File:Cherenkov radiation-animation.gif

From Infogalactic: the planetary knowledge core
Jump to: navigation, search
Cherenkov_radiation-animation.gif(467 × 260 pixels, file size: 2.65 MB, MIME type: image/gif, looped, 190 frames)
Note: Due to technical limitations, thumbnails of high resolution GIF images such as this one will not be animated.

Summary

Animation of arise Cherenkov's radiation. From the left fly a particle, which polarizes atoms and molecules in surroundings her track. By backward depolarization these atoms and molecules emanate electromagnetic radiation, which from places rise expansive in spherical wave surface. Cover of these wave surface generates conus. In his cut it is possible find rectangular triangle. There is <img src="https://wikimedia.org/api/rest_v1/media/math/render/svg/fa2c392e1cf8d9c8f19142bffbc2ef4b5e720e09" class="mwe-math-fallback-image-inline mw-math-element" aria-hidden="true" style="vertical-align: -1.838ex; width:17.22ex; height:6.176ex;" alt="{\displaystyle \cos {\theta }={\frac {\frac {ct}{n}}{vt}}={\frac {c}{nv}}}">. c . t is displacement, which travel Cherenkov's radiation behind time t, v . t is displacement, which travel a particle.

Licensing

Lua error in package.lua at line 80: module 'strict' not found.

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current10:29, 7 January 2017Thumbnail for version as of 10:29, 7 January 2017467 × 260 (2.65 MB)127.0.0.1 (talk)Animation of arise Cherenkov's radiation. From the left fly a particle, which polarizes atoms and molecules in surroundings her track. By backward depolarization these atoms and molecules emanate electromagnetic radiation, which from places rise expansive in spherical wave surface. Cover of these wave surface generates conus. In his cut it is possible find rectangular triangle. There is <span><span class="mwe-math-mathml-inline mwe-math-mathml-a11y mw-math-element" style="display: none;"><math xmlns="http://www.w3.org/1998/Math/MathML"><semantics><mrow class="MJX-TeXAtom-ORD"><mstyle displaystyle="true" scriptlevel="0"><mi>cos</mi><mo>⁡<!-- ⁡ --></mo><mrow class="MJX-TeXAtom-ORD"><mi>θ<!-- θ --></mi></mrow><mo>=</mo><mrow class="MJX-TeXAtom-ORD"><mfrac><mfrac><mrow><mi>c</mi><mi>t</mi></mrow><mi>n</mi></mfrac><mrow><mi>v</mi><mi>t</mi></mrow></mfrac></mrow><mo>=</mo><mrow class="MJX-TeXAtom-ORD"><mfrac><mi>c</mi><mrow><mi>n</mi><mi>v</mi></mrow></mfrac></mrow></mstyle></mrow><annotation encoding="application/x-tex">{\displaystyle \cos {\theta }={\frac {\frac {ct}{n}}{vt}}={\frac {c}{nv}}}</annotation></semantics></math></span><img src="https://wikimedia.org/api/rest_v1/media/math/render/svg/fa2c392e1cf8d9c8f19142bffbc2ef4b5e720e09" class="mwe-math-fallback-image-inline mw-math-element" aria-hidden="true" style="vertical-align: -1.838ex; width:17.22ex; height:6.176ex;" alt="{\displaystyle \cos {\theta }={\frac {\frac {ct}{n}}{vt}}={\frac {c}{nv}}}"></span>. c . t is displacement, which travel Cherenkov's radiation behind time t, v . t is displacement, which travel a particle.
  • You cannot overwrite this file.

The following page links to this file: