Written Information: As you enter text, the area will expand. Make sure to check the required details of the assignment and review the rubric (see document links) to self-assess your work. Your paragraphs will be in block format, enter one return between paragraphs. The tab key, indent feature will not appear when typing directly into the wiki page.
Visuals
Make sure to include the location of
your image; add a caption with this information
Works Cited Sources: Include the source information for all of the magazine articles, reference sources (encyclopedias) and web site pages that were used to complete your project. The source information for encyclopedias may be found at the end or beginning of each entry in iCONN. When using periodicals, the publication information will be at the beginning or end of the article. This needs to be formatted for MLA standards. If it is not labeled 'Source Citation' it can be formatted appropriately by using EasyBib.com. You should use EasyBib for the web sites. The final Works Cited should be listed in alphabetical order by the first word of the source citation. Sample:
"Milky Way." Kids InfoBits Presents: Astronomy. Gale, 2008. Reproduced in Kids InfoBits. Detroit: Gale, 2012.
"The Milky Way." WMAP's Universe. NASA, 28 June 2010. Web. 06 Mar. 2012. <http://map.gsfc.nasa.gov/universe/rel_milkyway.html>.
Vergano, Dan. "Galaxy Bracketed by Big Bubbles." USA Today 10 Nov. 2010: 05A. Web. 6 Mar. 2012. Your Source List:
C. R. O'Dell, Ph.D., Professor of Space Physics and Astronomy, Rice University.
C. R. O'Dell, "Aurora," World Book Online Americas Edition, http://
Topic: Research Focus What is your topic? State the focus of your research: Notes
Include notes, statistics and facts that you will use to write your final paper. You may want to label sections of your notes to help you be more organized as you write. As you take notes from a source, you should list the source citation in the Works Cited section above.
Aurorais a natural display of light in the sky that can be seen with the unaided eye only at night. An auroral display in the Northern Hemisphere is called the aurora borealis, or the northern lights. A similar phenomenon in the Southern Hemisphere is called the aurora australis. Auroras are the most visible effect of the sun's activity on the earth's atmosphere.
Most auroras occur in far northern and southern regions. They appear chiefly as arcs, clouds, and streaks. Some move, brighten, or flicker suddenly. The most common color in an aurora is green. But displays that occur extremely high in the sky may be red or purple. Most auroras occur about 60 to 620 miles (97 to 1,000 kilometers) above the earth. Some extend lengthwise across the sky for thousands of miles or kilometers.
Auroral displays are associated with the solar wind, a continuous flow of electrically charged particles from the sun. When these particles reach the earth's magnetic field, some get trapped. Many of these particles travel toward the earth's magnetic poles. When the charged particles strike atoms and molecules in the atmosphere, energy is released. Some of this energy appears in the form of auroras.
Auroras occur most frequently during the most intense phase of the 11-year sunspot cycle. During this phase, dark patches on the sun's surface, called sunspots, increase in number. Violent eruptions on the sun's surface, known as solar flares, are associated with sunspots. Electrons and protons released by solar flares add to the number of solar particles that interact with the earth's atmosphere. This increased interaction produces extremely bright auroras. It also results in sharp variations in the earth's magnetic field called magnetic storms.During these storms, auroras may shift from the polar regions toward the equator.
People who live nearer the poles than the equator often see colored lights in the night sky. The lights usually look like moving curtains of green light, but may also be red, blue, or yellow. They are the auroras ("dawns," although unconnected to sunrise), also called the northern lights (aurora borealis) or southern lights (aurora australis). The further north or south, the more frequently auroras appear.
Auroras are caused by the bombardment of solar electrons on oxygen and nitrogenatoms. The electrons literally excite the oxygen and nitrogen atoms high in the atmosphere to create the beautiful light show we know as an aurora. Auroras Are Like Neon LightsNeon lights work by exciting gases inside of a tube with electricity. The resulting colors that you see are a result of the different gases used to make neon lights. In an aurora, the neon colors you see are the different wavelengths of light from gases high in the atmosphere.
The active phase of an auroral display will last on the order of 15 to 40 minutes and may recur in 2 to 3 hours. Auroral band features may persist all night. A red dominated auroral glow will be very diffuse. It will vary in location and intensity very slowly (time scales of half a minute or so).
Getting Started
Project Documents:
Rubric:
Space Exploration Adventure Rubric.doc
- Details
- Download
- 32 KB
, 
Space Exploration Adventure Rubric.pdf
- Details
- Download
- 49 KB
Written Information: As you enter text, the area will expand. Make sure to check the required details of the assignment and review the rubric (see document links) to self-assess your work. Your paragraphs will be in block format, enter one return between paragraphs. The tab key, indent feature will not appear when typing directly into the wiki page.
Visuals
Make sure to include the location of
your image; add a caption with this information
Detroit: Gale, 2012. http://galenet.galegroup.com/servlet/KidsInfoBits
Works Cited
Sources: Include the source information for all of the magazine articles, reference sources (encyclopedias) and web site pages that were used to complete your project. The source information for encyclopedias may be found at the end or beginning of each entry in iCONN. When using periodicals, the publication information will be at the beginning or end of the article. This needs to be formatted for MLA standards. If it is not labeled 'Source Citation' it can be formatted appropriately by using EasyBib.com. You should use EasyBib for the web sites. The final Works Cited should be listed in alphabetical order by the first word of the source citation.
Sample:
"Milky Way." Kids InfoBits Presents: Astronomy. Gale, 2008. Reproduced in Kids InfoBits. Detroit: Gale, 2012.
"The Milky Way." WMAP's Universe. NASA, 28 June 2010. Web. 06 Mar. 2012. <http://map.gsfc.nasa.gov/universe/rel_milkyway.html>.
Vergano, Dan. "Galaxy Bracketed by Big Bubbles." USA Today 10 Nov. 2010: 05A. Web. 6 Mar. 2012.
Your Source List:
C. R. O'Dell, Ph.D., Professor of Space Physics and Astronomy, Rice University.
C. R. O'Dell, "Aurora," World Book Online Americas Edition, http://
www.aolsvc.worldbook.aol.com/wbol/wbPage/na/ar/co/038160, October 20, 2001.
http://weather.about.com/od/spaceweather/ss/topauroras_5.htm
http://www.antarcticconnection.com/antarctic/weather/aurora.shtml
http://galenet.galegroup.com/servlet/KidsInfoBits
Topic: Research Focus
What is your topic?
State the focus of your research:
Notes
Aurorais a natural display of light in the sky that can be seen with the unaided eye only at night. An auroral display in the Northern Hemisphere is called the aurora borealis, or the northern lights. A similar phenomenon in the Southern Hemisphere is called the aurora australis. Auroras are the most visible effect of the sun's activity on the earth's atmosphere.
Most auroras occur in far northern and southern regions. They appear chiefly as arcs, clouds, and streaks. Some move, brighten, or flicker suddenly. The most common color in an aurora is green. But displays that occur extremely high in the sky may be red or purple. Most auroras occur about 60 to 620 miles (97 to 1,000 kilometers) above the earth. Some extend lengthwise across the sky for thousands of miles or kilometers.
Auroral displays are associated with the solar wind, a continuous flow of electrically charged particles from the sun. When these particles reach the earth's magnetic field, some get trapped. Many of these particles travel toward the earth's magnetic poles. When the charged particles strike atoms and molecules in the atmosphere, energy is released. Some of this energy appears in the form of auroras.
Auroras occur most frequently during the most intense phase of the 11-year sunspot cycle. During this phase, dark patches on the sun's surface, called sunspots, increase in number. Violent eruptions on the sun's surface, known as solar flares, are associated with sunspots. Electrons and protons released by solar flares add to the number of solar particles that interact with the earth's atmosphere. This increased interaction produces extremely bright auroras. It also results in sharp variations in the earth's magnetic field called magnetic storms.During these storms, auroras may shift from the polar regions toward the equator.
People who live nearer the poles than the equator often see colored lights in the night sky. The lights usually look like moving curtains of green light, but may also be red, blue, or yellow. They are the auroras ("dawns," although unconnected to sunrise), also called the northern lights (aurora borealis) or southern lights (aurora australis). The further north or south, the more frequently auroras appear.
Auroras are caused by the bombardment of solar electrons on oxygen and nitrogenatoms. The electrons literally excite the oxygen and nitrogen atoms high in the atmosphere to create the beautiful light show we know as an aurora. Auroras Are Like Neon LightsNeon lights work by exciting gases inside of a tube with electricity. The resulting colors that you see are a result of the different gases used to make neon lights. In an aurora, the neon colors you see are the different wavelengths of light from gases high in the atmosphere.
The active phase of an auroral display will last on the order of 15 to 40 minutes and may recur in 2 to 3 hours. Auroral band features may persist all night. A red dominated auroral glow will be very diffuse. It will vary in location and intensity very slowly (time scales of half a minute or so).