Earth's Energy Balance Flashcards

1
Q

What is the first law of thermodynamics?

A

Conservation of energy- energy cannot be created or destroyed only changed from one form to another.

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

What is entropy?

A

• Entropy is a measure of the unavailability of a
system’s heat energy for conversion to other
forms of energy
• Lower entropy – more energy the system has
for conversion to other forms of energy
• Higher entropy – more disorganized system

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

What is the second law of thermodynamics?

A

– entropy increases with time so the system becomes

more disorganized

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

Distinguishing between temperature and heat

A
  • Temperature – measure of the mean kinetic energy (speed) per molecule of an object (internal energy)
  • Heat – measure of total kinetic energy of all the molecules of an object
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Distinguishing between sensible and latent heat

A

• Sensible heat – heat acquired by transfer from
an object of higher temperature
• Latent heat – heat acquired when a body
changes to a higher state (solid to liquid or liquid
to gas). Heat added at the change of state
doesn’t raise the temperature

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

Heat transfer Processes- Conduction

A

Conduction – molecular impact without the

transfer of matter itself (heat transfer in solids)

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

Heat transfer Processes- Convection

A

Convection – involves the movement of large
volumes of the substance itself (mode of heat
transfer in fluids)

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

Heat transfer Processes- Radiation

A

Radiation – electromagnetic emission from a

body

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

Radiation

A

• Does not require a medium to travel through
• Has both a wave structure and a particle (photon) structure
• Spectrum of wavelengths
• Radiation laws – show that the amount of radiant energy emitted by an object is much greater as temperature
increases and is wavelength dependent

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

Global radiation receipt

A

Sum of all short-wave radiation received from
direct solar radiation and indirect diffuse radiation
Reflects astronomical factors and the distribution
of clouds
Shows a strong diurnal variation in intensity

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

Albedo

A

A measure of the reflecting power of a

surface (reflectivity)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

The Natural Greenhouse Effect

A

• Water vapour, CO2 and other trace gases absorb
long-wave radiation emitted by the Earths surface
– re-emitting some back to Earth
• Without the natural Greenhouse Effect, the Earth
would be much colder

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Radiative forcing of climate- forcing

A

Forcing – Processes acting as external agents to the
climate system that change the energy balance – e.g.
loading of the atmosphere with aerosols (particles)

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

Give examples of forcing

A

– Such forcing can occur naturally after volcanic eruptions or wildfires for example
– Aerosols scatter/reflect radiation and act as condensation nuclei promoting cloud formation
– Tropospheric sulphate aerosols slightly increase the atmospheric albedo – slight cooling effect (negative feedback)

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

Radiative forcing of climate- feedback

A

Feedback – Internal agent acting in response to forcing

agents (either negative or positive)

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

What is absolute zero?

A

As temperature decreases and the molecules are at complete rest where there is no internal energy, it is known as absolute zero.

17
Q

How does radiation travel?

A

Radiation does not require any medium through which to travel and so it can pass through a vacuum with the speed of light.

18
Q

What is a black body?

A

One that absorbs all the radiation falling on it and that emits, at any temperature, the maximum amount of radiant energy.

19
Q

Why is albedo important?

A

It determines the fraction of the incoming solar radiation that is absorbed by the surface.
The greater the albedo, the less solar radiation is absorbed.

20
Q

What is net radiation?

A

The difference between the total incoming and the total outgoing radiation.

21
Q

What is the effect of thermal inertia?

A

To delay the atmospheric and oceanic response to various climate forcings.

22
Q

What does the presence of thermal inertia imply?

A

That still greater climate changes will be in store for present increased atmosphere CO2 levels, which may be difficult or impossible to avoid.

23
Q

What is the primary symptom of the climate system’s thermal inertia, in the presence of increasing greenhouse gas concentrations?

A

An imbalance between the energy absorbed and emitted by the planet.

24
Q

What did Hansen (2005) discover?

A

Using a climate model, driven mainly by increasing human-made greenhouse gases and aerosols, among other forcing that the sun is now absorbing 0.85 +/- 0.15 W m-2 more energy from the sun than it is emitting to space.

25
Q

What is the imbalance between the energy absorbed and emitted by the planet confirmed by?

A

Precise measurements of increasing ocean heat content over the past 10 years.
This implies an expectation of additional global warming of about 0.6oC without further change of atmospheric composition.

26
Q

IPCC Working Group 1, Fourth Assessment Report (2007a) estimated that..

A

a further 0.6oC unavoidable warming by the end of the century relative to 1980-1999 even if atmospheric greenhouse levels remain at 2000 levels.

27
Q

IPCC Working Group 2, Fourth Assessment Report (2007b) commented that…

A

this leads to the conclusion that there are some impacts for which adaptation is the only available and appropriate response.

28
Q

What is lost and gained in terms of radiation in the atmosphere?

A

The atmosphere loses more heat to space in the form of long wave radiation than it gains from the absorption of short wave radiation, and this is the equivalent to a cooling of 1 or 2 degrees per day.

29
Q

What is the majority of the heat lost to space in long term radiation?

A

The latent heat released by atmospheric water vapour that has evaporated from the surface, condensing to form precipitation.

30
Q

What maintains the mean equilibrium atmospheric temperature?

A

A balance between radiative cooling and condensational heating.

31
Q

Radiation has

A

a wave and a particle structure

32
Q

Incoming radiation from the sun is predominantly

A

shortwave

33
Q

• Radiation laws –

A

show that the amount of radiant energy emitted by an object is much greater as temperature increases and is wavelength dependent