The Seven Wonders of the World embodies the indefatigable human spirit, their adroit endeavours and unflagging toil. The Ancient wonders are reminiscent of a world long lost; the Modern wonders represent the limitless boundaries of human skill and technology while the Natural wonders are proof of the many marvels in nature. Learn about the Seven Wonders of the World and get all the related facts through our comprehensive listing of informative sites.
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The Seven Wonders of the Ancient World
 
The Great Pyramid of Giza
The Hanging Gardens of Babylon
The Temple of Artemis at Ephesus
The Statue of Zeus at Olympia
The Mausoleum at Halicarnassus
The Colossus of Rhodes
The Pharos of Alexandria
The Seven Natural Wonders of the World
 
Mount Everest
The Great Barrier Reef
The Grand Canyon
Victoria Falls
The Harbor of Rio de Janeiro
Paricutin Volcano
The Northern Lights
The Seven Underwater Wonders of the World
 
Palau
The Belize Barrier Reef
The Galapagos Islands
The Northern Red Sea
Lake Baikal
The Great Barrier Reef
The Deep Sea Vents
The Seven Wonders of the Medieval Mind
 
Stonehenge
The Colosseum
The Catacombs of Kom el Shoqafa
The Great Wall of China
The Porcelain Tower of Nanjing
The Hagia Sophia
The Leaning Tower of Pisa
The Seven Wonders of the Modern World
 
The Empire State Building
The Itaipú Dam
The CN Tower
The Panama Canal
The Channel Tunnel
The North Sea Protection Works
The Golden Gate Bridge
The Seven Forgotten Natural Wonders of the World
 
Angel Falls
The Bay of Fundy
Iguaçú Falls
Krakatoa Island
Mount Fuji
Mount Kilimanjaro
Niagara Falls
The Seven Forgotten Modern Wonders of the World
 
The Clock Tower (Big Ben)
Eiffel Tower
The Gateway Arch
The Aswan High Dam
Hoover Dam
Mount Rushmore National Memorial
The Petronas Towers
The Seven Forgotten Wonders of the Medieval Mind
 
Abu Simbel Temple
Angkor Wat
Taj Mahal
Mont Saint-Michel
The Moai Statues
The Parthenon
The Shwedagon Pagoda
The Forgotten Wonders
 
The Aztec Temple
The Banaue Rice Terraces
The Borobudur Temple
The Inca City
The Statue of Liberty
The Mayan Temples
The Temple of the Inscriptions
The Throne Hall of Persepolis
Petra
The Suez Canal
The Sydney Opera House
The Red Fort in India

Northern Lights

Although Galileo Galilei, the Italian mathematician, wasn't the first to see the Northern Lights, he gave it its scientific name. They have a number of names in history, although the scientific name for the phenomenon is Aurora Borealis (in Latin it means 'the red dawn of the north'), and 'aurora' for short. On the latitude where Galileo was living, the Northern Lights consist of mainly of red color. It is also called the Nordlys in Norwegian.

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The other names of the Lights are Aurora Australis for the Southern Lights (also called Sørlys in Norwegian) and the Aurora Polaris or Polar lights (Polarlys is the general Norwegian term for both the northern and the southern lights). The Northern Lights is a light phenomenon often seen in the northern regions. The lights have been around since Earth formed an atmosphere -the dinosaurs saw it, early humans saw it and our descendants will see it. The Northern Lights originate from our sun.

During large explosions and flares, considerable amounts of solar particles are emitted from the sun into deep space. These plasma clouds travel through space with immense speeds of over a million kms per hour, yet it takes them two or three days to reach Earth. While closing in they are captured by the Earth's magnetic field - the magnetosphere - and guided towards the two magnetic poles of the Earth - the geomagnetic south pole and the geomagnetic north pole.

On their way down towards the geomagnetic poles, the solar particles are stopped by Earth's atmosphere, which acts as an effective shield against these deadly particles. Due to the obstruction, they collide with the atmospheric gases present, and the collision energy between the solar particle and the gas molecule is emitted as a photon or a light particle. Countless such collisions make an aurora. Due to the collisions, the lights seem to be moving across the sky.

Quantitative measurements of the auroral heights were carried out by Carl Størmer between 1910 and 1940, using the parallax method. Two observers located between a distance of 50 to 100 kilometers apart took pictures of the same aurora at the same time. From the star patterns, they could read the angular distance and thus calculate the height. There are, however, certain variations that occur from time to time, depending on circumstances. Some of them are:

· The intensity and frequency is highest between 10:00 p.m. to 12:00 a.m. (this time span is known as the magnetic time).


· Seasonal changes also affect their frequency. In northern Norway, February, March and October are the best times for star-gazing.

· Since active areas on the sun's surface face the Earth after 27 days of the rotation cycle, the most brilliant auroras occur during this period.

· The Northern Lights' activity directly corresponds to the sun-spot activity, so they follow an 11-year cycle. As a direct result of this, the activity is affected 20-30% depending on whether it is a solar maximum or a solar minimum.


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