electron excitation and emission on the CG.
Click on the picture above.You can watch "System of electron excitation and emission" on the CG.
 

The photos we usually see portray aurorae in a kaleidoscopic range of colors. So why was the aurora we encountered in step 3 red? The basic colors of the aurora are green and pink. The electrons accelerated by the action of the solar wind and the Earth's magnetic field collide with the air (which consists chiefly of oxygen and nitrogen), separating the electrons from their the atoms somewhat. This process is called excitation. When the excited electron, which had been circling the outer perimeter of the atom, rejoins the its original orbit in the atom, this surplus energy is released. This energy is visible as luminescence, and its properties vary depending on the element. The light emitted from oxygen atoms is generally green or dark red, while that of nitrogen molecules is pink. Hence the basic colors of the aurora are green and pink. This is how we know that the aurora observed at Rikubetsu-cho in Hokkaido was created by the luminescence of oxygen atoms.

We can demonstrate that each element has its own characteristic color in an experiment known as the "flame reaction." In this reaction, solutions of different elements are heated to energize the atoms. The electrons are excited (moved to the a higher orbit in the atom), then differences are observed in the color of the light generated when the electrons return to their original orbits. By comparing the colors with those in the photo below, try to guess which type of atom the light is generated by.

Strontium(Sr)
Calcium(Ca)
Cesium(Cs)
Barium(Ba)
Click on the picture above. You can watch "System of electron excitation and emission" on the CG.
 
By this method, we can analyze the wavelength of the light generated when an unknown atom or molecule is excited to determine what element it is. As we mentioned in the opening paragraph, Jupiter has its own aurora; since its atmosphere consists mainly of hydrogen, its color is the pink characteristic of that element. By analyzing the light of the aurora, we can learn what atoms and molecules are prevalent in the upper atmosphere where the aurora forms. This field of study, known as spectroscopy, has long been applied in astronomy, enabling researchers to determine the types of atoms and molecules present in distant nebulae. Currently numerous gases are known to exist in nebulae, including hydrogen and helium.

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