Lecture 5 - Solar Energy to Earth and the Seasons &  Earth’s Modern Atmosphere Flashcards

1
Q

What is the sun?

A

A star located in the Orion Spur of the Sagittarius Arm, which sustains a nuclear fusion reaction at its core to produce radiant energy.

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2
Q

How is solar energy produced?

A

Hydrogen atoms are forced together to produce helium, and energy is released.

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3
Q

What is the importance of solar energy?

A

The ultimate energy source for most life processes in our biosphere.

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4
Q

What is a solar cycle?

A

The periodic variation in the sun’s activity and appearance over time.

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5
Q

Define sunspots.

A

Disturbances on the surface of the Sun caused by magnetic storms.

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6
Q

What are solar minimum and solar maximum?

A

Solar minimum is a period of years with few sun spots, while solar maximum is a period of years when sun spots are numerous.

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7
Q

Define solar flares.

A

Magnetic storms that cause surface explosions and prominence eruptions (outbursts of gasses arcing from the surface), which often occur near sunspots.

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8
Q

What is solar wind?

A

Clouds of electrically charged particles emitted by the sun that surge outward in all directions from the Sun’s surface (corona).

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9
Q

How does the Earth’s magnetic field protect us?

A

It deflects the solar wind toward both of Earth’s poles.

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10
Q

What are coronal mass ejections (CMEs)?

A

Massive outbursts of charged materials that are part of the solar wind.

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11
Q

What is the effect of coronal mass ejections?

A

Create auroras in the upper atmosphere near the poles (Aurora borealis and Aurora Australis).

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12
Q

What are the effects of solar winds on telecommunication systems?

A

Solar winds can disrupt radio broadcasts and satellite transmissions and cause overloads on Earth-based electrical systems.

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13
Q

Define thermopause.

A

The outer boundary of the Earth’s energy system.

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14
Q

Define insolation.

A

The solar radiation that is intercepted by Earth (incoming solar radiation).

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15
Q

Define solar constant.

A

The average insolation received at the thermopause when Earth is at its average distance from the Sun.

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16
Q

Define subsolar point.

A

The point on the earth’s surface where insolation arrives perpendicular to the surface.

17
Q

What are the three things that can happen to solar radiation?

A

Scattering, absorption, and reflection.

18
Q

Define seasonality.

A

1) the seasonal variation of the Sun’s position above the horizon 2) changing day-lengths during the year.

19
Q

What causes seasonal variations?

A

Changes in the sun’s altitude, or angle between the sun and the horizon.

20
Q

Define the sun’s declination.

A

The latitude of the subsolar point, between the Tropic of Cancer and the Tropic of Capricorn.

21
Q

What are the three variations that result in seasons?

A

1) the Sun’s altitude above the horizon, 2) the sun’s declination (latitude of the subsolar point), 3) day-length during the year.

22
Q

Define solstice and equinox.

A

When the sun’s subsolar point is on the Tropic of Cancer or the Tropic of Capricorn, it is the Solstice. When the sun’s subsolar point is on the equator, it is the Equinox, days and nights are of equal length.

23
Q

How does day-length vary?

A

Varies everywhere, except at the equator, which always receives equal hours of day and night and at the poles, which have 6 months of day and 6 months of night.

24
Q

What are the three main aspects of the Earth’s atmosphere?

A

Composition, temperature, and function.

25
Describe the heterosphere.
80 to 480 km altitude, gases occur in distinct layers sorted by gravity according to their atomic weight.
26
Describe the homosphere.
Earth’s surface to 80 km altitude, gases are blended, except for the ozone layer 19 to 50 km above sea level.
27
Describe the troposphere.
Closest to the Earth, supports life, 90% of the total mass of the atmosphere, contains the bulk of all water vapor, clouds, and air pollution.
28
Describe the ionosphere.
Extends from the mesosphere through the thermosphere, absorbs cosmic rays, gamma rays, x-rays, and shorter wavelengths of ultraviolet radiation, changing atoms to positively charged ions, auroras occur here.
29
Describe the ozonosphere.
This “ozone layer” absorbs all UVC rays and some UVB rays, UVA is not absorbed and makes up 95% of all UV radiation reaching the Earth.
30
Define air pollution.
The presence of chemicals or compounds in the air which are usually not present, and which lower the quality of the air and/or cause detrimental changes to the quality of life or the health of humans and other life forms.
31
What are natural sources of air pollution?
Volcanic eruptions, forest fires, dust storms, organic decay.
32
Define persistent organic pollutants (POPs).
PCBs and DDT are examples of POPs.
33
Define transboundary issues.
Related to something happening within one bounded area which adversely affects adjacent areas, causes inter-jurisdictional conflict.
34
How does acid rain form and what are its transboundary effects?
Sulfur dioxide and nitric oxide emissions from one country can be deposited as acidic pollution in another, depending on wind patterns.
35
What are the effects of a thinning ozone layer?
Harm to human health, harm to agriculture, harm to marine life, harm to animals.
36
What is the Montreal Protocol?
An international treaty designed to protect the ozone layer by phasing out the production of numerous substances that are responsible for ozone depletion.
37
What is smog?
A mixture of pollutants that are formed when nitrogen oxides and volatile organic compounds (VOCs) react to sunlight, creating a brown haze above cities.
38
What is an inversion layer?
A reversal of the normal decrease of air temperature with altitude.