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The Effects of Coronal Mass Ejections (CME) on Planet Earth

The Effects of Coronal Mass Ejections (CME) on Planet Earth. By Alvin Sanchez and Andrew Walant. What are CMEs?. Coronal Mass Ejection (CME) are gas-formed plasma storms that burst out of the Sun’s corona.

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The Effects of Coronal Mass Ejections (CME) on Planet Earth

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  1. The Effects of Coronal Mass Ejections (CME) on Planet Earth By Alvin Sanchez and Andrew Walant

  2. What are CMEs? • Coronal Mass Ejection (CME) are gas-formed plasma storms that burst out of the Sun’s corona. • They occur from the sun’s corona at an explosive rate of 1 million mph. The fastest recorded was set at 4.5 million mph. • CME’s occur about once a week, but solar maximum rates of about two per day are not out of the ordinary. • The area called dark matter, also referred to as the interplanetary medium, is where the CMEs travel through this to reach the earth’s magnetosphere. • CMEs were only acknowledged until after the coming of the great space race, which began with the release of the satellite Sputnik into space. • CME’s not only disrupt life on earth they disrupt the flow of solar winds.

  3. Common Misconceptions of Solar Activity Explained… • CME’s and solar winds are not the same thing. A solar wind can be disrupted by a CME and have CME’s accelerated to their speeds, either high of low. More than half the time, CME’s are a result of solar flares. Otherwise there is not much difference between CMEs and Solar winds. • The CME’s are not the same throughout. The comet like structure is similar to what a CME looks like. Although, its movements are unknown. • CME’s can be visible during an eclipse. During this event, when the sun is blocked by our moon, you would look like at the Corona using a coronagraph. You would indicate it as the outlines around the moon. • The Corona, where the solar winds extend and CMEs form, can be also observed using x-ray spectroscopy.

  4. Corona • The Corona is a type of atmosphere that surrounds the Sun at over a million degrees. • Its physical features include those of coronal loops and releasing plasma out into space. • Those phenomena are called solar flares and CMEs. They are created around the sun’s atmosphere.

  5. Solar Flares • Solar flares, are usually created from explosive spots near cooler regions known as Sunspots. • They produce electromagnetic radiation that emerge into the Suns corona emitting stored energy into the surface. • They can be observed at wavelengths from radio to gamma rays. • Solar flares can actually cause a CME by its Kinetic energy passing through the Corona.

  6. Physical properties of CMEs • CMEs are simply particles consisting of protons and electrons that eject from the Suns corona. • CMEs are formed as bubble like plasma being pulled into space. • They are often associated with solar flares or solar wind. CMEs originate from active regions and are usually from stored energy formed in the coronal belt. • They travel at an average speed of 1 million miles per hour and are much cooler than solar flares.

  7. CMEs affecting Earth • When CMEs eject out of the Suns atmosphere, and travel towards our earth. About most of the energy being impacted into our planet gets repelled due to our magnetosphere. • After impact, the ejection extends and reaches the night side of the magnetosphere. This creates a strong electrical force.

  8. Disruption on Earth • When CMEs impact our earth and we get affected by its enormous energy, about 1% of those particles penetrate pass our magnetosphere. (interplanetary CMEs) • Thus creating disruptions and corrosions into our planet, such as power surges through every house, interferences with radio transmissions, damages to satellites and spacecraft, and any mechanism using electrical currents. • LASCO, a telescope that was sent to observe and collect data from the sun, can tell us when we are about to have a solar disturbance from any solar storm.

  9. Article Summaries from NASAon Solar flares

  10. On October 1st, 2007 • On April 20, 2007 Encke, a comet, was travelling a little to close to the sun. • This caused a “magnetic connection” between a CME and the tail, ripping it off. • The mass of a CME is spread out over a large area of space which makes it is surprising that it could rip the tail of the comet off. • It is also surprising because a Gossamer CME releases a few nanopascals of pressure softer than a baby’s breath. • This shows the destructive power a CME has in short range and without the protection of a magnetosphere.

  11. On May 27, 2008 • The “cartwheel” to the left occurred on April 9, 2008. • It happened because the magnetic flux tube broke under a lot of stress and caused an explosion greater than 100 million hydrogen bombs. In other words, the effect was a CME. • As can be seen in the second picture the magnetic flux tube healed itself rather quickly. • This was extremely exciting for scientists because it is extremely rare • This entire event will lead to more discoveries about the “magnetic reconnection” of Solar flares and CMEs.

  12. The 1859 Super storm • The solar storm in 1859 was the strongest and most greatest ever recorded. • The auroras on this day were as far south as the Caribbean • Scientists believe the storms happen once every 500 years. • Even if it happens every 50 years it would still have drastic effects on humans Ex. Some of our satellites would be fried • The large CME could also cause coast to coast blackouts and jam radios.

  13. The End

  14. Bibliography • http://imagine.gsfc.nasa.gov/docs/science/mysteries_l1/corona.html • http://pwg.gsfc.nasa.gov/istp/nicky/cme-chase.html • http://www-spof.gsfc.nasa.gov/Education/wsolwind.html • http://www.nasa.gov/mission_pages/stereo/news/stereo_astronauts.html • http://www.suntrek.org/flowing-from-sun/solar-storms-comets/what-causes-cmes.shtml

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