1. Which is the origin of the sun’s energy?
A. charged particles
B. burning hydrogen
C. solar flares
D. nuclear fusion
2. Which of the following protects Earth's atmosphere from solar wind?
A. convection currents
B. radiative zone
C. magnetosphere
D. hydrogen atoms
3. How have astronomers formed their ideas about the layers of the sun?
A. observing all the layers during total solar eclipses
B. using theoretical models combined with known data
C. Developing mathematical models based only on known data
D. making direct observations of the sun's layers
4. Two astronomers are viewing temperature data from each of the sun's layers, but the layers aren't identified. Describe one way the scientists can use temperature to identify which layer they are studying.
A. The lowest temperatures are from the core.
B. The highest temperatures are from the corona.
C. The lowest temperatures are from the photosphere.
D. The highest temperatures are from the radiative zone.
23 answers
A. charged particles
B. burning hydrogen
C. solar flares
D. nuclear fusion
A. convection currents
B. radiative zone
C. magnetosphere
D. hydrogen atoms
A. observing all the layers during total solar eclipses
B. using theoretical models combined with known data
C. Developing mathematical models based only on known data
D. making direct observations of the sun's layers
A. The lowest temperatures are from the core.
B. The highest temperatures are from the corona.
C. The lowest temperatures are from the photosphere.
D. The highest temperatures are from the radiative zone.
rapid spinning of metals in the core
uniform clockwise rotation of charged particles
uneven churning of plasma
upward movement of super-heated gases in the convective zone
A. They appear as bright spots on the sun's surface.
B. They tend to occur during active periods of the solar cycle.
C. They are caused by outward fluctuations of the sun's magnetic field.
D. They appear as dark spots on the sun's surface.
C. They are caused by outward fluctuations of the sun's magnetic field.
Geomagnetic storms occur only occasionally; solar wind is constant.
Geomagnetic storms are constant; solar wind occurs only occasionally.
Geomagnetic storms are associated with CMEs; solar wind is associated with the constant activity in the sun.
Solar wind sometimes results in geomagnetic storms; geomagnetic storms do not cause solar wind.
Geomagnetic storms travel at the speed of light, while solar wind takes four days to reach Earth.
Geomagnetic storms are associated with CMEs; solar wind is associated with the constant activity in the sun.
Solar wind sometimes results in geomagnetic storms; geomagnetic storms do not cause solar wind.
It generates auroras.
It forms radiation belts.
It causes geomagnetic storms.
It develops solar wind.
It causes geomagnetic storms.
electrical systems in satellites will fail
power grid operations will go offline
high-frequency radio waves used for radio communication will be blocked
radio navigation systems and global positioning systems will be inaccurate
Responses
solar wind
solar wind
solar energetic particles
solar energetic particles
solar flares
solar flares
coronal mass ejections (CMEs)
Responses
Satellites will need to be repositioned due to satellite drag.
Satellites will need to be repositioned due to satellite drag.
Radio communications at high latitudes will be blocked.
Radio communications at high latitudes will be blocked.
Power will go out in cities across the world.
Power will go out in cities across the world.
Radio navigation and GPS systems will be inaccurate.
Radio navigation and GPS systems will be inaccurate.