A) magnetic field and the force of gravity
B) force of gravity and outward gas pressure
C) numbers of hydrogen and helium nuclei
D) hydrogen gas pressure and helium gas pressure
Correct Answer
verified
Multiple Choice
A) only in a narrow band along the solar equator
B) only at the polar regions
C) only in coronal holes
D) only within sunspot groups
Correct Answer
verified
Multiple Choice
A) 3/4 of 1%
B) 100%
C) 1/20 of 1%
D) 4%
Correct Answer
verified
Multiple Choice
A) less massive
B) cooler in its core
C) less luminous
D) smaller
Correct Answer
verified
Multiple Choice
A) The neutrinos oscillate and change their nature en route from the Sun to Earth.
B) The core of the Sun is actually about 10% cooler than had been originally predicted.
C) The Davis result was subjected to much uncertainty because it measured only a small-yield side branch of the main nuclear reaction.
D) The neutrinos Davis detected were coming not from the Sun but instead from sources within Earth.
Correct Answer
verified
Multiple Choice
A) the Moon
B) the Sun
C) Jupiter
D) Saturn
Correct Answer
verified
Multiple Choice
A) a storm of waves and vortices on the Sun's surface generated by a solar flare
B) the constant flux of photons from the Sun's visible surface
C) the circulation of gases between the equator and the poles of the Sun
D) the Sun's outer atmosphere streaming out into space
Correct Answer
verified
Multiple Choice
A) less dense but with a greater vertical extent.
B) cooler and with a greater vertical extent.
C) denser but with a narrower vertical extent.
D) hotter and with a narrower vertical extent.
Correct Answer
verified
Multiple Choice
A) edge
B) center
C) top
D) bottom
Correct Answer
verified
Multiple Choice
A) The Sun does not have an overall coherent field but magnetic fields, and their polarity is centered on sunspots and randomly distributed over the Sun.
B) The northern and southern hemispheres have the same magnetic polarity, which reverses every 11 years.
C) The northern and southern hemispheres have opposite magnetic polarity, which reverses every 11 years.
D) The poles of the Sun have the opposite magnetic polarity from the equator, which reverses every 11 years.
Correct Answer
verified
Multiple Choice
A) during lunar eclipses, when the sky is darker.
B) during solar eclipses.
C) over a period of a few years around times of maximum solar activity.
D) in spring and fall seasons because of the tilt of the spin axis of the Sun.
Correct Answer
verified
Multiple Choice
A) convection zone.
B) conduction zone.
C) photosphere.
D) corona.
Correct Answer
verified
Multiple Choice
A) the impact of meteoroids and comets on the solar surface.
B) differential rotation and its effect on weak magnetic fields just under the solar surface.
C) dark, absorbing clouds hanging over the surface, above the magnetic field regions.
D) coronal holes, which darken the surface.
Correct Answer
verified
Multiple Choice
A) conduction because the chromosphere and corona contain high densities of free electrons that facilitate conduction.
B) rearrangements within complex magnetic field structures that energize the ionized gas.
C) convective currents in the chromosphere that carry hot gas outward from the photosphere.
D) radiative heat from the photosphere that is strongly absorbed by highly ionized atoms such as Fe XIV.
Correct Answer
verified
Multiple Choice
A) thermonuclear fusion in the core
B) radioactive decay of the nuclei of heavy elements
C) primordial heat, left behind from when the Sun first formed
D) heat released by gravitational contraction as the Sun slowly shrinks
Correct Answer
verified
Multiple Choice
A) is almost constant from the center to the surface but falls abruptly above the visible surface.
B) decreases outward from the center but then increases again in the atmosphere.
C) decreases smoothly outward from the center, gradually merging at the "top" of the atmosphere into the cold of the interplanetary medium.
D) increases and decreases several times between the center and the surface, then decreases through the atmosphere.
Correct Answer
verified
Multiple Choice
A) upward in the centers of some cells and downward in the centers of others; the gas cools as it passes over the boundaries between cells.
B) upward in the bright cell centers and downward around the darker edges.
C) downward in the bright cell centers and upward around the darker edges.
D) almost nonexistent; the dark patterns represent a network of absorbing gases overlying the photosphere.
Correct Answer
verified
Multiple Choice
A) visible.
B) radio.
C) X ray.
D) ultraviolet.
Correct Answer
verified
Multiple Choice
A) The gases near the edge are in regions where stronger magnetic fields inhibit the emission of light.
B) We see more deeply into the Sun near its edge, and the gas is cooler at the deeper levels.
C) We see into shallower layers of the Sun near the edge, where the gas is cooler and so emits less light.
D) We see into shallower layers of the Sun near the edge; because the gas is less dense there, it emits less light.
Correct Answer
verified
Multiple Choice
A) Refraction of light around the coin will cause light from the photosphere to enter your eye along with light from the chromosphere.
B) Light from the very rarified chromosphere is too weak to penetrate Earth's atmosphere.
C) Scattering by Earth's atmosphere will allow light from the photosphere to pass around the coin and enter your eye.
D) Even with electronic equipment, it is not possible to hold the coin steady enough against the apparent motion of the Sun to view only the thin chromosphere.
Correct Answer
verified
Showing 221 - 240 of 274
Related Exams