Energy and Radiation Laws Flashcards

1
Q

Energy

A

the ability to do work, and work is done when a unit force acts over unit distance.

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

Forms on energy in atmosphere

A

Radiant energy - electromagnetic waves (Sun, hot fire, clouds, any
object)
- Sensible heat – thermal energy we can feel (warm air)
- Latent heat – due to phase changes of a substance, especially water
(cooling we feel after getting out of the swimming pool)

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

Thermodynamics:

A

Physics that deals with the relationships and conversions

between heat and other forms of energy.

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

Conservation of energy:

A

Energy can be neither created nor

destroyed, but can be converted from one form to another.

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

Energy balance:

A

Within a system all inflows and outflows of

energy and mass have to balance.

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

Radiant energy, in the form of electromagnetic

waves…

A

is emitted at the speed of light by all objects with a

temperature above absolute zero (-273° C)

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

Electromagnetic radiation

A
  • Emitted from all matter
  • has a wide spectrum of wavelengths
  • Can travel in a vacuum (space)
  • Travels in straight lines
  • Travels at C=3 x 108 m s-1
    (speed of light). e.g. it takes 8
    min 20 s for radiation to travel from the Sun to the Earth
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Wavelength

A

distance between crests in mm

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

Planck’s Law

Every:

A

object emits radiation at all times and at all
wavelengths.
- gives the amount of blackbody monochromatic (single wavelength) radiative flux, called
irradiance,

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

Wien’s Law

States:

A

the wavelength of maximum emission

from a blackbody is inversely proportional to its absolute T of its surface

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

Kirchhoff’s Law

A

assuming no transmission the absorptivity of a body equals its emissivity

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

Stefan-Boltzmann Law

A
  • The total energy emitted by a blackbody is proportional to
    the fourth power of its absolute T:
  • Natural objects are not full radiators. The emittance from
    these objects (called grey bodies)
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

What does an infrared thermometer do?

A

It uses the uses the Stefan-Boltzmann
law and can be used to
measure the surface
temperature of objects

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

Thick clouds on a satellite image look:

A

bright white

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

thin clouds on a satellite image look:

A

greyish

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

Bright clouds mean:

A

cold and a higher top

17
Q

Feathery, not too bright and relatively thin clouds that appear white mean…

A

They have cold tops and are categorized as cirrus

18
Q

Fairly bright, modestly thick clouds with a greyish appearance means…

A

They are low clouds and can be classified as stratocumulus

19
Q

Solar constant:

A

the solar radiant flux density (irradiance) at top of Atmosphere, normal to solar beam, at Earth’s mean distance from
Sun

20
Q

Cosine law of radiation

A

Describes how the incident radiant flux density of a
beam decreases as the beam’s angle varies from overhead
(normal) to a more slanted path relative to the surface

21
Q

What surface properties control incident

radiation?

A
  • absorptivity: fraction of incident radiation
    absorbed
  • reflectivity: fraction reflected from the surface
  • transmissivity: fraction transmitted through the
    surface
22
Q

Absorption:

A

the full energy transfer from

radiation to a substance

23
Q

Atmospheric absorption varies by

substance:

A
UV – absorbed by O3
(stratosphere)
Visible – hardly absorbed
Infrared – partially absorbed by water
vapour, CO2
24
Q

Scattering

A

– the deflection of radiation

by a substance

25
Q

Diffuse scattering

A

– radiation deflected
in many directions, becomes diffuse
radiation

26
Q

Reflection

A

– a type of scattering,
radiation is deflected back with equal
intensity (mirror)

27
Q

Albedo

A

– the fraction of light reflected

earth’s albedo is ~0.3

28
Q

Lowest albedos

A
(best absorbers) are open water, organic soils,
coniferous forest (0.03-0.15)
29
Q

Highest albedos

A
(poor absorption) are snow, ice, dry light soils,
desert sand (0.35-0.95)
30
Q

Intermediate albedos

A
deciduous forest (0.15-0.2), agricultural
crops (0.2-0.25)
31
Q

Scattering affects:

A
• The blue sky and red sunsets 
(Rayleigh scattering)
• Hazy or polluted days making the sky white
or gray (Mie scattering)
- White clouds (nonselective scatterin
32
Q

Rayleigh

scattering

A
the smallest
gaseous
molecules and
aerosols responsible for
blue sky and red
sunsets
33
Q

Mie

scattering

A
by
larger particles
(e.g. water
droplets).
Produces hazy
and whiter
skies. Heavy
aerosol
pollution
causes even
redder sunset
34
Q

non-selective scattering

A
  • bigger particles
  • individual droplets:
    refraction ➔ rainbow