How Does The Color Of The Lights?

Named for the Roman goddess of dawn, the aurora is a mysterious and unpredictable display of light in the night sky. The aurora borealis and aurora australis – often called the northern lights and southern lights – are common occurrences at high northern and southern latitudes, less frequent at mid-latitudes, and seldom seen near the equator. While usually a milky greenish color, auroras can also show red, blue, violet, pink, and white. These colors appear in a variety of continuously changing shapes. Sometimes the aurora is so dim and scattered as to be mistaken for clouds or the Milky Way; sometimes it is bright enough to read by. What does an aurora look like? Auroras can appear as long, narrow arcs of light, often extending east to west

However, this has not happened and it’s starting to make secular scientist themselves admit that our sun is special and unique in design, because it does not emit these monster super flares like the ones produced by Proxima Centauri. The question is, could our sun send out such a flare powerful enough to even melt the ice on Jupiter’s moon’s, destroy earth’s ozone layer and even obliterate all our satellites? Well the answer is yes. Scientist have studied other sun like stars in our galaxy and discovered that they produce these super flares about once a century. But, they have no explanations as to why our sun does not produce such solar

In Race and Ethnicity Class we read two books. We read The Color of Water and Night. I really liked both books. They are informative on two different races. They are interesting and emotional.

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.

Overall, results indicate that the manipulation of the color of questionnaire had no effect on mood. However, there was an effect of time of day on mood as well as an effect of gender on mood. The results did not support the main hypothesis that different colors would elicit different moods. Thus, this study found no support for the prediction that brighter colors would elicit positive moods, whereas less bright colors would elicit negative moods. These results do not support past research findings that brighter colors tend to elicit positive moods, whereas, dark colors elicit negative moods (Hemphill, 1996; Kaya & Epps, 2004). Moreover, this result was not expected given the previously discussed research by Weller and Livingston (1988)

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.

Solar flares are defined as brief eruptions of highly energized radiation from the sun, but why does this happen? Solar flares occur when magnetic energy is built up, then rapidly released at once, during, the sun gives off generous amounts of X and gamma rays. Strangely enough the energy of a solar flare is ten million times that of a volcanic eruption, but only 1/10th of the energy that comes from the sun every second. There are three stages of solar flares, first, the precursor stage “where the release

The northern lights (aurora borealis) and southern lights (aurora australis) occurs at high northern and southern latitudes. They are uncommon at mid-latitudes and almost never seen near the equator. Auroras displays a great range of colours including red, blue, violet, pink, and white yet milky-greenish colour is most common. These colours also appear in dynamic patterns and shapes. They can also be mistaken for clouds when they are very dim.

Hello, and welcome to Physics Flies “wonders of the universe tour” preview. I am here today to give you a glimpse of some of the wonders of the universe that you will experience during Physics Flies Aurora Borealis tour such as why the colour of a star is related to its surface temperature, what exactly are H-R diagrams and the relationship between temperature of a celestial body and its radiation wavelength.

The Northern Lights are an extraordinary, surreal and legendary phenomenon. They are magical: if you have already observed them in nature, you know that words fail to describe this breathtaking spectacle. Out in the wide open darkness, nature’s spectacular display takes on an added dimension when the glowing ribbons of light are accompanied by the howling of wolves.

As many people know, Aurora Borealis are lights in the sky. The lights are seen over the attractive shafts of the northern and southern sides of the equator.1 They are known as 'Aurora borealis' in the north and 'Aurora australis' in the south.1 Auroral showcases show up in numerous colors light green and pink are the most widely recognized.1 “The lights of the Aurora for the most part stretch out from 80 kilometers (50 miles) to as high as 640 kilometers (400 miles) over the world's surface.”1 Shades of red, yellow, green, blue, and violet have been accounted for.1 The lights show up in numerous structures from patches or scattered billows of light to streamers, circular segments, undulating drapes or shooting beams that light up the sky with

Transition*** The first point I would like to expand on, is what the Northern Lights are, and where they are found.

Aurora Borealis or the Northern Lights, as they are most popularly known, are bright dancing lights that are usually either a pale green or a pink, but they have been reported being seen in more vibrant colors as well. They are usually seen above the magnetic poles of the northern and southern hemispheres. They are caused by collisions between electrically charged particles from the sun that enter the Earth’s atmosphere. The lights can be seen in many forms: patches, scattered clouds of light, streamers, arcs, rippling curtains, or shooting rays that light up the sky with an eerie glow. Aurora Borealis can be seen anywhere from late September to March from 6 p.m. to 6 a.m., but the lights are very

It’s dark, then all of a sudden everything lights up with colors of green, red and blue. The cascade of colors roaming through the sky has the crowd of people in “awe.” These colors of light are known as the Northern Light’s, also known as Aurora Borealis.

The solar wind containing these hot gases races toward the edges of the solar system, and smash in to the magnetosphere. The magnetosphere protects the earth by deflecting most of the solar wind around the planet. Trillions of these charged particles mange to get through and project from the North and South poles. Energy released in this fashion excites atoms of nitrogen and oxygen, which in turn emit pulses of colored light. These formations are called an aurora. The aurora borealis, which are visible in Alaska, are a result of this sort of space storm.