Deck 8: The Sun

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سؤال
The layer above the chromosphere is the photosphere.
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سؤال
Sunspots tend to occur in groups, or pairs, with the magnetic field around the pair resembling that around a bar magnet.
سؤال
Nuclear fusion within the Sun proceeds step by step in a series of reactions called the neutron-neutron chain.
سؤال
Spicules can trigger communications blackouts and auroras on Earth.
سؤال
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
سؤال
When the Sun generates its own energy, it uses weak forces to bind together atomic nuclei.
سؤال
Helioseismology maps of rotation in the Sun's interior show that its internal gases rotate with equal periods.
سؤال
The Sun is a ball of hot gas held together by its own gravity.
سؤال
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
سؤال
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
سؤال
The corona is so dim that it is not visible in Earth's daytime sky.
سؤال
The visible surface of the Sun is composed of solid matter.
سؤال
Granulation is caused by convection currents just below the photosphere.
سؤال
Sunspot numbers follow a seven-year cycle.
سؤال
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
سؤال
Nuclear fusion in the Sun is tremendously powerful.
سؤال
What are the dark regions that give the Sun's photosphere a mottled appearance?

A) sunspots
B) spicules
C) granules
D) flares
E) CMEs
سؤال
The upper chromosphere is hot enough to emit X-rays.
سؤال
Almost all the light we receive from the Sun escapes from underneath its photosphere.
سؤال
Sunspots are parts of active solar regions dominated by magnetic fields that encompass all layers of the Sun's atmosphere.
سؤال
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
سؤال
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
سؤال
How many nuclear reactions occur in a proton-proton chain?

A) one
B) two
C) three
D) four
E) five
سؤال
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
سؤال
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
سؤال
What causes granulation on the photosphere?

A) convection
B) solar cycle
C) magnetic fields
D) bursts of energy
E) differential rotation
سؤال
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
سؤال
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.
سؤال
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
سؤال
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
سؤال
<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
سؤال
<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
سؤال
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
سؤال
What methodology do astronomers use to map the inside of the Sun?

A) heliogeology
B) chromography
C) coronagraphy
D) helioseismology
E) magnetic field mapping
سؤال
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
سؤال
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
سؤال
Of the following parts of the Sun, which is the hottest?

A) sunspots
B) corona
C) photosphere
D) supergranules
E) chromosphere
سؤال
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
سؤال
Astronomers refer to the dark center of a sunspot as a(n) ____

A) eye
B) flare
C) umbra
D) spicule
E) penumbra
سؤال
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
سؤال
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
سؤال
Match between columns
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
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
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
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
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
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
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
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
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
سؤال
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?
سؤال
During nuclear fusion, four hydrogen nuclei fuse into how many helium?

A) one
B) two
C) three
D) four
E) eight
سؤال
Explain the role of convection on the Sun's surface.
سؤال
The number of _______________ visible on the Sun varies in a cycle with a period of 11 years.
سؤال
What are the only four forces that can affect matter?
سؤال
Which of the natural forces bind atomic nuclei?

A) strong force
B) weak force
C) gravitational force
D) Newtonian force
E) electromagnetic force
سؤال
Explain the Babcock model and why the solar cycle should really be considered as a 22-year cycle instead of 11-year cycle.
سؤال
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.
سؤال
The _______________ is a thin layer of gas from which Earth receives most of the Sun's light.
سؤال
What occurs during nuclear fusion within the Sun and how much energy is produced?
سؤال
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
سؤال
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
سؤال
The chromosphere is roughly _______________ times fainter than the photosphere.
سؤال
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
سؤال
The most abundant gas making up the Sun's composition is _______________.
سؤال
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.
سؤال
The magnetic polarities of sunspots _______________ at the end of an 11-year cycle.
سؤال
Why do sunspots occur darker than the rest of the Sun's surface?
سؤال
The images produced by _______________ reveal streamers in the corona that follow magnetic lines of force in the Sun's magnetic field.
سؤال
The solar wind extends to the _______________ , marking an outer boundary of the Solar System.
سؤال
How is the Sun's rotation different than that of Earth's?
سؤال
Historical records show that there were very few sunspots from about 1645 to 1715, a phenomenon known as the _______________.
سؤال
Stars, like our Sun, generate their energy by way of nuclear _______________.
سؤال
What is the safest way to view the Sun and its sunspots?
سؤال
The _______________ of the solar disk is dimmer than the center, which is caused by the absorption of light in the photosphere.
سؤال
Gas flows away from the Sun in the _______________, which can be considered an extension of the corona.
سؤال
The _______________ predicts that pairs of sunspots should occur where magnetic tubes burst through the Sun's surface.
سؤال
What causes auroras and where are they most prominent on Earth?
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ملء الشاشة (f)
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Deck 8: The Sun
1
The layer above the chromosphere is the photosphere.
False
2
Sunspots tend to occur in groups, or pairs, with the magnetic field around the pair resembling that around a bar magnet.
True
3
Nuclear fusion within the Sun proceeds step by step in a series of reactions called the neutron-neutron chain.
False
4
Spicules can trigger communications blackouts and auroras on Earth.
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5
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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6
When the Sun generates its own energy, it uses weak forces to bind together atomic nuclei.
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7
Helioseismology maps of rotation in the Sun's interior show that its internal gases rotate with equal periods.
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8
The Sun is a ball of hot gas held together by its own gravity.
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9
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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10
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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11
The corona is so dim that it is not visible in Earth's daytime sky.
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12
The visible surface of the Sun is composed of solid matter.
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13
Granulation is caused by convection currents just below the photosphere.
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14
Sunspot numbers follow a seven-year cycle.
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15
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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16
Nuclear fusion in the Sun is tremendously powerful.
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17
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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18
The upper chromosphere is hot enough to emit X-rays.
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19
Almost all the light we receive from the Sun escapes from underneath its photosphere.
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20
Sunspots are parts of active solar regions dominated by magnetic fields that encompass all layers of the Sun's atmosphere.
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21
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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22
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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23
How many nuclear reactions occur in a proton-proton chain?

A) one
B) two
C) three
D) four
E) five
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24
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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25
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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26
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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27
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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28
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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29
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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30
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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31
<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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32
<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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33
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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34
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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35
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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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
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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38
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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39
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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40
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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41
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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42
Match between columns
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
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
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
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
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
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
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
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
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
spicules
prominences
solar wind
coronal mass ejection
photosphere
sunspots
corona
neutrinos
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43
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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44
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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45
Explain the role of convection on the Sun's surface.
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46
The number of _______________ visible on the Sun varies in a cycle with a period of 11 years.
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47
What are the only four forces that can affect matter?
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48
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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49
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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50
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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51
The _______________ is a thin layer of gas from which Earth receives most of the Sun's light.
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52
What occurs during nuclear fusion within the Sun and how much energy is produced?
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53
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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54
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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55
The chromosphere is roughly _______________ times fainter than the photosphere.
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56
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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57
The most abundant gas making up the Sun's composition is _______________.
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58
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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59
The magnetic polarities of sunspots _______________ at the end of an 11-year cycle.
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60
Why do sunspots occur darker than the rest of the Sun's surface?
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61
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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62
The solar wind extends to the _______________ , marking an outer boundary of the Solar System.
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63
How is the Sun's rotation different than that of Earth's?
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64
Historical records show that there were very few sunspots from about 1645 to 1715, a phenomenon known as the _______________.
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65
Stars, like our Sun, generate their energy by way of nuclear _______________.
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66
What is the safest way to view the Sun and its sunspots?
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67
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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68
Gas flows away from the Sun in the _______________, which can be considered an extension of the corona.
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69
The _______________ predicts that pairs of sunspots should occur where magnetic tubes burst through the Sun's surface.
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70
What causes auroras and where are they most prominent on Earth?
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