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A solar flare creates a radio disturbance on Earth a few minutes after going off and again several days later.Explain.

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A flare will give off intense X-rays and...

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We know the Sun rotates differentially by observing sunspots; as with Jupiter the solar equator rotates the fastest.

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The surface magnetic field of the Sun is found by measurement of the extra width in spectral lines due to the ________ Effect.

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In the proton-proton cycle,the helium atom and neutrino have less mass than the original hydrogen.What happens to the "lost" mass?


A) It is recycled back into hydrogen.
B) It is ejected into space.
C) It is converted to energy.
D) It is transformed into electrons.
E) Conservation of mass dictates no mass can be lost.

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If the corona is so hot,why must we wait for a total solar eclipse to glimpse it?

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It is so hot that almost all the energy ...

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Prominences hanging off the limb of the Sun are the same as filaments seen in front of the disk.

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The solar corona is much cooler than the Sun's surface; hence we must wait for a total solar eclipse to glimpse it with the naked eye.

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The pattern of rising hot gas cells all over the photosphere is called:


A) filaments.
B) granulation.
C) sunspots.
D) convective projections.
E) prominences.

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The number of sunspots and their activity peak about every:


A) 36 days.
B) six months.
C) year.
D) eleven years.
E) 76 years.

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The most striking example of solar variability was:


A) the Dust Bowl drought of the 1930s.
B) the Maunder Minimum from 1645-1715.
C) the Sporer Minimum that doomed the Anasazi.
D) the fall of Rome.
E) Joseph's seven lean years in the Old Testament.

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How long does the sunspot cycle last,on average?


A) between 25 and 35 days
B) 365.25 days
C) about seven years
D) about 11 years
E) about 76 years

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In the proton-proton cycle,you must first make deuterium,then helium.

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Scientists suspect changes in the flow of the Sun's Conveyor Belt caused the Sun to be less active in 2008 and 2009 than had been seen in almost 100 years.

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What is it about the Sun's corona that astronomers don't understand?


A) No one knows why that part of the Sun's atmosphere does not drift away into space.
B) During total solar eclipses, the corona sometimes disappears from view.
C) The corona seems to absorb 2/3 of the neutrinos that pass through it.
D) The corona is much hotter than layers of the Sun that are closer to the solar interior.
E) The Sun's corona extends to the outer reaches of the solar system.

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During a period of high solar activity,the corona:


A) disappears.
B) is more irregular.
C) cools almost to the temperature of the photosphere.
D) becomes smooth and even.
E) shrinks to half its normal size.

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What was the Maunder Minimum?

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A period of unusually low solar activity...

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The density of the Sun is most similar to which object?


A) Halley's Comet's nucleus
B) the Earth
C) Mercury
D) the Moon
E) Jupiter

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What do sunspots tell us about the Sun's rotation rate?

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Watching and timing sunspots as they tra...

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Large circulation patterns in the Sun,dubbed "Conveyor Belts," transport material from the equator to the poles,then back to the equator at a depth of 300,000 km,take how long to complete a cycle?


A) Less than a day
B) A few years
C) A few decades
D) A few centuries
E) Tens of millions of years, comparable to the convection cycle in Earth's mantle

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The luminosity of the Sun is a measure of:


A) the energy received by the Sun on Earth's surface.
B) the energy received by the Sun at the location of Earth.
C) the energy received by the Sun at any location in the solar system.
D) the energy emitted by the Sun at the photosphere.
E) the total energy emitted by the Sun in all directions.

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