Radiation and Energy Balance, Pt.1 Flashcards

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1
Q

When was our solar system formed?

A

~4.6 billion years ago

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2
Q

Our sun captured ___% of the matter from a nebula of dust and gas. The remaining ___% went to forming the remaining planets, moons, and all other objects found in our solar system.

A

99.9, 0.1

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3
Q

True or False: The sun is the only object in our solar system, massive enough to sustain nuclear fusion in its core, producing radiant energy.

A

True

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4
Q

Describe Solar Radiation:

A

Solar radiation occupies a portion of the electromagnetic spectrum of radiant energy.

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5
Q

Describe Radiant Energy:

A

Radiant energy travels at the speed of light to Earth. (~300,000 km/s). Light reaches Earth from the Sun in about 8 minutes and 20 seconds. The total spectrum of this radiant energy is made up of different wavelengths.

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6
Q

What two ways can you describe Electromagnetic Radiation (EMR)?

A

Wavelength and Frequency

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7
Q

Define a wavelength:

A

distance between adjacent wave crests (ex. Meters is too large to measure, that’s why we use nanometers.)

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8
Q

Short wavelengths have _____ frequency. Long wavelengths have ____ frequency.

A

high and low

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9
Q

Define Frequency:

A

time between passes of adjacent waves, how many waves can pass a given area in time.

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10
Q

What are the units for frequency?

A

(cycles per second, Hertz, Hz)

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11
Q

What is a nanometer?

A

A nanometer (symbol nm) is a unit of length in the metric system, equal to one billionth of a meter. It can be written in scientific notation as 1×10−9 m which is 1 / 1,000,000,000 meter. The nine signifies how many zeros we have.

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12
Q

What is a micrometer?

A

A micrometer (symbol μm) is metric system unit of length equal to one millionth of a meter, or equivalently, one thousandth of a millimeter. It is also commonly known as a micron. It can be written as 1×10−6 m, meaning 1 / 1,000,000 meter.

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13
Q

Can ‘micron’ be interchanged with micrometer?

A

Yes

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14
Q

Wavelength of radiated energy depends on _________ of the radiating body.

A

temperature

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15
Q

What kind of wave energy does the sun radiate?

A

The sun is hot, it radiates shorter wave energy, mainly visible and near infrared portion of the spectrum.

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16
Q

What kind of wavelength does the earth radiate?

A

The earth is cooler, so it radiates longer wave energy, mainly thermal infrared.

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17
Q

What does UTC mean?

A

Greenwich Mean Time

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18
Q

How do you convert UTC to Winnipeg?

A

Winnipeg = UTC –6

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19
Q

The Band 13 sensor on the satellite detects ________ radiation that is good at showing where clouds are day and night.

A

thermal infrared

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20
Q

What is Solar Energy?

A

Energy is the capacity of a physical system to do work.

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21
Q

What is the unit measurement for work?

A

1 Joule

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22
Q

How is Solar Energy generated?

A

By the nuclear fusion reaction process in which pairs of hydrogen nuclei are joined, to form helium, and emit a large amount of energy. Essentially mass is converted to energy. Pairs of hydrogen molecules join, then mass is lost and then converted into energy, then radiated to earth.

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23
Q

What is the Solar Constant? *

A

Solar Constant = Average intensity of sunlight 1372 watts per square meter (W/m2)

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24
Q

1 Watt = 1 ____

A

Joule (J) of energy/second

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25
Q

1 J = _________

A

0.239 calories and/or 1 Watt

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26
Q

True or False: the solar constant is a short term average.

A

false, its a long term average.

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27
Q

Define Sunspots:

A

Sunspots are caused by magnetic storms on the Sun. They can be more than 12 times Earth’s diameter. Their temperatures are less than the temperatures of their surroundings, which is why we see them as darker spots in images.

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28
Q

Sunspots have an activity cycle of ____ years.

A

11

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29
Q

Is it true that sunspots fluctuate over the years? Decreasing and increasing in amounts.

A

Yes.

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30
Q

True or False: The sun rotates, about once every 27 days (like the earth, faster at the equator than the poles). Increasing sunspots are from increasing solar intensity.

A

True.

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31
Q

How often does the Sun rotate?

A

Once every 27 days.

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32
Q

When/How did the measurement of sun spots begin?

A

That numbering began on January 5th, 1972, and on June 14, 2002, reached the active region number of 10,000. But since June 14th, active region reports drop at least the leading digit.
-0001, 0002. Instead of 10,001 and 10,002

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33
Q

What is Solar Wind?

A

Solar wind is clouds of electrically charged particles, principally hydrogen nuclei and free electrons.

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34
Q

What are solar winds composed of?

A

principally hydrogen nuclei and free electrons

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35
Q

True or False: Solar wind first interacts with earths magnetosphere, which deflects the solar wind toward both of Earth’s poles.

A

True.

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36
Q

Do solar winds go into the ionosphere?

A

Yes, a small portion of it enters the atmosphere and interacting with our ionosphere, producing auroras. (At 80 – 500kms above the surface).

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37
Q

Solar radiation that reaches a horizontal plane at Earth is called _________.

A

Insolation

38
Q

Insolation at the top of the atmosphere is expressed as the _____________.

A

solar constant (1372W/m2)

39
Q

What is the first level of earths energy system that interacts with insolation?

A

The Thermopause (480km)

40
Q

What region of earth receives the most insolation and why?

A

Tropics receive more concentrated insolation due to Earth’s curvature, and the migration of the subsolar point (between 23.5°N and 23.5°S).

41
Q

What three factors determine the amount of insolation received in a region?

A

-the length of the photoperiod (latitude/date), how much sun we have over the course of the day.
-the angle of incidence of the sunlight on the surface throughout the day (is the sun high in the sky, how much radiation is that beam of radiating.
-the date (distance from the sun)

42
Q

Why is the Angle of Incidence so important?

A

he angle of incidence affects the intensity of the solar beam hitting that surface, whether the beam is directly overhead (intensity of spread). The angle of incidence of solar radiation on a flat surface affects the intensity of the radiation. Becomes starker at the poles because there is a larger area receiving solar radiation. The difference between 90 degrees horizon vs. 45 degrees on the horizon (more solar radiation at the 45 degrees because it covers a larger area).

43
Q
  • __________ affects angle of incidence and intensity. *
A

Solar altitude

44
Q

What does a Sun path Diagram show us?

A

Day of year affects: Length of photoperiod, The solar altitude during the day. The half circles depict where the sun sits in the sky.

45
Q

What factors determine Intensity of Solar Radiation on a Flat Surface? (2)

A

-The intensity of the original solar radiation before it hits the surface (Io)
-The angle between the radiation and the flat surface (A)

46
Q

What is the formula to finding the intensity of radiation for an angle?

A

I = (Io) (sin A)

47
Q

What are the components in this formula, and what do they mean? I = (Io) (sin A) .

A

-I = Intensity of the radiation for angle A
-Io = Intensity of perpendicular radiation (A = 90°)
-A = the angle of incidence (measured from the surface)

48
Q

What is the significance of Sin(63.5)?

A

Highest point the sun will be throughout the year, during the Solar noon during the June Solstice! The most solar intensity is 89% of the original beam of solar radiation, what we will ever receive if the horizon is at 63.5 degrees.

49
Q

What is the significance of Sin(16.5)?

A

Sunlight striking the surface at an angle of 16.5° is only 28% as strong as perpendicular sunlight. Lowest point in the sky, during solar noon in the Winter Solstice!

50
Q

Why is Sin(90)=0?

A

Sin(90) is directly above, so there is no change in intensity (max amount of solar intensity).

51
Q

Why is Sin(0)=0?

A

Sin(0) means there is no incoming solar radiation.

52
Q

How does Sin(45)=0.71? What does this mean?

A

Sin(45), the sun is 45 degrees above the horizon, giving 71% of the solar radiation.

53
Q
  • The highest daily average of insolation value is near the____ pole in dec/Jan. The most solar insolation in a 24hour period during certain times of the year.* What solar event does this refer to?
A

South, the winter solstice.

54
Q

High values are also seen at the _____ pole in June, the pole is tilted the most toward the sun at this time of the year. What solar event does this refer to?

A

north, summer solstice

55
Q

Why are the highest daily average of insolation value is near the south pole in dec/Jan?

A

Because the pole is tilted the most toward the sun at this time of the year. (-23.5 declination)

56
Q

True or False: North and south poles get zero insolation for 6 months until we reach the equinox.

A

True.

57
Q

What is Radiant Energy?

A

EMR emitted by the sun is shortwave energy (ultraviolet, visible, shortwave infrared, and EMR emitted by the earth (aka terrestrial radiation) is longwave energy (thermal infrared).

58
Q

What types of energy are shortwave energy, and where are they emitted from, and why?

A

ultraviolet, visible, shortwave infrared, emitted from the sun, its shortwave because of the suns high heat.

59
Q

What is an example of long wave energy, where is it emitted from?

A

Thermal infrared, emitted from earth.

60
Q

What is EMR emitted by earth also known as?

A

(aka terrestrial radiation)

61
Q

What can happen to shortwave EMR that enters the atmosphere? (4)

A

-It can be transmitted through the atmosphere, without changing direction.
-It can be reflected by a body (liquid or solid) that it strikes, changing direction.
-It can be scattered by atmospheric gases/aerosols, causing it to change directions (aka diffuse reflection)
-It can be absorbed by the mass that it strikes, such that the energy of the wave is now the energy within the mass (energy changes form, from waveform to kinetic).

62
Q

In short, what can happen to shortwave EMR that enters the atmosphere?

A

Reflection, Transmitted, absorption, and scattering.

63
Q

What is Scattering AKA?

A

Diffuse Reflection

64
Q

When EMR enters the atmosphere and it goes through the process of absorption, what process occurs?

A

It is absorbed by the mass that it strikes, such that the energy of the wave is now the energy within the mass (energy changes form, from waveform to kinetic).

65
Q

Define Transmission in terms of EMR:

A

Refers to the passage of shortwave and longwave energy through the atmosphere or water, without getting blocked or reflected.

66
Q

Define Absorption in terms of EMR:

A

Absorption is the assimilation of radiation by molecules of matter and its conversion from one form of energy to another.

67
Q

** ____ and ______ absorb solar radiation and longwave radiation, good at blocking and absorbing energy from shortwave and outgoing longwave radiation. **

A

CO2 and water vapor

68
Q

Define Reflection in terms of EMR:

A

Reflection is a portion of arriving radiation that bounces directly back into space without being absorbed or performing any work.

69
Q

________ is the ratio of reflected solar radiation to the incident solar radiation.

A

Albedo

70
Q

What type of conditions can affect Albedo Reflection?

A

Light color surface versus dark color surface Smooth surface versus rough surface, light can reflect more radiation than dark surfaces.

71
Q

What does a low Albedo mean?

A

Low albedo means that more is being absorbed instead of reflected.Albedo of water surface varies with Sun altitude.

72
Q

What are some examples of a low albedo vs. a high albedo?

A

agricultural crops (low albedo) vs. fresh snow (high albedo, 0.95)

73
Q

________ is essentialy an indicator of how close a surface is to being a perfect blackbody.

A

Emissivity

74
Q

What is Scattering in terms of EMR?

A

When the sunlight (especially visible EMR) encounters gases or aerosols, the direction of the rays are changed.

75
Q

What is Scattering caused by?

A

-diffuse radiation
-The sunlight that strikes the surface without being scattered on the way down is direct-beam radiation.

76
Q

What is Diffuse Radiation and what is it related to?

A

This is the radiation that is coming down that is not coming directly to us from the sun; This is why there is light when there is no sun in the sky.

77
Q

True or False: if there was no atmosphere, the sky would be black during the day, except where the sun is located. Why is the sky blue? It’s because of scattering.

A

True

78
Q

What are the two types of scattering?

A

-Rayleigh scattering
-Mie scattering

79
Q

What is scattering determined by?

A

The particle size of radiation.

80
Q

What is Diffraction?

A

It is the spreading of waves that encounter obstacles.

81
Q

What is Refraction?

A

Change in speed and direction of light as light passes from one medium to another, bending of light as it passes through air with changing densities.

82
Q

What is the difference between refraction and diffraction?

A

-refraction of waves involves a change in the direction of waves as they pass from one medium to another;
-diffraction involves a change in direction of waves as they pass through an opening or around a barrier in their path.

83
Q

What is Rayleigh Scattering?

A

The smaller gas molecules in the atmosphere preferentially scatter shorter wavelengths (blues and violets). The scattering of 0.4 microns emr is about 9 times stronger than the scattering of 0.7 microns (wavelengths) emr.

84
Q

In what direction does Rayleigh Scattering scatter?

A

Generally scattered in all directions.

85
Q

Why is the sky blue?

A

Because the very short violet wavelengths are scattered (off of small gas molecules). Well, there is hardly any left by the time it gets to the surface…so the blues dominate. Best when the sky is clear, and the sun is high.

86
Q

What causes bluer light to be scattered in all directions?

A

When the sun is close to the horizon, it must pass through more atmosphere to get to you; and it must pass through more high-density air near the surface.

87
Q

White clouds result from strong ______ of all wavelengths, effective in ___________ all wavelengths to our eyes.

A

reflection and reflecting.

88
Q

What is Mie Scattering?

A

This is scattering of sunlight by larger molecules and particles in the atmosphere.

89
Q

What size of particles does Mie Scattering interact with? What does it produce?

A

Scatters all wavelengths about equally…which together produces white light in the sky. Produces the very whitish light around the sun.

90
Q

What size of particles does Rayleigh Scattering often interact with?

A

Particles less than 1/10th of the wavelength.

91
Q

What size of particles does Mie Scattering often interact with?

A

When particles and molecules are larger than the wavelength.

92
Q

What does it mean when the sunrise/sunset is red and orange?

A

The colors that have not yet been scattered, more opportunity for Insolation to scatter. When the sun is close to the horizon, it must penetrate a lot of atmospheres. It has to pass through high-density air, causing bluer light to be scattered. By the time it gets to us, there is little blue light to be seen.