Final Study Guide 9 Flashcards

Paleo Climate

1
Q

What is Earth systems science?

A

Earth system science seeks to integrate various fields of academic study to understand the Earth as a system.Earth system science embraces chemistry, physics, biology, mathematics and applied sciences in transcending disciplinary boundaries to treat the Earth as an integrated system and seeks a deeper understanding of the physical, chemical, biological and human interactions that determine the past, current and future states of the Earth. Earth system science provides a physical basis for understanding the world in which we live and upon which humankind seeks to achieve sustainability.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

What is the greenhouse effect?

A

trapping of the sun’s warmth in a planet’s lower atmosphere due to the greater transparency of the atmosphere to visible radiation from the sun than to infrared radiation emitted from the planet’s surface.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Why is albedo a critical factor in climate-related feedbacks?

A
  • Albedo- used to define the percentage of solar energy reflected back by a surface
  • Understanding local, regional, and global albedo effects is critical to predicting global climate change
  • The following are some of the factors that influence the earth’s albedo: clouds, ice,snow,surface, oceans and forests
  • It is a very strong “positive feedback” (increases an initial warming) that has been included in climate models since the 1970s
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

List some of the long-term climate variability

A
  • solar
    > changes in the intensity of solar radiation reaching earth
  • volcanic
    > eruptions add aerosols to the atmosphere, increasing reflection of radiation
    > adds CO2, which increases global warming
  • greenhouse gases
    > adds CO2, which increases global warming
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

How do we know past climate before the instrumental era?

A

Historical records; change in growth (tree rings, speleothems, corals); changes in organism/plant distribution (pollen records); chemical records (changes in isotopic ratios, in ice and sediment cores); geological evidence (glacial sediments)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Weather

A

natural phenomena within the atmosphere at a given time (seconds to hours to days)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Climate

A

the average weather conditions, and their range of variability, over a long period of time (~30 years or more)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Radiative Balance

A

the solid earth + atmosphere receive heat energy from the sun but they also radiate the same amount of heat back into space

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Frequency

A

the number of times that something happens during a particular period

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Wavelength

A

distance from one wave of energy to another as it is travelling from one point to another point

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Electromagnetic Spectrum

A
  • is the range of all possible frequencies of electromagnetic radiation; the “electromagnetic spectrum” of an object has a different meaning, and is instead the characteristic distribution of electromagnetic radiation emitted or absorbed by that particular object
  • Higher frequency = more energetic
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Wien’s Law

A
  • relationship between temperature of a black body and the wavelength at which it emits the most light
  • wavelength of emitted radiation is shorter for bodies at higher temperatures
  • Used to infer the temperature of the sun
  • Sunlight wavelengths ~500 nm (UV radiation)  5500-6000 K
  • Objects that are cooler radiate longer wavelengths – so Earth radiates long wavelengths (red)
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Black body radiation

A

radiation emitted by non-reflective body held at constant temperature- used to approximate radiation from stars and planets

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Absorption

A

is the way in which the energy of a photon is taken up by matter, typically the electrons of an atom; thus, the electromagnetic energy is transformed to other forms of energy for example, to heat

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Spectrum

A

group of colors that a ray of light can be separated into including red, orange, green, blue, indigo, and violet: the colors can be seen in a rainbow

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Greenhouse effect

A

Energy radiated by the sun converts to heat when it reaches earth. Some heat is reflected back through the atmosphere, while some is absorbed by atmospheric gases and radiated back to earth.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

Solar constant

A

a measure of flux density, is the amount of incoming solar electromagnetic radiation per unit area that would be incident on a plane perpendicular to the rays, at a distance of one astronomical unit (AU) (roughly the mean distance from the Sun to the Earth)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

Hadley cells

A
  • a large-scale atmospheric convection cell in which air rises at the equator and sinks at medium latitudes
  • Steps:
    > Moist warm air expands, rises
    > Cools, condenses, rain falls
    > Dense air sinks in sub tropics
    > Warmed, dry air
 spreads at surface
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

Great ocean conveyor

A
  • refers to a part of the large-scale ocean circulation that is driven by global density gradients created by surface heat and freshwater fluxes (salt driven)
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

Climate proxies

A

preserved physical characteristics of the past that stand in for direct measurements (as statistical proxies), to enable scientists to reconstruct the climatic conditions that prevailed during much of the Earth’s history

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

El Nino (drought)

A
  • refers to the climatic conditions associated with temperatures in the eastern south pacific - in years with weak trade winds, these waters wam, and the warmer water influence global climate
  • hard to predict
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

La Nina

A
  • Warm ocean temperature in western pacific

- Opposite of El Nino

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

Paleoclimatology

A

is the study of changes in climate taken on the scale of the entire history of Earth

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

Forcings

A
  • external boundary conditions or inputs to a climate model
  • Main long-term climate forcings:
    > Solar: changes in the intensity of solar radiation reaching the Earth
    > Volcanic: eruptions add aerosols to the atmosphere that increase reflection of radiation over short periods of time, but also add CO2 to the atmosphere that increases greenhouse warming over long periods
    > Greenhouse forcing: addition of CO2 to atmosphere contributes to climate warming
25
Q

Ice Core

A
  • a core sample that is typically removed from an ice sheet, most commonly from the polar ice caps of Antarctica, Greenland or from higher mountain glaciers elsewhere
  • Lower layers are older than upper layers of snow (and an ice core contains ice formed over a range of years)
  • The properties of the ice can then be used to reconstruct a climate record over the age range of the core, normally through isotopic analysis
  • This enables the reconstruction of local temperature records and the history of atmospheric composition
26
Q

Milankovitch Cycle

A

theory describes the collective effects of changes in the Earth’s movements upon its climate; explains the repeating, cyclical changes from glacial to interglacial

27
Q

Orbital Changes

A

changes solar energy reaching Earth-> changes in global climate

28
Q

Glacial/Interglacial (Cycles)

A
  • the cycles are caused by variations in the Earth’s orbit through time have changed the amount of solar radiation received by the Earth in each season
  • Interglacial periods tend to happen during times of more intense summer solar radiation in the Northern Hemisphere
29
Q

Precession

A
  • the trend in the direction of the Earth’s axis of rotation relative to the fixed stars, with a period of roughly 26,000 years; is due to the tidal forces exerted by the Sun and the Moon on the solid Earth, which has the shape of an oblate spheroid rather than a sphere
  • The Sun and Moon contribute roughly equally to this effect
30
Q

Obliquity

A

a deviation from a vertical or horizontal line, plane, position, or direction.

31
Q

Albedo

A

the proportion of the incident light or radiation that is reflected by a surface, typically that of a planet or moon. Like the snow that reflects the sunlight to prevent the surface of the earth from overheating.

32
Q

Photons

A

elementary particles (one of the basic building blocks) characterized by oscillating electrical and magnetic fields that propagate through space. They behave like particles and waves.

33
Q

Boltzmann’s Law

A

S(amount of energy emitted by black body)= K(constant)x T^4(temperature)

34
Q

Methane

A
  • Driver of Climate Change
  • Along with CO2, nitrous oxide, Methane levels have reached levels that are unprecedented in the last 800,000 years
  • Green house gas
35
Q

Ozone

A
  • helps make up the atmosphere, especially the stratosphere
  • helps filter out incoming UV light from the sun
  • acts like greenhouse gas, absorbs outgoing infrared energy from earth
36
Q

Thermo-haline circulation

A
  • large scale ocean circulation driven by global density gradients created by surface heat and freshwater fluxes
  • same as ocean conveyor belt
37
Q

ENSO

A

El-Nino-Southern Oscillation

38
Q

Global Circulation Models

A
  • A computerized model of general circulation of the atmosphere
  • Analog for non-linear oscillator system
  • Stress vs. time graph (stick slip cycle)
39
Q

Discretization

A

the process of transferring continuous models and equations into discrete counterparts. This process is usually carried out as a first step toward making them suitable for numerical evaluation and implementation on digital computers

40
Q

Chaotic

A

sensitive dependence on initial conditions

Unpredictable over long times (weather forecast)

41
Q

Non-linear systems (like Climate) can be

A
  • metastable
  • phase state depends on crucially on parameters
  • chaotic
42
Q

Control parameter

A
  • parameters that can affect climate

> time of year, ocean temp, albedo, continentality, etc.

43
Q

Periodic Doubling

A

switching to a new behavior with twice the period of the original system

44
Q

Poincare Section

A

A method for examining the motion of dynamical systems; essentially the Poincare section provides a means to visualize an otherwise messy, possibly aperiodic, attractor. It the flow has an attractor, we should see it in the Poincare section

45
Q

Attractor

A

In dynamical systems, an attractor is a set of physical properties toward which a system tends to evolve, regardless of the starting conditions of the system.[1] Property values that get close enough to the attractor values remain close even if slightly disturbed.

46
Q

Phase space

A

A space in which all possible states in a system are represented

47
Q

Sensitive dependence on initial condition

A

small changes in one area of a system can result in large changes later

48
Q

Lyapunov Exponent

A

exponent of a dynamical system is a quantity that characterizes the rate of separation of infinitesimally close trajectories.

49
Q

Lorenz System

A

Lorenz attractor is a set of chaotic solutions of the Lorenz system which, when plotted, resemble a butterfly or figure eight. Atmospheric convection system in choatic parameter space.

50
Q

Bifurcation

A

means the splitting of a main body into two parts.

51
Q

Tipping Point

A

A tipping point is an example of hysteresis in which the point at which an object is displaced from a state of stable equilibrium into a new equilibrium state qualitatively dissimilar from the first.

52
Q

Metastability

A

describes the extended time spent by an isolated system in a long lived configuration other than the system’s state of least energy.

53
Q

Speleothem

A

a cave formation or “cave deposit” is a secondary mineral deposit formed in a cave. typically formed in limestone.

54
Q

δ18O

A

measure of the number of stable isotopes. Used as a measure of temperature of precipitation.

55
Q

Isotopes

A

variations in an element due to a different number of neutrons (all isotopes of an element have the same number of protons.

56
Q

Medieval Warm Period (MWP)

A
  • Warm period from 950-1250

- Marked some of the warmest weather in those regions for the time, but lower temps than the current global temps

57
Q

Little Ice Age (LIA)

A
  • A period of cooling after the Medieval Warm Period from 1550-1850
  • Modest cooling in the Northern Hemisphere
  • Consisted of largely independent regional climate changes instead of global cooling
58
Q

Eccentricity

A
  • Parameter associated with every conic (cone) section.
  • Measure of how conic the section deviates from being circular
  • relates to the Milanokovitch Cycle; eccentricity and the term orbital changes are essentially the same.
59
Q

Climate Proxies

A
  • geological objects sensitive to climate
  • Allow us to reconstruct temp before thermometers
    > rock and fossils, glacial evidence, tree rings, historical records, instruments (now)
  • often tied to stable water isotopes