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・ Fermeuse Formation
・ Fermi (crater)
・ Fermi (disambiguation)
・ Fermi (microarchitecture)
・ Fermi (Turin Metro)
・ Fermi acceleration
・ Fermi and Frost
・ Fermi arc
・ Fermi ball
・ Fermi contact interaction
・ Fermi coordinates
・ Fermi energy
・ Fermi filter
・ Fermi Gamma-ray Space Telescope
・ Fermi gas
Fermi glow
・ Fermi heap and Fermi hole
・ Fermi level
・ Fermi Linux
・ Fermi liquid theory
・ Fermi motion
・ Fermi Nuclear Power Plant
・ Fermi paradox
・ Fermi Paradox (album)
・ Fermi point
・ Fermi problem
・ Fermi Project
・ Fermi resonance
・ Fermi surface
・ Fermi surface of superconducting cuprates


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Fermi glow : ウィキペディア英語版
Fermi glow
The Fermi glow are ultraviolet-glowing〔"(The Heliosphere is Tilted - implications for the 'Galactic Weather Forecast'? )". (Hubble ). 13 March 2000.〕 particles, mostly hydrogen,〔 originating from the solar system's bow shock, created when light from stars and the Sun enter the region between the heliopause and the interstellar medium〔"(A Glowing Discovery at the Forefront of Our Plunge Through Space )". SPACE.com. 15 March 2000.〕 and undergo Fermi acceleration,〔"(Where the Solar Wind Hits the Wall )". (BRIC ). 20 March 2000.〕 bouncing around the transition area several times, gaining energy via collisions with atoms of the interstellar medium. The first evidence of the Fermi glow, and hence the bow shock, was obtained with the help from Voyager 1〔〔 and the Hubble Space Telescope.〔〔
In 2012, data collected from the Interstellar Boundary Explorer satellite and Voyager 1 and 2 indicated that the Sun isn't moving fast enough through its current interstellar environment to have a bow shock.
==See also==

* Heliosphere
*
* Heliopause
* Termination shock
* Bow shock

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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