Aurora Borealis Research Papers

CORAL GABLES- Fla. (April 19 2015) – University of Miami are putting into effect at the mental health services offered at their University.

On day 1 the scientist reached the Smithsonian and talked to the people in charge. The instrument was a Meteor Composition Detector and X-Ray, it will detect any trace of meteor trails in the atmosphere or space and see what they hold inside. The people of Clare were a little freaked out on this day, but still did not know what

Overtime what constitutes as a city has drastically changed. Migration, economic growth, and physical development of land have turned small towns into bustling cities; these circumstances have transformed the once small suburban town of Aurora into one of the largest city in Illinois. Aurora’s size, density, and diverse population have made it the city it is today. Although, Aurora is drastically different than Chicago, it still possessed the key characteristics of a city while remaining unique.

3. Solar Flares: these are ejections of large volumes of gas. They can sometimes head our way causing radio interference and auroras.

Despite the amounts of incoming radiation, very little actually reaches the Earth’s surface. One layer of protection the Earth provides is in the form of a magnetic field that deflects charged particles from reaching the Earth’s surface. This magnetic field is generated by a combination of the liquids within the Earth’s core and the interplanetary magnetic field generated by the Sun. This field reaches out thousands of miles from Earth, so when solar wind travels through space and encounters Earth’s

Coronal Mass Ejection also known as CME is usually created around the sun’s surface by magnetic reconnection. CME is a large bubble of gas and magnetic field lines that are emerged from the sun. There isn’t a full proven understanding of how CME’s occur but Astronomers have come to a theory that because the sun is a fluid, the turbulence gets kinks that get shot out into space in any direction as a superheated gas. The gas that is ejected from the sun is made of protons and electrons carried through solar winds. This gas is known as plasma and can accelerate over 1 million miles per hour and reach Earth that is 93 million miles away in less than 4 days. When the sun is most active Coronal Mass Ejections can happen multiple times per day however, it usually occurs once every 5 days.

Solar wind is a continuous stream of mostly of protons and electrons but also some atomic nuclei. It results from radiation pressure pushing parts of the corona into space and peaks during times of increased sunspot activity. Most of the solar wind is diverted around the Earth due to Earth’s magnetic field.

In 1945, Joseph Henry and Stephen Alexander, professors from Princeton University, discovered that sunspots emitted less radiation than surrounding areas of the sun. This is because the Sun’s outer shell, the photosphere, behaves as plasma, which is a very good conductor of electricity, and interacts with the magnetic fields of sunspots. The plasma slows down and cools to 1000 K less than the surrounding photosphere which makes it look darker than the surrounding areas. These areas were concentrated magnetic fields appear, are usually part of a loop, as sunspots generally present in pairs which line up parallel to the equator, showing a magnetic polarity. The sunspots in each hemisphere have the opposite polarity to the other. Over the 11 year cycle, the whole polarity reverses as the new set of sunspots form away from the Sun’s equator. Therefore, a complete 22 year cycle returns the polarity to its original

A halo event is a coronal mass ejection aimed directly for the Earth. The plan is to use magnetic scoop technology to form an enormous magnetic loop projecting out from the surface of the sun. As plasma drains upwards into the magnetic loop, anyone looking from Earth would see a dark filament of cooler plasma against the hotter chromosphere. Once sufficient mass has been entrapped by the magnetic loop, Sans Gravitas triggers a magnetic reconnection event, ejecting energy in the form of intense radio and x rays, as well as a mass in plasma in excess of four billion tons. This mass will speed toward the Earth at five hundred kilometers per second, expanding as it travels through space, and impact the alien

2nd P: To understand the effects of solar plasma on Earth’s magnetosphere, one must look at the creation of plasma in the early days of the sun. The sun’s creation is similar to the process in the explosion of a hydrogen bomb, only with the energy created equaling the force of 10 billion hydrogen bombs per second. When the sun was originally forming, hydrogen gas in the middle was crushed from weight above. Eventually, the pressures and temperatures reached such an intense point to where the hydrogen atoms broke apart into electrons and photons, thus, creating plasma. Photons from the explosion of electrons and protons are made so fast and so many at a time that it creates the observed power of the sun. This reaches us as sunlight. Even though the process of the energy created is relatively quick, the process in which the photons travel to Earth happens over a long time within the Sun’s layers. The energy of sunlight that shines down on us today is over 100,000 years 1

The corona is the hotter than the surface of the sun (Fox). The ribbon-like strands surround the freckled skin with hair, frizzing. The flares are zits popping off the bubbling surface, the magnetic seasons in cycles. Even the sun has mood swings.

For this essay, I chose the constellation Corona Borealis. It was one of 48 constellations listed by Ptolemy, an astronomer of the second century. Its Latin name is translated as “Northern Crown”, due to its crown-like shape. The brightest star in the constellation is Alpha Coronae Borealis, and is a magnitude 2.2 star. Other notable stars in the constellation include R Coronae Borealis, a yellow supergiant, and T Coronae Borealis, also known as the Blaze Star, which is a recurrent supernova. Corona Borealis covers 179 square degrees (0.433% of the sky), placing it 73rd in size of the 88 recognized constellations. It is positioned in the Northern Celestial Hemisphere, and is surrounded by Hercules (to the east), Boötes (to the north),

In the 18th century, a new form of art, called Romanticism developed in Europe, and reached its peak in the 19th century. One of the significant artists of the Romanticism art period was Frederick Edwin Church, a painter from New York, who portrayed landscapes. One of his remarkable works is his oil, canvas piece, Aurora Borealis, in which he portrays the Northern Lights.

Firstly, charged particles from the sun during solar flare penetrate Earth's magnetic field and collide with atoms and molecules in our atmosphere. These collisions result in little bursts of light called photons (a particle representing a quantum of light of other electromagnetic radiation) Great storms on the sun send gusts of solar particles hurtling across space.

Storms in space could have a devastating effect on our society. Solar storms are a result of solar flares and are electromagnetic in nature. They are capable of causing power outages and halting all types of communication, including; electronic pagers; radio and television broadcasts; credit card transactions; military communications; etc.