Deck 8: The Sun

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Question
The upper chromosphere is hot enough to emit X-rays.
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Question
The visible surface of the Sun is composed of solid matter.
Question
The layer above the chromosphere is the photosphere.
Question
The Sun is a ball of hot gas held together by its own gravity.
Question
Helioseismology maps of rotation in the Sun's interior show that its internal gases rotate with equal periods.
Question
Spicules can trigger communications blackouts and auroras on Earth.
Question
Sunspots are parts of active solar regions dominated by magnetic fields that encompass all layers of the Sun's atmosphere.
Question
Nuclear fusion in the Sun is tremendously powerful.
Question
What is the approximate average temperature of the Sun's surface?

A) 5000 o C
B) 5800oC
C) 5800 K
D) 6400 K
E) 10,000oC
Question
Nuclear fusion within the Sun proceeds step by step in a series of reactions called the neutron-neutron chain.
Question
Sunspots tend to occur in groups, or pairs, with the magnetic field around the pair resembling that around a bar magnet.
Question
Granulation is caused by convection currents just below the photosphere.
Question
What are the dark regions that give the Sun's photosphere a mottled appearance?

A) sunspots
B) spicules
C) granules
D) flares
E) CMEs
Question
Almost all the light we receive from the Sun escapes from underneath its photosphere.
Question
Sunspot numbers follow a seven-year cycle.
Question
The corona is so dim that it is not visible in Earth's daytime sky.
Question
Which two elements are most abundant within the Sun?

A) hydrogen and oxygen
B) hydrogen and helium
C) helium and carbon
D) helium and nitrogen
E) hydrogen and carbon
Question
Which is the correct order of the Sun's atmospheric layers, from the innermost to outermost?

A) chromosphere → corona → photosphere
B) corona → chromosphere → photosphere
C) chromosphere → photosphere → corona
D) photosphere → chromosphere → corona
E) photosphere → corona → chromosphere
Question
What is the average distance between the Sun and Earth?

A) 1 AU
B) 2 AU
C) 5 AU
D) 10 AU
E) 20 AU
Question
When the Sun generates its own energy, it uses weak forces to bind together atomic nuclei.
Question
Astronomers often record solar images in the ____ part of the electromagnetic spectrum because the gaseous layers high in the Sun's atmosphere are very hot and emit most of their light at short wavelengths.

A) visible light
B) microwave
C) ultraviolet
D) gamma
E) infrared
Question
The corona can reach temperatures of up to ____.

A) 5800 K
B) 10,000 K
C) 500,000 K
D) 1,000,000 K
E) 2,000,000 K
Question
Why does the temperature of the corona rise with latitude?

A) Atoms within the corona become more ionized at higher altitudes.
B) Atoms are forced upward from the chromosphere to the corona.
C) Atoms become neutralized as they dissipate in higher altitudes.
D) Atoms undergo fission when repelled by the corona.
E) Atoms are less excited as they move from the photosphere to the corona.
Question
How many nuclear reactions occur in a proton-proton chain?

A) one
B) two
C) three
D) four
E) five
Question
The pink color of the chromosphere is produced by the combined light of three emission lines of hydrogen: ____.

A) blue, green, and yellow
B) red, blue, and violet
C) green, blue, and violet
D) red, magenta, and violet
E) indigo, blue, and red
Question
Consider the complete magnetic cycle of sunspot activity on the Sun. Approximately how many years is this cycle?

A) 7 years
B) 11 years
C) 22 years
D) 40 years
E) 100 years
Question
When mapping the interior of the Sun, astronomers must measure _____ as the photosphere moves up and down.

A) sunspots
B) magnetic fields
C) supergranules
D) limb darkening
E) Doppler shifts
Question
What causes granulation on the photosphere?

A) convection
B) solar cycle
C) magnetic fields
D) bursts of energy
E) differential rotation
Question
Galileo proposed that the Sun is a rotating sphere after he ____.

A) timed a full rotation of the Sun's equator
B) observed sunspots move across the surface of the Sun
C) measured different spectral lines of emission on different days
D) noted how the Sun rose in the east and set in the west
E) discovered the parallax of the Sun
Question
<strong>  Figure 8-1b Which layer of the Sun's atmosphere is represented in the accompanying visual-wavelength image?</strong> A) magnetic carpet B) chromosphere C) heliosphere D) solar wind E) corona <div style=padding-top: 35px> Figure 8-1b
Which layer of the Sun's atmosphere is represented in the accompanying visual-wavelength image?

A) magnetic carpet
B) chromosphere
C) heliosphere
D) solar wind
E) corona
Question
The Babcock model of the solar magnetic cycle explains the sunspot cycle as primarily a consequence of the Sun's ____.

A) meridional flow
B) convection currents
C) differential rotation
D) coronal mass ejections
E) helioseimologic activity
Question
The _____ occurs when some of the energy in the convective motion of gas is converted into magnetic field energy.

A) Zeeman effect
B) Maunder minimum
C) meridional flow
D) dynamo effect
E) reconnection event
Question
What methodology do astronomers use to map the inside of the Sun?

A) heliogeology
B) chromography
C) coronagraphy
D) helioseismology
E) magnetic field mapping
Question
What occurs on the surface of the Sun during a solar cycle minimum?

A) reversal in rotation of the Sun
B) little to no sunspot activity
C) decreased temperature of the photosphere
D) partial dissipation of the corona
E) little to no solar wind
Question
<strong>  Figure 8-2b What process on the Sun's photosphere does this figure represent?</strong> A) solar cycle B) sunspot cycle C) convection currents D) magnetic field shifts E) differential rotation <div style=padding-top: 35px> Figure 8-2b
What process on the Sun's photosphere does this figure represent?

A) solar cycle
B) sunspot cycle
C) convection currents
D) magnetic field shifts
E) differential rotation
Question
Granulation is evidence that energy in the photosphere ____.

A) is flowing downward towards the core
B) stays horizontal on the surface
C) is spiraling westward
D) is spiraling eastward
E) is flowing upward
Question
When two arches in a magnetic field encounter each other, ____ can cause powerful eruptions called ____.

A) reconnection events; flares
B) supergranules; Coulumb barriers
C) filaments; coronal holes
D) solar winds; convective zones
E) prominences; limb darkening
Question
Of the following parts of the Sun, which is the hottest?

A) sunspots
B) corona
C) photosphere
D) supergranules
E) chromosphere
Question
Astronomers can measure the magnetic fields of sunspots using the ____, which splits spectral lines into multiple components.

A) Zeeman effect
B) Maunder effect
C) Babcock effect
D) Galileo effect
E) Payne effect
Question
Astronomers refer to the dark center of a sunspot as a(n) ____

A) eye
B) flare
C) umbra
D) spicule
E) penumbra
Question
Match between columns
Subatomic particles released from the proton-proton chain of nuclear fusion
coronal mass ejection
Subatomic particles released from the proton-proton chain of nuclear fusion
photosphere
Subatomic particles released from the proton-proton chain of nuclear fusion
sunspots
Subatomic particles released from the proton-proton chain of nuclear fusion
spicules
Subatomic particles released from the proton-proton chain of nuclear fusion
solar wind
Subatomic particles released from the proton-proton chain of nuclear fusion
corona
Subatomic particles released from the proton-proton chain of nuclear fusion
prominences
Subatomic particles released from the proton-proton chain of nuclear fusion
neutrinos
Question
Which equation represents the overall nuclear fusion process of the Sun?

A) "4 4 H => 4 He - energy"
B) "2 1 H => 1 He + energy"
C) "4 1 H => 2 1 He - energy"
D) "4 1 H => 4 He + energy"
E) " 4 H => 8 He + energy"
Question
Match between columns
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
photosphere
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
spicules
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
solar wind
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
corona
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
prominences
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
neutrinos
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
coronal mass ejection
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
sunspots
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
photosphere
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
spicules
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
solar wind
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
corona
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
prominences
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
neutrinos
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
coronal mass ejection
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
sunspots
Arches of magnetic field visible in the chromosphere and corona
photosphere
Arches of magnetic field visible in the chromosphere and corona
spicules
Arches of magnetic field visible in the chromosphere and corona
solar wind
Arches of magnetic field visible in the chromosphere and corona
corona
Arches of magnetic field visible in the chromosphere and corona
prominences
Arches of magnetic field visible in the chromosphere and corona
neutrinos
Arches of magnetic field visible in the chromosphere and corona
coronal mass ejection
Arches of magnetic field visible in the chromosphere and corona
sunspots
Question
Why was the Davis experiment only able to detect one-third of the neutrinos originally predicted?

A) Most of the neutrinos were absorbed by Earth's atmosphere.
B) The neutrinos combined with other particles as they entered Earth's atmosphere.
C) The neutrinos distributed evenly among three different flavors while traveling to Earth.
D) The number of neutrinos was too great to be held in the tank that Davis designed.
E) The other two-thirds of neutrinos dissipated while traveling to Earth.
Question
During the first reaction of the proton-proton chain of nuclear fusion, a weak force causes one of the protons to transform into a neutron and emit ____.

A) a positron and a neutrino
B) a positron and a deuterium
C) a neutrino and a deuterium
D) a neutrino and an electron
E) a deuterium and an electron
Question
Match between columns
Subatomic particles released from the proton-proton chain of nuclear fusion
spicules
Subatomic particles released from the proton-proton chain of nuclear fusion
prominences
Subatomic particles released from the proton-proton chain of nuclear fusion
solar wind
Subatomic particles released from the proton-proton chain of nuclear fusion
coronal mass ejection
Subatomic particles released from the proton-proton chain of nuclear fusion
photosphere
Subatomic particles released from the proton-proton chain of nuclear fusion
sunspots
Subatomic particles released from the proton-proton chain of nuclear fusion
corona
Subatomic particles released from the proton-proton chain of nuclear fusion
neutrinos
The outermost part of the Sun's atmosphere
spicules
The outermost part of the Sun's atmosphere
prominences
The outermost part of the Sun's atmosphere
solar wind
The outermost part of the Sun's atmosphere
coronal mass ejection
The outermost part of the Sun's atmosphere
photosphere
The outermost part of the Sun's atmosphere
sunspots
The outermost part of the Sun's atmosphere
corona
The outermost part of the Sun's atmosphere
neutrinos
Flame-like structures that extend upward into the lower corona
spicules
Flame-like structures that extend upward into the lower corona
prominences
Flame-like structures that extend upward into the lower corona
solar wind
Flame-like structures that extend upward into the lower corona
coronal mass ejection
Flame-like structures that extend upward into the lower corona
photosphere
Flame-like structures that extend upward into the lower corona
sunspots
Flame-like structures that extend upward into the lower corona
corona
Flame-like structures that extend upward into the lower corona
neutrinos
Arches of magnetic field visible in the chromosphere and corona
spicules
Arches of magnetic field visible in the chromosphere and corona
prominences
Arches of magnetic field visible in the chromosphere and corona
solar wind
Arches of magnetic field visible in the chromosphere and corona
coronal mass ejection
Arches of magnetic field visible in the chromosphere and corona
photosphere
Arches of magnetic field visible in the chromosphere and corona
sunspots
Arches of magnetic field visible in the chromosphere and corona
corona
Arches of magnetic field visible in the chromosphere and corona
neutrinos
A breeze of low-density ionized gas streaming away from the Sun
spicules
A breeze of low-density ionized gas streaming away from the Sun
prominences
A breeze of low-density ionized gas streaming away from the Sun
solar wind
A breeze of low-density ionized gas streaming away from the Sun
coronal mass ejection
A breeze of low-density ionized gas streaming away from the Sun
photosphere
A breeze of low-density ionized gas streaming away from the Sun
sunspots
A breeze of low-density ionized gas streaming away from the Sun
corona
A breeze of low-density ionized gas streaming away from the Sun
neutrinos
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
spicules
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
prominences
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
solar wind
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
coronal mass ejection
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
photosphere
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
sunspots
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
corona
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
neutrinos
The layer in the Sun from which visible photons most easily escape
spicules
The layer in the Sun from which visible photons most easily escape
prominences
The layer in the Sun from which visible photons most easily escape
solar wind
The layer in the Sun from which visible photons most easily escape
coronal mass ejection
The layer in the Sun from which visible photons most easily escape
photosphere
The layer in the Sun from which visible photons most easily escape
sunspots
The layer in the Sun from which visible photons most easily escape
corona
The layer in the Sun from which visible photons most easily escape
neutrinos
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
spicules
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
prominences
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
solar wind
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
coronal mass ejection
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
photosphere
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
sunspots
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
corona
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
neutrinos
Question
Which of the natural forces bind atomic nuclei?

A) strong force
B) weak force
C) gravitational force
D) Newtonian force
E) electromagnetic force
Question
The Maunder minimum occurred in the 17th century, which many scientists debate the labeling of that time as the "Little Ice Age". However, it occurred before the Industrial Revolution and thus, had no significant impact on the human standard of living as we know in today's society. Suppose the Sun experienced a similar period today. How would life on Earth be impacted?
Question
The images produced by _______________ reveal streamers in the corona that follow magnetic lines of force in the Sun's magnetic field.
Question
What occurs during nuclear fusion within the Sun and how much energy is produced?
Question
The number of _______________ visible on the Sun varies in a cycle with a period of 11 years.
Question
Why do sunspots occur darker than the rest of the Sun's surface?
Question
During nuclear fusion, four hydrogen nuclei fuse into how many helium?

A) one
B) two
C) three
D) four
E) eight
Question
The _______________ is a thin layer of gas from which Earth receives most of the Sun's light.
Question
The solar wind extends to the _______________ , marking an outer boundary of the Solar System.
Question
What is released from the proton-proton chain and is immediately absorbed by the surrounding gas, thereby heating it?

A) positrons
B) deuterium
C) gamma rays
D) neutrinos
E) electron motion
Question
The most abundant gas making up the Sun's composition is _______________.
Question
In order for nuclear fusion to occur, atomic nuclei must overcome the ____ by colliding violently.

A) coronal hole
B) dynamo effect
C) convective zone
D) radiative zone
E) Coulomb barrier
Question
What is the safest way to view the Sun and its sunspots?
Question
Stars, like our Sun, generate their energy by way of nuclear _______________.
Question
Explain the role of convection on the Sun's surface.
Question
What causes auroras and where are they most prominent on Earth?
Question
What forms of electromagnetic radiation from the Sun's emissions do we experience here on Earth? Illustrate how we know this to be the case with one practical example for each form.
Question
The _______________ of the solar disk is dimmer than the center, which is caused by the absorption of light in the photosphere.
Question
Gas flows away from the Sun in the _______________, which can be considered an extension of the corona.
Question
The magnetic polarities of sunspots _______________ at the end of an 11-year cycle.
Question
Explain the Babcock model and why the solar cycle should really be considered as a 22-year cycle instead of 11-year cycle.
Question
The _______________ predicts that pairs of sunspots should occur where magnetic tubes burst through the Sun's surface.
Question
Historical records show that there were very few sunspots from about 1645 to 1715, a phenomenon known as the _______________.
Question
The chromosphere is roughly _______________ times fainter than the photosphere.
Question
What are the only four forces that can affect matter?
Question
How is the Sun's rotation different than that of Earth's?
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Deck 8: The Sun
1
The upper chromosphere is hot enough to emit X-rays.
True
2
The visible surface of the Sun is composed of solid matter.
False
3
The layer above the chromosphere is the photosphere.
False
4
The Sun is a ball of hot gas held together by its own gravity.
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5
Helioseismology maps of rotation in the Sun's interior show that its internal gases rotate with equal periods.
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6
Spicules can trigger communications blackouts and auroras on Earth.
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7
Sunspots are parts of active solar regions dominated by magnetic fields that encompass all layers of the Sun's atmosphere.
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8
Nuclear fusion in the Sun is tremendously powerful.
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9
What is the approximate average temperature of the Sun's surface?

A) 5000 o C
B) 5800oC
C) 5800 K
D) 6400 K
E) 10,000oC
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10
Nuclear fusion within the Sun proceeds step by step in a series of reactions called the neutron-neutron chain.
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11
Sunspots tend to occur in groups, or pairs, with the magnetic field around the pair resembling that around a bar magnet.
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12
Granulation is caused by convection currents just below the photosphere.
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13
What are the dark regions that give the Sun's photosphere a mottled appearance?

A) sunspots
B) spicules
C) granules
D) flares
E) CMEs
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14
Almost all the light we receive from the Sun escapes from underneath its photosphere.
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15
Sunspot numbers follow a seven-year cycle.
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16
The corona is so dim that it is not visible in Earth's daytime sky.
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17
Which two elements are most abundant within the Sun?

A) hydrogen and oxygen
B) hydrogen and helium
C) helium and carbon
D) helium and nitrogen
E) hydrogen and carbon
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18
Which is the correct order of the Sun's atmospheric layers, from the innermost to outermost?

A) chromosphere → corona → photosphere
B) corona → chromosphere → photosphere
C) chromosphere → photosphere → corona
D) photosphere → chromosphere → corona
E) photosphere → corona → chromosphere
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19
What is the average distance between the Sun and Earth?

A) 1 AU
B) 2 AU
C) 5 AU
D) 10 AU
E) 20 AU
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20
When the Sun generates its own energy, it uses weak forces to bind together atomic nuclei.
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21
Astronomers often record solar images in the ____ part of the electromagnetic spectrum because the gaseous layers high in the Sun's atmosphere are very hot and emit most of their light at short wavelengths.

A) visible light
B) microwave
C) ultraviolet
D) gamma
E) infrared
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22
The corona can reach temperatures of up to ____.

A) 5800 K
B) 10,000 K
C) 500,000 K
D) 1,000,000 K
E) 2,000,000 K
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23
Why does the temperature of the corona rise with latitude?

A) Atoms within the corona become more ionized at higher altitudes.
B) Atoms are forced upward from the chromosphere to the corona.
C) Atoms become neutralized as they dissipate in higher altitudes.
D) Atoms undergo fission when repelled by the corona.
E) Atoms are less excited as they move from the photosphere to the corona.
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24
How many nuclear reactions occur in a proton-proton chain?

A) one
B) two
C) three
D) four
E) five
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25
The pink color of the chromosphere is produced by the combined light of three emission lines of hydrogen: ____.

A) blue, green, and yellow
B) red, blue, and violet
C) green, blue, and violet
D) red, magenta, and violet
E) indigo, blue, and red
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26
Consider the complete magnetic cycle of sunspot activity on the Sun. Approximately how many years is this cycle?

A) 7 years
B) 11 years
C) 22 years
D) 40 years
E) 100 years
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27
When mapping the interior of the Sun, astronomers must measure _____ as the photosphere moves up and down.

A) sunspots
B) magnetic fields
C) supergranules
D) limb darkening
E) Doppler shifts
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28
What causes granulation on the photosphere?

A) convection
B) solar cycle
C) magnetic fields
D) bursts of energy
E) differential rotation
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29
Galileo proposed that the Sun is a rotating sphere after he ____.

A) timed a full rotation of the Sun's equator
B) observed sunspots move across the surface of the Sun
C) measured different spectral lines of emission on different days
D) noted how the Sun rose in the east and set in the west
E) discovered the parallax of the Sun
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30
<strong>  Figure 8-1b Which layer of the Sun's atmosphere is represented in the accompanying visual-wavelength image?</strong> A) magnetic carpet B) chromosphere C) heliosphere D) solar wind E) corona Figure 8-1b
Which layer of the Sun's atmosphere is represented in the accompanying visual-wavelength image?

A) magnetic carpet
B) chromosphere
C) heliosphere
D) solar wind
E) corona
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31
The Babcock model of the solar magnetic cycle explains the sunspot cycle as primarily a consequence of the Sun's ____.

A) meridional flow
B) convection currents
C) differential rotation
D) coronal mass ejections
E) helioseimologic activity
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32
The _____ occurs when some of the energy in the convective motion of gas is converted into magnetic field energy.

A) Zeeman effect
B) Maunder minimum
C) meridional flow
D) dynamo effect
E) reconnection event
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33
What methodology do astronomers use to map the inside of the Sun?

A) heliogeology
B) chromography
C) coronagraphy
D) helioseismology
E) magnetic field mapping
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34
What occurs on the surface of the Sun during a solar cycle minimum?

A) reversal in rotation of the Sun
B) little to no sunspot activity
C) decreased temperature of the photosphere
D) partial dissipation of the corona
E) little to no solar wind
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35
<strong>  Figure 8-2b What process on the Sun's photosphere does this figure represent?</strong> A) solar cycle B) sunspot cycle C) convection currents D) magnetic field shifts E) differential rotation Figure 8-2b
What process on the Sun's photosphere does this figure represent?

A) solar cycle
B) sunspot cycle
C) convection currents
D) magnetic field shifts
E) differential rotation
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36
Granulation is evidence that energy in the photosphere ____.

A) is flowing downward towards the core
B) stays horizontal on the surface
C) is spiraling westward
D) is spiraling eastward
E) is flowing upward
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37
When two arches in a magnetic field encounter each other, ____ can cause powerful eruptions called ____.

A) reconnection events; flares
B) supergranules; Coulumb barriers
C) filaments; coronal holes
D) solar winds; convective zones
E) prominences; limb darkening
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38
Of the following parts of the Sun, which is the hottest?

A) sunspots
B) corona
C) photosphere
D) supergranules
E) chromosphere
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39
Astronomers can measure the magnetic fields of sunspots using the ____, which splits spectral lines into multiple components.

A) Zeeman effect
B) Maunder effect
C) Babcock effect
D) Galileo effect
E) Payne effect
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40
Astronomers refer to the dark center of a sunspot as a(n) ____

A) eye
B) flare
C) umbra
D) spicule
E) penumbra
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41
Match between columns
Subatomic particles released from the proton-proton chain of nuclear fusion
coronal mass ejection
Subatomic particles released from the proton-proton chain of nuclear fusion
photosphere
Subatomic particles released from the proton-proton chain of nuclear fusion
sunspots
Subatomic particles released from the proton-proton chain of nuclear fusion
spicules
Subatomic particles released from the proton-proton chain of nuclear fusion
solar wind
Subatomic particles released from the proton-proton chain of nuclear fusion
corona
Subatomic particles released from the proton-proton chain of nuclear fusion
prominences
Subatomic particles released from the proton-proton chain of nuclear fusion
neutrinos
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42
Which equation represents the overall nuclear fusion process of the Sun?

A) "4 4 H => 4 He - energy"
B) "2 1 H => 1 He + energy"
C) "4 1 H => 2 1 He - energy"
D) "4 1 H => 4 He + energy"
E) " 4 H => 8 He + energy"
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43
Match between columns
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
photosphere
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
spicules
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
solar wind
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
corona
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
prominences
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
neutrinos
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
coronal mass ejection
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
sunspots
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
photosphere
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
spicules
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
solar wind
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
corona
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
prominences
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
neutrinos
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
coronal mass ejection
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
sunspots
Arches of magnetic field visible in the chromosphere and corona
photosphere
Arches of magnetic field visible in the chromosphere and corona
spicules
Arches of magnetic field visible in the chromosphere and corona
solar wind
Arches of magnetic field visible in the chromosphere and corona
corona
Arches of magnetic field visible in the chromosphere and corona
prominences
Arches of magnetic field visible in the chromosphere and corona
neutrinos
Arches of magnetic field visible in the chromosphere and corona
coronal mass ejection
Arches of magnetic field visible in the chromosphere and corona
sunspots
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44
Why was the Davis experiment only able to detect one-third of the neutrinos originally predicted?

A) Most of the neutrinos were absorbed by Earth's atmosphere.
B) The neutrinos combined with other particles as they entered Earth's atmosphere.
C) The neutrinos distributed evenly among three different flavors while traveling to Earth.
D) The number of neutrinos was too great to be held in the tank that Davis designed.
E) The other two-thirds of neutrinos dissipated while traveling to Earth.
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45
During the first reaction of the proton-proton chain of nuclear fusion, a weak force causes one of the protons to transform into a neutron and emit ____.

A) a positron and a neutrino
B) a positron and a deuterium
C) a neutrino and a deuterium
D) a neutrino and an electron
E) a deuterium and an electron
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46
Match between columns
Subatomic particles released from the proton-proton chain of nuclear fusion
spicules
Subatomic particles released from the proton-proton chain of nuclear fusion
prominences
Subatomic particles released from the proton-proton chain of nuclear fusion
solar wind
Subatomic particles released from the proton-proton chain of nuclear fusion
coronal mass ejection
Subatomic particles released from the proton-proton chain of nuclear fusion
photosphere
Subatomic particles released from the proton-proton chain of nuclear fusion
sunspots
Subatomic particles released from the proton-proton chain of nuclear fusion
corona
Subatomic particles released from the proton-proton chain of nuclear fusion
neutrinos
The outermost part of the Sun's atmosphere
spicules
The outermost part of the Sun's atmosphere
prominences
The outermost part of the Sun's atmosphere
solar wind
The outermost part of the Sun's atmosphere
coronal mass ejection
The outermost part of the Sun's atmosphere
photosphere
The outermost part of the Sun's atmosphere
sunspots
The outermost part of the Sun's atmosphere
corona
The outermost part of the Sun's atmosphere
neutrinos
Flame-like structures that extend upward into the lower corona
spicules
Flame-like structures that extend upward into the lower corona
prominences
Flame-like structures that extend upward into the lower corona
solar wind
Flame-like structures that extend upward into the lower corona
coronal mass ejection
Flame-like structures that extend upward into the lower corona
photosphere
Flame-like structures that extend upward into the lower corona
sunspots
Flame-like structures that extend upward into the lower corona
corona
Flame-like structures that extend upward into the lower corona
neutrinos
Arches of magnetic field visible in the chromosphere and corona
spicules
Arches of magnetic field visible in the chromosphere and corona
prominences
Arches of magnetic field visible in the chromosphere and corona
solar wind
Arches of magnetic field visible in the chromosphere and corona
coronal mass ejection
Arches of magnetic field visible in the chromosphere and corona
photosphere
Arches of magnetic field visible in the chromosphere and corona
sunspots
Arches of magnetic field visible in the chromosphere and corona
corona
Arches of magnetic field visible in the chromosphere and corona
neutrinos
A breeze of low-density ionized gas streaming away from the Sun
spicules
A breeze of low-density ionized gas streaming away from the Sun
prominences
A breeze of low-density ionized gas streaming away from the Sun
solar wind
A breeze of low-density ionized gas streaming away from the Sun
coronal mass ejection
A breeze of low-density ionized gas streaming away from the Sun
photosphere
A breeze of low-density ionized gas streaming away from the Sun
sunspots
A breeze of low-density ionized gas streaming away from the Sun
corona
A breeze of low-density ionized gas streaming away from the Sun
neutrinos
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
spicules
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
prominences
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
solar wind
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
coronal mass ejection
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
photosphere
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
sunspots
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
corona
Violent bursts of ionized gas ejected from magnetic fields that flow outward in the solar wind
neutrinos
The layer in the Sun from which visible photons most easily escape
spicules
The layer in the Sun from which visible photons most easily escape
prominences
The layer in the Sun from which visible photons most easily escape
solar wind
The layer in the Sun from which visible photons most easily escape
coronal mass ejection
The layer in the Sun from which visible photons most easily escape
photosphere
The layer in the Sun from which visible photons most easily escape
sunspots
The layer in the Sun from which visible photons most easily escape
corona
The layer in the Sun from which visible photons most easily escape
neutrinos
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
spicules
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
prominences
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
solar wind
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
coronal mass ejection
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
photosphere
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
sunspots
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
corona
Cool, relatively dark spots on the Sun's photosphere, usually appearing in group
neutrinos
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47
Which of the natural forces bind atomic nuclei?

A) strong force
B) weak force
C) gravitational force
D) Newtonian force
E) electromagnetic force
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48
The Maunder minimum occurred in the 17th century, which many scientists debate the labeling of that time as the "Little Ice Age". However, it occurred before the Industrial Revolution and thus, had no significant impact on the human standard of living as we know in today's society. Suppose the Sun experienced a similar period today. How would life on Earth be impacted?
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49
The images produced by _______________ reveal streamers in the corona that follow magnetic lines of force in the Sun's magnetic field.
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50
What occurs during nuclear fusion within the Sun and how much energy is produced?
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51
The number of _______________ visible on the Sun varies in a cycle with a period of 11 years.
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52
Why do sunspots occur darker than the rest of the Sun's surface?
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53
During nuclear fusion, four hydrogen nuclei fuse into how many helium?

A) one
B) two
C) three
D) four
E) eight
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54
The _______________ is a thin layer of gas from which Earth receives most of the Sun's light.
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55
The solar wind extends to the _______________ , marking an outer boundary of the Solar System.
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56
What is released from the proton-proton chain and is immediately absorbed by the surrounding gas, thereby heating it?

A) positrons
B) deuterium
C) gamma rays
D) neutrinos
E) electron motion
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57
The most abundant gas making up the Sun's composition is _______________.
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58
In order for nuclear fusion to occur, atomic nuclei must overcome the ____ by colliding violently.

A) coronal hole
B) dynamo effect
C) convective zone
D) radiative zone
E) Coulomb barrier
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59
What is the safest way to view the Sun and its sunspots?
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60
Stars, like our Sun, generate their energy by way of nuclear _______________.
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61
Explain the role of convection on the Sun's surface.
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62
What causes auroras and where are they most prominent on Earth?
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63
What forms of electromagnetic radiation from the Sun's emissions do we experience here on Earth? Illustrate how we know this to be the case with one practical example for each form.
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64
The _______________ of the solar disk is dimmer than the center, which is caused by the absorption of light in the photosphere.
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65
Gas flows away from the Sun in the _______________, which can be considered an extension of the corona.
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66
The magnetic polarities of sunspots _______________ at the end of an 11-year cycle.
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67
Explain the Babcock model and why the solar cycle should really be considered as a 22-year cycle instead of 11-year cycle.
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68
The _______________ predicts that pairs of sunspots should occur where magnetic tubes burst through the Sun's surface.
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69
Historical records show that there were very few sunspots from about 1645 to 1715, a phenomenon known as the _______________.
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70
The chromosphere is roughly _______________ times fainter than the photosphere.
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71
What are the only four forces that can affect matter?
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72
How is the Sun's rotation different than that of Earth's?
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