What year was the study by Love et al. published?
2022.
What is the umbra?
The fully shaded inner region of a shadow.
1/159
p.11
太空天氣對地球的影響

What year was the study by Love et al. published?

2022.

p.31
太陽的結構與組成

What is the umbra?

The fully shaded inner region of a shadow.

p.4
太空天氣對地球的影響

What does NOAA/SWPC stand for?

National Oceanic and Atmospheric Administration / Space Weather Prediction Center.

p.6
太空天氣對地球的影響

What does NOAA stand for?

National Oceanic and Atmospheric Administration.

p.20
核融合反應與能量產生

What is the primary process occurring in the CNO Cycle?

Nuclear fusion of hydrogen into helium.

p.22
日震學與太陽內部結構

What is the temperature at the visible surface of the Sun?

5800 K.

p.13
太陽的結構與組成

What is the visible surface of the Sun called?

Photosphere.

p.10
太空天氣對地球的影響

What does GIC stand for?

Geomagnetically Induced Current.

p.11
太空天氣對地球的影響

Who conducted the study referenced in the credit?

Love et al.

p.7
太空天氣對地球的影響

What is the primary focus of Chancellor et al. (2021)?

The specific focus is not provided in the text.

p.29
太陽黑子與磁場

What is the observed tilt of sunspot groups attributed to?

The leading sunspot being closer to the equator than the trailing sunspot.

p.6
太空天氣對地球的影響

What does NCEI stand for?

National Centers for Environmental Information.

p.16
核融合反應與能量產生

What is the energy source of the Sun?

Nuclear fusion in the core.

p.16
核融合反應與能量產生

What is the process of hydrogen fusion summarized as?

4 hydrogen nuclei → 1 helium nucleus + energy + 2 neutrinos.

p.31
太陽的結構與組成

What is the penumbra?

The partially shaded outer region of a shadow.

p.12
日震學與太陽內部結構

Why is multiwavelength observation important in astrophysics?

It provides a more comprehensive understanding of celestial phenomena.

p.20
核融合反應與能量產生

Which elements are involved in the CNO Cycle?

Carbon, nitrogen, and oxygen.

p.25
太陽大氣層與光球層

What is the temperature range of the Corona in Kelvin?

10^6 to 10^7 K.

p.13
太陽的結構與組成

What layer lies just above the photosphere?

Chromosphere.

p.28
太陽黑子與磁場

What is the average magnetic field strength of the Earth?

Approximately 0.5 Gauss.

p.15
太陽的結構與組成

What is the primary chemical composition of the photosphere by mass?

Hydrogen: 73.46%, Helium: 24.85%, Oxygen: 0.77%, Carbon: 0.29%, Iron: 0.16%.

p.15
太陽的結構與組成

What is the density of the Sun's interior (center)?

160,000 kg/m³.

p.14
太陽的結構與組成

What is the radius of the Sun in meters?

6.955 x 10^8 m.

p.19
核融合反應與能量產生

What is produced in the second reaction of the PP Chain?

2 H + 1 H → 3 He + γ.

p.14
太陽的結構與組成

What is the mean density of the Sun?

1.409 g/cm^3.

p.3
太空天氣對地球的影響

What does NOAA/SWPC stand for?

National Oceanic and Atmospheric Administration / Space Weather Prediction Center.

p.12
日震學與太陽內部結構

What does multiwavelength observation refer to?

The study of astronomical objects using different wavelengths of light.

p.6
太空天氣對地球的影響

What does GOES refer to?

Geostationary Operational Environmental Satellites.

p.31
太陽的結構與組成

What is the temperature difference between the center of a granule and its surroundings?

The center is about 300 K hotter than the surroundings.

p.21
太陽的結構與組成

How does energy escape from the radiation zone?

In the form of radiation, primarily gamma rays.

p.28
太陽黑子與磁場

Who discovered the strong magnetic fields near sunspots?

George Ellery Hale in 1908.

p.28
太陽黑子與磁場

How much stronger is the magnetic field near sunspots compared to the average solar magnetic field?

About 1000 times stronger.

p.21
太陽的結構與組成

What is the density change in the radiation zone?

From 20 g/cm³ to 0.2 g/cm³.

p.27
太陽黑子與磁場

What is the temperature at the center of a sunspot?

Approximately 4000 K.

p.27
太陽黑子與磁場

What is the strength of the magnetic field in sunspots compared to the average solar surface?

It is several hundred times stronger.

p.27
太陽黑子與磁場

What is the range of magnetic field strength in the umbra of a sunspot?

Between 1000 to 4000 Gauss.

p.18
核融合反應與能量產生

What percentage of collisions result in nuclear fusion?

Only a small percentage.

p.24
日震學與太陽內部結構

How do scientists infer the Sun's internal structure?

By analyzing seismic waves that reach the surface during solar vibrations.

p.14
太陽的結構與組成

What is the mean distance from the Earth to the Sun?

1 AU (1.496 x 10^8 km).

p.2
地球磁層與磁暴

What are Enhanced Ionospheric Currents?

Increased currents in the ionosphere caused by solar activity.

p.8
太空天氣對地球的影響

What is the primary focus of the study by Nwankwo et al. (2020)?

The specific focus is not provided in the content.

p.23
太陽的自轉與差動自轉

How long does it take for the Sun to rotate at the equator?

Approximately 25 days.

p.12
日震學與太陽內部結構

What types of telescopes are used in multiwavelength observations?

Telescopes that detect various wavelengths, including radio, infrared, visible, ultraviolet, and X-rays.

p.28
太陽黑子與磁場

What causes the lower temperature in sunspot regions?

The magnetic field suppresses energy transfer from the convective layers below the photosphere.

p.22
日震學與太陽內部結構

What phenomenon occurs in the plasma of the convective zone?

Differential rotation.

p.21
太陽的結構與組成

How long does it take for photons to pass through the radiation zone?

About one million years.

p.16
核融合反應與能量產生

What equation represents the energy-mass equivalence in nuclear fusion?

ΔE = (Δm) c^2.

p.18
核融合反應與能量產生

What are the main processes of hydrogen nuclear fusion?

Proton-proton chain and CNO cycle.

p.17
核融合反應與能量產生

What energy is released from one hydrogen fusion reaction?

4.3 x 10^-12 J.

p.18
核融合反應與能量產生

How many fusion reactions does the Sun need to perform every second?

10^38 reactions.

p.26
太陽輻射與輻射層

What type of radiation does the spectrum from the Sun resemble?

Black body radiation at 5800 K.

p.14
太陽的結構與組成

What is the luminosity of the Sun?

3.86 x 10^33 erg/s (or 3.86 x 10^26 W).

p.15
太陽的結構與組成

What is the density of the photosphere?

10⁻⁶ kg/m³.

p.2
太陽輻射與輻射層

What is Solar Cell Degradation?

The reduction in efficiency of solar cells due to radiation exposure.

p.5
太空天氣對地球的影響

What does NOAA/SWPC stand for?

National Oceanic and Atmospheric Administration / Space Weather Prediction Center.

p.13
太陽的結構與組成

What is the outermost layer of the Sun called?

Corona.

p.30
太陽黑子與磁場

What is the relationship between the polarity of leading sunspots in the Northern and Southern Hemispheres during the same solar cycle?

The polarity of leading sunspots in the Northern Hemisphere is opposite to that in the Southern Hemisphere.

p.20
核融合反應與能量產生

In which type of stars does the CNO Cycle primarily occur?

In more massive stars.

p.25
太陽大氣層與光球層

What is the electron density in the Corona?

Approximately 10^1 to 10^2 cm^-3.

p.17
核融合反應與能量產生

What is the mass of one helium nucleus?

6.645 x 10^-27 kg.

p.17
核融合反應與能量產生

How many hydrogen fusion reactions are needed per second to sustain the Sun's energy?

Approximately 10^38 reactions.

p.17
核融合反應與能量產生

How much mass is converted to energy per second in the Sun?

About 5 million tons.

p.15
太陽的結構與組成

What is the typical temperature of a sunspot's umbra?

4240 K.

p.26
太陽黑子與磁場

What phenomena are primarily observed in the photosphere?

Sunspots and granulation.

p.2
太陽風暴與太陽風

What are Coronal Mass Ejections?

Large expulsions of plasma and magnetic field from the Sun's corona.

p.14
太陽輻射與輻射層

How long does light take to travel from the Sun to the Earth?

8.32 minutes.

p.10
太空天氣對地球的影響

Which organization is credited with information about GIC?

NASA and GAO.

p.10
太空天氣對地球的影響

What is the primary effect of geomagnetically induced currents?

They can affect electrical systems and infrastructure.

p.4
日震學與太陽內部結構

What does NASA/SDO stand for?

National Aeronautics and Space Administration / Solar Dynamics Observatory.

p.13
太陽的結構與組成

Which layer of the Sun is responsible for the majority of its energy production?

Core.

p.23
太陽的自轉與差動自轉

Do the core and radiative zone of the Sun exhibit differential rotation?

No, they do not exhibit differential rotation.

p.30
太陽黑子與磁場

Which solar cycle corresponds to the year 2014?

Solar cycle 24.

p.16
太陽的結構與組成

What is the temperature of the Sun's core?

1.5 x 10^7 K.

p.21
太陽的結構與組成

What type of particles almost do not react with the Sun's internal matter?

Neutrinos.

p.21
核融合反應與能量產生

Why can't hydrogen fusion occur in the radiation zone?

Because the temperature and pressure are not high enough.

p.26
太陽的結構與組成

What is the thickness of the photosphere?

Approximately 500 km.

p.24
日震學與太陽內部結構

What did helioseismology reveal about the Sun's internal temperature?

It is higher than previously thought.

p.19
核融合反應與能量產生

What is the final reaction in the Proton-Proton Chain?

3 He + 3 He → 4 He + 2 1 H.

p.14
太陽的結構與組成

What is the effective temperature of the Sun?

5770 K.

p.24
日震學與太陽內部結構

What is the relationship between seismic waves and the Sun's internal structure?

Seismic waves help scientists model and understand the Sun's internal movements and structure.

p.2
太空天氣對地球的影響

What atmospheric effects can solar activity cause?

Auroras and other disturbances in the atmosphere.

p.23
太陽的自轉與差動自轉

What is the average rotation period of the Sun?

About 27 days.

p.20
核融合反應與能量產生

What does CNO stand for in the CNO Cycle?

Carbon-Nitrogen-Oxygen.

p.13
太陽的結構與組成

What is the layer of the Sun where energy is transported by radiation?

Radiative zone.

p.31
太陽的結構與組成

What is the lifespan of a granule?

Approximately 10 minutes.

p.30
太陽黑子與磁場

Which solar cycle corresponds to the year 2003?

Solar cycle 23.

p.16
太陽的結構與組成

How much greater is the pressure in the Sun's core compared to Earth's atmospheric pressure?

2.5 x 10^11 times.

p.25
太陽大氣層與光球層

What is the region between the Chromosphere and the Corona called?

Transition Region.

p.27
太陽黑子與磁場

What is the temperature difference between sunspots and other areas of the photosphere?

Sunspots are about 1000-1500 K cooler.

p.19
核融合反應與能量產生

What is the Proton-Proton Chain (PP Chain)?

The primary process for energy production in the Sun, accounting for 90% of its energy.

p.14
太陽的結構與組成

How does the volume of the Sun compare to Earth?

1.41 x 10^27 m^3, which is 1.3 million times the volume of Earth.

p.27
太陽黑子與磁場

How do sunspots typically appear?

They often appear in groups or pairs.

p.2
太陽風暴與太陽風

What is a Solar Flare?

A sudden eruption of intense high-energy radiation from the Sun's surface.

p.2
太陽風暴與太陽風

What is Solar Wind?

A continuous flow of charged particles from the Sun.

p.29
太陽黑子與磁場

How does the tilt angle of sunspot groups change?

The tilt angle increases with latitude.

p.22
日震學與太陽內部結構

What is the tachocline?

A transition layer between the radiative zone and the convective zone in the Sun, located at approximately 0.7 to 0.74 solar radii.

p.21
太陽的結構與組成

What is the range of the radiation zone in the Sun?

0.25 to 0.7 solar radii (R_s).

p.13
太陽的結構與組成

In which layer of the Sun does convection occur?

Convective zone.

p.21
太陽的結構與組成

What happens to gamma rays in the radiation zone?

They collide with particles and are absorbed, then re-emitted at lower energy.

p.28
太陽黑子與磁場

What is the magnetic field strength of sunspots?

Up to about 1000 Gauss.

p.28
太陽黑子與磁場

What phenomenon explains the formation of sunspots?

Strong magnetic fields suppress convective energy transfer.

p.19
核融合反應與能量產生

What is the first reaction in the Proton-Proton Chain?

1 H + 1 H → 2 H + e + + ν.

p.26
太陽的結構與組成

What part of the Sun can we see from Earth?

The photosphere.

p.18
核融合反應與能量產生

Why is high gas density important for sustaining the Sun's energy?

It increases the number of collisions necessary for fusion.

p.9
太空天氣對地球的影響

What does NOAA/SWPC stand for?

National Oceanic and Atmospheric Administration / Space Weather Prediction Center.

p.31
太陽的結構與組成

What is granulation in the context of the Sun?

A structure caused by convection, where each granule is about 1500 km in size.

p.23
太陽的自轉與差動自轉

What is the rotation period of the Sun at higher latitudes?

About 30 days.

p.30
太陽黑子與磁場

What happens to the polarity of sunspots in the Northern and Southern Hemispheres in the next solar cycle?

The polarity of sunspots will reverse in both hemispheres.

p.28
太陽黑子與磁場

How do sunspots compare to the photosphere in terms of brightness?

Sunspots are darker than the photosphere.

p.20
核融合反應與能量產生

What is the end product of the CNO Cycle?

Helium.

p.25
太陽大氣層與光球層

What is the height of the Chromosphere above the solar surface?

Approximately 10^3 km.

p.14
太陽的結構與組成

What is the age of the Sun?

4.5 x 10^9 years.

p.14
太陽的結構與組成

What is the spectral type of the Sun?

G2V.

p.24
日震學與太陽內部結構

What does helioseismology study?

The internal structure of the Sun using seismic waves.

p.14
太陽的結構與組成

What is the mass of the Sun in kilograms?

1.989 x 10^30 kg.

p.24
日震學與太陽內部結構

What is the significance of the interface between the convection zone and radiation zone?

It is where the Sun generates its magnetic field and is related to solar activity cycles.

p.24
日震學與太陽內部結構

What method is used to detect the frequency of the Sun's surface vibrations?

Doppler shift.

p.14
太陽的自轉與差動自轉

What is the sidereal rotation period of the Sun at the equator?

25.05 days.

p.2
太陽風暴與太陽風

What are Solar Energetic Protons?

High-energy protons emitted during solar events like flares and CMEs.

p.13
太陽的結構與組成

What are the main layers of the Sun's structure?

Core, radiative zone, convective zone, chromosphere, photosphere, and corona.

p.29
太陽黑子與磁場

What phenomenon is described by the tilt of sunspot groups?

The observed tilt of sunspot groups.

p.22
日震學與太陽內部結構

What occurs in the convective zone of the Sun?

Energy is transported by convection, with a significant temperature decrease towards the surface.

p.25
太陽大氣層與光球層

What is the outermost layer of the Sun's atmosphere?

Corona.

p.31
太陽的結構與組成

What causes the structure of granulation?

Convection, where the center of the granule rises and the surrounding areas sink.

p.17
核融合反應與能量產生

What is the mass of 4 hydrogen nuclei?

6.693 x 10^-27 kg.

p.28
太陽黑子與磁場

What is the average magnetic field strength of the Sun?

Approximately 1.0 Gauss.

p.18
核融合反應與能量產生

What must happen for two atomic nuclei to fuse?

They must be close enough to overcome their mutual repulsion.

p.18
核融合反應與能量產生

What type of motion is required for atomic nuclei to overcome repulsion?

High-speed collisions.

p.18
核融合反應與能量產生

What additional condition is necessary for nuclear fusion besides high temperature?

High gas density.

p.24
日震學與太陽內部結構

What was ruled out regarding the solar neutrino problem?

That it was due to incorrect models of the Sun's interior.

p.19
核融合反應與能量產生

What is the overall result of the Proton-Proton Chain?

4 hydrogen atoms produce 1 helium atom, energy, and 2 neutrinos.

p.15
太陽大氣層與光球層

What is the temperature range of the chromosphere?

4300 to 50,000 K.

p.24
日震學與太陽內部結構

What is the challenge in studying the Sun's internal structure directly?

It is not possible to place detectors inside the Sun.

p.2
太空天氣對地球的影響

What is a Single Event Upset?

A change in a bit of memory caused by a single ionizing particle.

p.22
日震學與太陽內部結構

Why is the plasma in the convective zone not dense or hot enough?

The energy from the radiative zone can no longer effectively transfer heat outward by conduction.

p.27
太陽黑子與磁場

Why do sunspots appear dark compared to the surrounding areas?

Because they are cooler than the surrounding photosphere.

p.15
太陽輻射與輻射層

What is the solar constant?

The energy received from the Sun per square meter at the top of Earth's atmosphere, approximately 1366 W/m².

p.26
太陽的結構與組成

Why is the Sun opaque to visible light below the photosphere?

Because it is not transparent to visible light.

p.22
日震學與太陽內部結構

What is the significance of the transition region between the radiative and convective zones?

It has a large shear profile, which can form large-scale magnetic fields.

p.21
太陽的結構與組成

What is the temperature range in the radiation zone?

From 7 million K to 2 million K.

p.17
核融合反應與能量產生

What is the mass loss during the hydrogen fusion process?

0.048 x 10^-27 kg.

p.25
太陽大氣層與光球層

What phenomenon is associated with the heating of the Corona?

Coronal heating.

p.25
太陽大氣層與光球層

What is the temperature of the Photosphere?

Approximately 10^4 K.

p.17
核融合反應與能量產生

Why is a large number of fusion reactions necessary for a star?

To counteract the star's gravitational collapse and maintain stability.

p.26
太陽的結構與組成

What is the temperature of the photosphere?

About 5800 K.

p.27
太陽的結構與組成

What is granulation in the context of the sun?

It refers to the grainy appearance of the solar surface caused by convection.

p.15
太陽黑子與磁場

What is the magnetic field strength of sunspots?

3000 Gauss.

p.26
太陽的結構與組成

Why can photons escape from the photosphere?

Because its temperature and density are appropriate.

p.24
日震學與太陽內部結構

What was previously used to predict the Sun's internal structure?

Star theory.

p.2
太空天氣對地球的影響

What are Cosmic Rays?

High-energy particles from outer space that can affect Earth's atmosphere.

p.2
地球磁層與磁暴

What is HF Radio Wave Disturbance?

Interference in high-frequency radio waves caused by solar activity.

p.15
太陽的結構與組成

What is the mean density of the entire Sun?

1410 kg/m³.

p.18
核融合反應與能量產生

What is the required temperature for nuclear fusion to occur?

10 million Kelvin (10^7 K).

p.15
太陽的結構與組成

What is the temperature at the center of the Sun?

15,000,000 K.

p.27
太陽黑子與磁場

What are the two main regions of a sunspot?

The penumbra and the umbra.

p.15
太空天氣對地球的影響

How much does a 1% change in solar radiation affect Earth's temperature?

It can cause a temperature change of 1 to 2 °C.

p.2
太空天氣對地球的影響

What is Radiation Damage?

Harm caused to living tissues by exposure to radiation.

p.2
地球磁層與磁暴

What are GICs in Power Systems?

Geomagnetically Induced Currents that can affect electrical grids.

p.2
地球磁層與磁暴

What is Signal Scintillation?

Rapid fluctuations in signal strength due to ionospheric disturbances.

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