EAE3111 Chapter 6

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

1/99

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 6:14 AM on 6/19/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

100 Terms

1
New cards

Mean

Seasonal or daily cycles

2
New cards

Variability

Difference to the long time mean

3
New cards

Standard deviation

Spread of a distribution, strength of the variability

4
New cards

Correlation

How much two variables tend to have anomalies at the same time

5
New cards

Central limit theorum

Tendency of long term averages to have less variation than a single data point

6
New cards

Time scale dependence of variability

Increasing the time scale reduces the variability

7
New cards

Characteristics of climate variability: strength

More variability over land

8
New cards

Characteristics of climate variability: time scales

Longer time scales have less variability, different regions have different time scales.

9
New cards

Oscillation

Positive and negative anomalies taking turns on irregular time intervals

10
New cards

Chaotic

Persistence of anomalies

11
New cards

Trend

The climate drifts on one direction over time

12
New cards

Characteristics of climate variability: spatial scales

Generally larger variability over land, varies between regions.

13
New cards

Teleconnections

Unexpected connections between remote regions

14
New cards

Hoevmoeller diagram

Presents the variability of a climate variable as a function of a spatial direction versus the time dimension

15
New cards

Shorter time scale variability tends to be on

Smaller spatial scales

16
New cards

Longer time scale variability tends to be on

Larger spatial scales

17
New cards

External influences on the climate system

Climate system cannot feedback (changes in insolation, volcanic eruptions, anthropogenic forcing or meteorites)

18
New cards

Internal influences on the climate system

Dynamics of the climate system within itself given external boundary conditions

19
New cards

A stable equilibrium system

A dynamical system which, given initial conditions and certain fixed boundary conditions, would converge towards an equilibrium point.

20
New cards

Oscillating system

Highly predictable repeating cycle, with some internal variability

21
New cards

Deterministic chaos system

Tendency equations of the system are known (deterministic) but the system is largely unpredictable, varying around equilibria points in a non-periodic, chaotic and unpredictable way.

22
New cards

The Lorenz-salzman model

Simplified convection dynamics which illustrate the important characteristics of chaotic weather dynamics.

23
New cards

The Lorenz model has

3 equilibria

24
New cards

Characteristics of the Lorenz-Salzman model: no stable equilibria

Always varies, no valleys in the climate potential POV

25
New cards

Characteristics of the Lorenz-Salzman model: regime behaviour

Oscillations between two non-zero equilibria (attractors) with transitions between two regimes.

26
New cards

Characteristics of the Lorenz-Salzman model: non-periodic flow

The system never reaches the same point twice.

27
New cards

Deterministic

The tendency equations are exactly defined if the state of the system is known.

28
New cards

Chaos

The time evolution beyond a given time interval cannot be predicted, no matter how well the initial state of the system is known.

29
New cards

Characteristics of the Lorenz-Salzman model: chaotic time evolution

Only predictable up to a certain time period, depending on how precisely the initial conditions is known. There will be a point where the system fills all likely points in dynamical space.

30
New cards

Characteristics of the Lorenz-Salzman model: numerical uncertainty

No general analytical solution, thus must be estimated with numerical approximations, which are limited by computer precision.

31
New cards

Characteristics of the Lorenz-Salzman model: non-linear response to forcing

As the distribution shifts, the shape changes (shifting to higher values results in the lower value regime becoming more likely)

32
New cards

Stochastic climate variability

Randomness of climate variability on larger and longer time and spatial scales results from chaotic weather on shorter and smaller time and spatial scales.

33
New cards

The Power Spectrum

How much each frequency contributes to the variability of the time series

34
New cards

Area under the power spectrum curve

Total variance over the range of frequencies

35
New cards

White noise

Power spectrum has the same amount of variance for all frequencies, result of a time series of purely random numbers.

36
New cards

Red noise

Climate can vary on long time scales without a cause (external forcing) simply due to the weather variability that exist on shorter time scales.

37
New cards

Red Noise Null Hypothesis

The system is linearly damped and forced by white noise (random weather)

38
New cards

Slab ocean model

An example of red noise process, the ocean is just a heat capacity that integrates atmospheric sensible heat fluxes

39
New cards

Glacier red noise model

An example of a red noise process, the glaciers mass is controlled by random weather events of snow accumulation and melting

40
New cards

SST variability is in the order of

0.5ºC

41
New cards

Elements of the spatial complexity: domain boundaries

Coastlines or mountains

42
New cards

Elements of the spatial complexity: different mean states

Wind directions, temperature

43
New cards

Elements of the spatial complexity: different dynamics

Coriolis force or water vapour saturation pressure

44
New cards

Principle component analysis or empirical orthogonal functions (EOFs)

Dimensionality reduction to explain the maximum amount of variance in data.

45
New cards

Statistical modes

Has three elements: Data = Amplitude * EOF Pattern * time series

46
New cards

Climate variability of the domain at any given time

Sum of all modes with the pattern * the amplitude * the current value of the time series

47
New cards

Mode hierarchy

The modes are in order by how much of the data they can explain

48
New cards

Maximum variance

The EOF analysis is the optimal approach to maximise the explained variance in one mode

49
New cards

Orthogonal

The EOF modes are not similar to each other, thus the time series and patterns of two modes is uncorrelated

50
New cards

Multipoles

Orthogonality constraints lead to multi-pole like patterns in the whole domain.

51
New cards

Null hypothesis for spatial structure

Nearby regions will influence each other to behave similarly over time (isotropic diffusion), red noise but on the spatial scale

52
New cards

Climate mode

A reappearing pattern in space or time that is potentially predictable beyong stochastic red noise.

53
New cards

Deviation from chaos

Structure in variability beyond the simple stochastic model

54
New cards

A phyiscal mode

You can predict the next phase of the oscillator by knowing the current state of the system, a swing or a pendulum

55
New cards

Phase space

The system moves from one phase to the next in a highly predictable manner

56
New cards

Two variables can be measured with an out-of-phase relation

Position and velocity

57
New cards

When position is at maximum

Velocity is at zero

58
New cards

Level 1: subjective / impact focused

Usually defined based on a statistical mode, subjective, no physical oscillator or deviations from pure noise.

59
New cards

Damped persistence

Current anomalies will persist in the near term, but mathematically decay toward zero

60
New cards

Level 2: structures different from noise

Indications of deviations from pure noise, not clear is this is a physical mode, could be chaotic but different from red noise.

61
New cards

Level 3: a physical mode/predictable oscillator

A structure different from red noise, physical phase space with clear propagation, predictable beyond damped persistence

62
New cards
<p>The green circle is</p>

The green circle is

Mode: deterministic

63
New cards
<p>The red circle is </p>

The red circle is

Chaos: stochastic climate

64
New cards

El Nino originated in

South American fisheries

65
New cards

Southern Oscillation

Pressure difference between Tahiti and Darwin

66
New cards

ENSO coupling origin

Bjerknes identified the relation and suggested that this may account for variability in both

67
New cards

ENSO numerical model origin

Cane and Zebiak determined that an ocean and atmospheric model could reproduce the ENSO mode

68
New cards

The El Nino

Peaks around November to January, warming

69
New cards

ENSO events are marked by a

SST pattern in the tropical pacific

70
New cards

La Nina

Not as strong as warming events, last longer, intensification of the mean state

71
New cards

ENSO lasts for

2-7 years (4 average)

72
New cards

ENSO dynamics are controlled by

Dynamics in the upper ocean tropical Pacific

73
New cards

Thermocline

Strongest ENSO variability, region of the upper ocean where the temperature decreases very quickly (change from light/warm surface water to dense/cold subsurface waters)

74
New cards

Deepening of the thermocline marks

Increased heat content before an El Nino event in the western/central equatorial Pacific, propagates to the east, followed by large-scale surface warming

75
New cards

During strong surface warming, western thermocline marks

Reduced heat content, which propagates to the east, introducing the La Nina event

76
New cards

Prominent teleconnection of ENSO

Reduced Indian monsoon and reduced hurricanes during El Nino

77
New cards

Tropical pacific mean state is marked by

A strong temperature gradient from east (cold) to west (warm)

78
New cards

Equatorial cold tongue

Result of prevailing easterly trade winds (Hadley cell induced boundary conditions) and the Ekman ocean currents induced by friction and Coriolis forcing

79
New cards

Easterly winds lead to

Pile up of warm water and higher sea level on the western side

80
New cards

The thermocline has an

East to west gradient

81
New cards

Coriolis forcing results in _ at the equator

Divergence

82
New cards

Walker circulation

Secondary tropical circulation, with rising over the western warm pool and cooling over eastern equatorial Pacific.

83
New cards

Walker circulation results in _ surface pressure in the west and _ surface pressure in the east

Low, high

84
New cards

Bjerknes feedback: SST forces zonal wind

Warm SST causes heating in the atmosphere, low surface pressure and a reduced zonal easterly wind

85
New cards

Bjerknes feedback: Zonal wind forces thermocline

Easterly zonal winds keep the western Pacific thermocline deeper, weakening leads to a shallowing of the thermocline which propagates to the east.

86
New cards

Bjerknes feedback: Thermocline forces SST

A deeper thermocline in the east reduces the upwelling of cold subsurface waters along the equator and the south American coasts, leading to warming of SST.

87
New cards

Thermohaline circulation

Deep ocean circulation that spans the global oceans

88
New cards

Reduced North Atlantic MOC during warming is due to

Reduced temperature gradients between tropics and polar regions and poles warm more strongly

89
New cards

Density differences between two boxes in the Stommel model are controlled by

Temperature and salinity differences

90
New cards

If temperature differences dominate in the Stommel model

Surface flow is from the equatorial box to the polar box, reducing temperature gradients

91
New cards

If salinity differences dominate in the Stommel model

Surface flow is from the polar box to the equatorial box, reducing the temperature in the equatorial box

92
New cards

Proxy data

Data from the past climate not related to direct measurements.

93
New cards

Milankovitch cycles

Cause the glacial cycles dominating the last 500,000 years, with warm periods every 100,000 years

94
New cards

The biggest driver of ice age cycles is most likely

Variations in earth’s orbit around the sun, caused by other planets and the moon (milankovitch cycles)

95
New cards

Glacier feedbacks

Ice albedo, water vapour, altitude cooling and atmospheric circulation

96
New cards

Ocean CO2 uptake feedback

Cold oceans can uptake more CO2 than warm oceans.

97
New cards

Eccentricity

The shape of the earth’s orbit around the sun

98
New cards

Precession

The position of the seasons within the orbit around the sun

99
New cards

Obliquity

Changes in the angle of tilt of Earth’s axis rotation

100
New cards