Editing Čerenkov radiation

From Halopedia, the Halo wiki

You are not logged in. Your IP address will be publicly visible if you make any edits. If you log in or create an account, your edits will be attributed to your username, along with other benefits.

The edit can be undone. Please check the comparison below to verify that this is what you want to do, and then publish the changes below to finish undoing the edit.

Latest revision Your text
Line 1: Line 1:
{{Status|Canon}}
{{Era|H3|GOO}}
{{Wikipedia|Cherenkov radiation}}
{{Ratings}}
'''Čerenkov''' radiation (also spelled Cerenkov or Cherenkov) is electromagnetic radiation emitted when a charged particle (such as a proton) passes through an insulator at a speed greater than the speed of light in that medium. The characteristic "blue glow" of nuclear reactors is due to Čerenkov radiation. It is named after Russian scientist Pavel Alekseyevich Čherenkov, the 1958 Nobel Prize winner who was the first to characterize it rigorously.<ref>[[Wikipedia:Čerenkov radiation|Čerenkov radiation at Wikipedia]]</ref>


'''Čerenkov radiation''' (also spelled '''Cerenkov''' or '''Cherenkov''') is electromagnetic radiation emitted when a charged particle (such as a proton) passes through an insulator at a speed greater than the speed of light in that medium. The characteristic "blue glow" of nuclear reactors is due to Čerenkov radiation. It is named after Russian scientist [[wikipedia:Pavel Alekseyevich Čherenkov|Pavel Alekseyevich Čherenkov]], the 1958 Nobel Prize winner who was the first to characterize it rigorously.<ref>[[Wikipedia:Čerenkov radiation|Čerenkov radiation at Wikipedia]]</ref> Čerenkov radiation only occurs in a medium such as air or water because the speed of light in the medium is slowed. Contrary to popular belief, this phenomena could occur in space, due to there being an extremely low density of particles, along with the container of the fissile material itself.  
During transitions from Slipspace to normal space, or vice versa, the glow of Cherenkov radiation emitted by a ships fissile materials, such as [[plutonium]], can give its presence away to enemy forces.<ref>''[[Halo: Ghosts of Onyx]]''</ref> It also seems that components of the [[MJOLNIR armor]] produce Cherenkov radiation, as the [[Mark VI MJOLNIR Powered Assault Armor/R variant]]'s design specifically reduced the amount of radiation emitted for stealth purposes<ref>''[[Halo 3]]''</ref>.


When a starship transitions from [[Slipstream space|slipspace]] to normal space, or vice versa, the glow of Čerenkov radiation emitted by fissile materials, such as [[plutonium]], can give its presence away to enemy forces even if the ship possesses stealth systems. As a result, if complete stealth is required, [[UNSC prowler|prowlers]] are forced to jettison any on-board [[nuclear weapon]]s before transitioning back to normal space to avoid detection.<ref>'''Halo: Ghosts of Onyx''', ''page 187''</ref> In addition, nukes launched from slipspace can easily be detected by enemy sensors, despite the use of [[Stealth ablative coating|stealth coatings]] or [[lead]] linings.<ref>'''Halo: Ghosts of Onyx''', ''page 15''</ref>
==Possible Contradictions==
 
Cherenkov radiation only occurs in a medium such as air or water because the speed of light in the medium is slowed. Contrary to popular belief, this phenomena could occur in space as mentioned in the book Halo: Ghosts Of Onyx, due to thier being a extremely low density of particles, along with the container of the fissile material itself.  
Components of the [[MJOLNIR Powered Assault Armor|MJOLNIR armor]], likely its [[Fusion reactor|microfusion plant]], produce Čerenkov radiation. The design of the [[MJOLNIR Powered Assault Armor/Mark VI/R variant|Recon]] and [[MJOLNIR Powered Assault Armor/Mark VI/S variant|Scout]] variants specifically reduces the amount of radiation emitted for stealth purposes.<ref>'''[[Halo: The Essential Visual Guide]]''', ''pages 152, 165''</ref>


==Sources==
==Sources==
{{Ref/Sources}}
<references/>
 
[[Category:Technology]]
[[Category:Physics]]
[[Category:Physics]]

Please note that all contributions to Halopedia are considered to be released under the Attribution-ShareAlike 3.0 Unported license (see Halopedia:Copyrights for details). If you don't want your writing to be edited mercilessly and redistributed at will, then don't submit it here. You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource. Do not submit copyrighted work without permission!

Cancel Editing help (opens in new window)

To view or search uploaded images go to the list of images. Uploads and deletions are also logged in the upload log. For help including images on a page see Help:Images. For a sound file, use this code: [[Media:File.ogg]].

Do not copy text from other websites without permission. It will be deleted.