The Sun
The Sun rests in the center of our solar system and the very world that we live in is the product of it. The Sun provides us with light that nourishes the plants and organisms on earth and thus starting the food chain in with all living things are apart of; it goes without question that if the Sun was not there we wouldn’t be here. Because of the supreme importance of this star we have invested our time and money to understand what goes on in the Sun and what keys it might hold for future science. It is important to know three main abnormal events that occur on the Sun: Sunspots, Solar flares and Coronal Mass Ejections. These events have interacted with us here on Earth. These events follow what is called the “Solar Cycle”. A Solar cycle is the cycle of solar minimums and maximums, the maximum level of the cycle is the “Active Sun” area, this is where the most sunspots, solar flares and Coronal Mass Ejections are observed. A sunspot is a relatively cool area on the Sun. First studied in detail by Galileo this was the first evident to prove that the Sun wasn’t a perfect creation but was something that was ever changing. They are darker and cooler in relation to their surrounding but if they were to be isola
The Sun is 150 million kilometers from the Earth and still has the power to affect us. It keeps us warm, it feeds the plants that nourish every living that is on the Earth and is thanked for the birth of all the planets in our solar system. But the Sun still holds many secrets that we have yet to discover. With the creation of better telescopes and better recording equipment we may learn even more about this fascinating star in the future. This interaction with the clouds on our planet might explain the drought in South Africa, but there is much debate about the validity of it.
Some topics in this essay:
Kelvin Sunspots,
Richard Hodgson,
Ejections Coronal,
Kelvin Inside,
GCR GCR,
Mass Ejections,
Flares Flare,
Earth Moon,
CME Halo,
Yes Coronal,
magnetic field,
solar flares,
coronal mass,
coronal mass ejections,
mass ejections,
solar wind,
active regions,
magnetic field lines,
solar flares coronal,
sunspots solar,
solar cycle,
1 sunspots,
solar flare,
sunspots solar flares,
flares coronal mass,
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Approximate Word count = 1891
Approximate Pages = 8 (250 words per page double spaced)
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