Radiation Flashcards

1
Q

What is the electromagnetic spectrum of an object

A

Characteristics distribution of electromagnetic radiation emitted or absorbed by that particular object

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2
Q

What are the electromagnetic spectrums

A

-Radiowaves
-Microwaves
-Infrared
-Visible
-Ultraviolet
-X-ray
-Gamma Ray

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3
Q

What is the trends of electromagnetic spectrum?

A

Wavelength gets shorter as you go down the spectrum
The frequency increases as you go down

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4
Q

What 3 things happen when thermal radiation hits a surface

A

-Can be absorbed by the surface
-Can be reflected off the surface
-Can be transmitted through the surface

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5
Q

How does temperature effect thermal radiation

A

Its intensity and spectrum

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6
Q

What happens when temperature increases in relation to wavelengths and energy

A

Wavelengths decrease and energy increases

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7
Q

What are the exchanges of radiation

A

-All bodies emit radiation to their surroundings
-All bodies receive radiation from their surrondings

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8
Q

What is prevosts theory

A

Body emits radiation at a rate which depends only on its temperature and nature of surface

A body absorbs radiation at a rate which depends only on the temperature of its surroundings and on the nature of its surface

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9
Q

“Consider a perfectly insulated body at a
temperature TB: it cannot lose or gain heat by
conduction or convection, only by radiation.
* If it is surrounded by some form of enclosure
which is maintained at a constant temperature TS”

Explain what happens in all situations of this?

A

If TB>TS the body emits radiation at a greater rate than it absorbs it so TB falls until it is equal to TS

If TS>TB the body absorbs radiation at a greater rate than it absorbs so TB rises until it is equal to TS

If TB=TS the rate of absorption is equal to the rate of emission and TB doesnt change

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10
Q

What colours are the best absorbers and emitters?

A

-Black (Best)
-White
-Gray (worst)

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11
Q

Difference between transmission and emission?

A

Transmission: Part of the radiation passes through the body
Emission: The amount of thermal radiation released or given off by a body

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12
Q

What is the Black Body?

A

An object that absorbs all the radiation which strikes it

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13
Q

What does emissivity describe?

A

Describes the surface radiation properties of a body

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14
Q

What is emissivity?

A

The ratio of energy radiated/absorbed by a particular material to energy radiated/absorbed by a black body at the same temperature

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15
Q

What do the emissivity range mean?

A

0-1
0:A body that does not emit or absorb at all
1:A body that emit at the maximum possible rate an absorbs all the energy striking it

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16
Q

A mirror has an emissivity of  = 0.1. A laser beam with a
power of 5 mW is incident on the mirror. What is the
power of the reflected beam

A

Since the emissivity is 0.1, so is the absorption factor.
10% of the power is absorbed, and 90% is reflected.
So the reflected power is 50.9 = 4.5 mW.
The rest of the power has been absorbed into the material of the mirror
and converted to heat

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17
Q

Explain how punching a small hole in the lid of an empty meal tin is a close approximation to a black body?

A

Light enters the hole and is reflected many times by the wall which will get a % absorbed each time before it reaches the hole again.

18
Q

Is the distribution of energy even?

A

No, the distributions of energy are not even and it depends on the source temperature
(for ex: heating metal red will appear first as it the longest wavelength then yellow then orange then blue and the combination appears white)

19
Q

What is Weins Law

A

Product of the wavelength of the peak of the spectrum and the temperature of the black body is a constant

20
Q

Describe the radiated power over wavelength graph

A

At lower wavelengths there is little photons so less radiated power and as wavelength increases there is a peak radiated power around the middle as there is a high number of photons at high energy

21
Q

What is weins formula?

A

Wavelengthp=0.0029/T (In kelvin)

22
Q

If the temperature of a blackbody is 500K what will the peak be?

A

p = 0.0029/500 m
= 5.8x10^-6 = 5.8 micrometer

23
Q

What is Stefans Law?

A

Gives the total intensity of the radiation over all the over all wavelengths

24
Q

Formula for Stefans Law

A

Q=oAT^4 (o=5.7x10^-8 Stefans constant, A is the area radiating and T is absolute temperature)

25
Q
A
26
Q

What is Weins law?

A

the product of the wavelength of the peak of the
spectrum and the temperature of the blackbody is a constant

27
Q

What is the formula for weins law?

A

Wavelength= Weins constant/Temperature in Kelvin (0.0029/T)

28
Q

Describe the Radiated Power vs Wavelength graph

A

Due to weins law curves with a higher radiated power peaks are at lowers wavelengths because as temperature increases wavelength max decreases

Lower temperature objects emit mainly in the infrared region

29
Q

What is Stefans Law

A

gives the total intensity (power) of
the radiation over all wavelengths

30
Q

How will Stefans Law be modified if the object isnt a perfect black body

A

Q=e (emissivity) x o (stefans consstant) x Area x Temperature

31
Q

What is the value of Stefans constant

A

5.7x10^-8Wm^-2K^-4

32
Q

A 100 W light bulb has a filament which is 0.60 m long with a
diameter of 8.010−5 m. The filament may be regarded as a black
body. Estimate its working temperature. If the filament is not a
perfect blackbody, would the working temperature be higher or
lower? Why?

A

Surface area of filament (excluding ends) = pixdxL
= pi x 8.0x10^−5x0.60 = 1.51x10−4 m2
For a blackbody, Stefan’s law:
The power of the light bulb is 100 W,
So 100 = 5.710−81.5110−4T4
Hence T4 = 1.161013 or T = 1846 K
The working temperature of the filament is 1846 K
If the filament is not a perfect black body, i.e. <1, since the electrical power
supplied stays the same, the radiated power stays the same, the working
temperature will be higher. For example, if
 = 0.9, T will rise to 1895 K.
However, the filament will be a less efficient radiator.

33
Q

What will happen if a black body at T1 is placed in an enclosure T2

A

-Heat is radiated at: Q=oxSxT1^4
Heat is absorbed at: oAT2^4
Net energy flow from the enclosure to the blackbody:oxA(T2^4-T1^4) (Heat absorbed-Heat radiated)

34
Q

A potato at a temperature of 150ºC is placed in a refrigerator whose
walls are at 2ºC. Assuming the potato is a perfect black body, and is
spherical with a diameter of 7 cm, and all heat transfer is by
radiation, calculate the rate at which it loses energy.

A

Surface area of potato =pi x d^2 = 1.54x10^−2 m2.
Power emitted is 5.7x10^−8x1.54x10^−2 x (273+150)^4 = 28.1 W
Power absorbed is
5.7x10^−8x1.54x10^−2x(273+2)^4 = 5.0 W
Thus, the potato therefore initially loses heat at 23.1 W.
This will fall with time, as it cools.
– If instead the potato was at 2ºC, and was in an oven at 150ºC, the calculation
would be the other way round: the potato would gain energy at 23.1 W.
– Microwave ovens supply much more power by restricting the wavelengths
radiated to a very narrow band which excites water molecules – they are not
black bodies

35
Q

Formula for energy of a photon

A

E=hf
E= Energy of photon
h= Plancks Constant (6.626x10^34)
f= Frequency

36
Q

Speed equation

A

c=f x wavelength
c= speed
f=frequency
wavelength

37
Q

Relationship between Energy, Frequency, and plancks constant and wavelength

A

E=hc/wavelength
E=energy
h= Wavelength (6.626x10^34)
c=speed of light (3x10^8)

38
Q

Formula for intensity

A

I=P/A
I=Intensity
P=Power
A=Area

39
Q

Surface area for a sphere?

A

A=4xpixr^2

40
Q

Surface area of a filament

A

A = 2 π r L

41
Q

What is the area of a cylinder? and what is it without the ends?

A

2nr^2+2nrh
n=pi
r=radius
h=height

Without ends:
n x d x L