

87
New cards

Biological Pump for Ocean Carbon

Carbon is physically moved downward via living organisms.

88
New cards

Physical Pump for Ocean Carbon

Carbon is transported by water movement and solubility, not biology.

89
New cards

What happens to CO2 in polar regions?

It gets absorbed and sinks.

90
New cards

What happens to CO2 in warm regions?

It gets released, and these regions become a carbon source.

91
New cards

Calcium Carbonate

Stores carbon in rocks and sediments for millions of years. A major part of the crustal carbon reservoir, helps regulate long-term climate.

92
New cards

Volcanic Emissions

Calcium carbonate -> buried sediments -> subduction -> volcanic CO2

93
New cards

What does the chemical weathering of Silicate Minerals do?

Slowly reduces atmospheric CO2 and helps stabilize Earth's climate over millions of years.

94
New cards

Is Silicate Weathering Feedback positive or negative?

Negative feedback because it opposes the temperature change.

95
New cards

Where does coal come from?

Land plants that have been buried in swamps.

96
New cards

Where does petroleum come from?

Marine plankton and algae, which have been mixed with sediments on the ocean floors.

97
New cards

Stable Carbon Isotopes

Rising atmospheric CO2 is becoming mode C12 heavy, showing the source of carbon is ancient plant material (fossil fuels).

98
New cards

Radioactive Carbon Isotopes

Fossil Fuels are so old that there is no C14 left. If atmospheric CO2 is less, it indicates the source is fossil carbon, not plants.

99
New cards

Ice Cores

Cylinders of ice drilled from glaciers or ice sheets, trap ancient air bubbles and give a direct record of past atmospheric gases.

100
New cards

Tree Rings

Show seasonal growth patterns.