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Jump
to: Intro, The Sun and Us,
Layers of the Sun, Page
2: Sunspots, Prominences,
Solar Flares, Page 3: Effects
of Solar Activity, For Mature Audience Only...
SUNSPOTS:
Sunspots are cooler, darker areas in the photosphere that
appear to be dark blemishes on the sun's surface. In 1610,
Galileo used his telescope to watch these sunspots. His findings
made the Roman Catholic Church very upset, for they believed that
God's creations had no imperfections. Today, we know that
sunspots are not merely imperfections, but in fact they are daily
solar events. They seem to be darker because they are cooler than
the other gases, even though they are still very hot, almost 7,000
degrees Fahrenheit. They can range from 500 to 50,000 miles in
diameter. Sunspots have a dark center, called its umbra and a less
dark region, called it's penumbra. Sunspots may appear alone
or in groups of over one hundred, lasting for either a few hours or
as long as eighteen months. On average, a sunspot lasts about a
week. Scientists have not yet been able to fully understand where they
come from or their purpose for existence. What they do know is that
the sun has a strong magnetic field. When these magnetic forces
break through the photosphere, sunspots appear. Magnetic forces slow
down the vibration of gas atoms, making these areas cooler and
darker than the surroundings. In 1843, astronomer
Samuel Heinrich Schwabe, noticed that sunspots appear in cycles. A
few sunspots, is called a solar minimum. When there are many
sunspots, it is called a solar maximum. The periods between maximums
can average almost eleven years but can vary from seven to
seventeen.
The
sun has many sun spots, as shown on this Doppler image of the
sun taken by the SOHO Michelson Doppler Imager (MDI) 6767 Å
continuous imager. |
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PROMINENCES: When a
sunpots's magnetic forces erupt in to space, hot gases are
carried with them. These flaming arches are called prominences.
Prominences extend in to the corona and loop back. Most are about
100,000 miles long an 3,000 miles thick. They can soar as high as
two million miles above the surface, traveling at about 100 miles
per second. Some may move as fast as 830 miles per second.
Prominences are best seen during a total solar
eclipse.
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SOLAR FLARES:
Solar flares are one of the most spectacular sights of the sun.
Flares are explosions caused by magnetic forces on the sun's
surface. A flare may only last a few minutes but it can be as
powerful as ten million hydrogen bombs. A big flare can produce
enough energy to supply one of our major cities with electricity for
200 million years. A flare sends
billions of tons of solar matter in to space, along with light,
heat, and radiation. Particles of matter are carried by the solar
wind. Solar wind blows even harder after a flare, but is constantly
moving. It can carry one million tons of the sun in to space every
second at a speed of 200 to 500 miles per second. Solar wind can not
be seen, but can be felt. NASA has designed a solar sail that can
use solar wind to push a spacecraft between planets without an
engine.
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