Adaptive Optics - Revision history

Lwcamp at 18:57, 7 March 2026

2026-03-07T18:57:39Z

← Older revision		Revision as of 11:57, 7 March 2026
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	[[Category:Lasers]][[Category:Astronomy & Cosmology‏‎]]		[[Category:Lasers]][[Category:Astronomy & Cosmology‏‎]][[Category:Physics & Math & Engineering]]

Lwcamp at 19:06, 26 August 2022

2022-08-26T19:06:56Z

← Older revision		Revision as of 12:06, 26 August 2022
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	[[Category:Lasers]]		[[Category:Lasers]][[Category:Astronomy & Cosmology‏‎]]

Lwcamp at 03:44, 12 October 2021

2021-10-12T03:44:52Z

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	<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>		<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>
	</table>		</table>

			==Credit==
			Author: Luke Campbell

			==References==



	[[Category:Lasers]]		[[Category:Lasers]]

Lwcamp at 22:50, 29 September 2021

2021-09-29T22:50:30Z

← Older revision		Revision as of 15:50, 29 September 2021
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	</table>		</table>

	~~==Credit==~~
	~~Author: Luke Campbell~~

	[[Category:Lasers]]		[[Category:Lasers]]

Lwcamp at 22:49, 29 September 2021

2021-09-29T22:49:47Z

← Older revision		Revision as of 15:49, 29 September 2021
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	<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>		<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>
	</table>		</table>

			==Credit==
			Author: Luke Campbell

	[[Category:Lasers]]		[[Category:Lasers]]

Lwcamp at 19:37, 29 September 2021

2021-09-29T19:37:11Z

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	[[File:Adaptive_optics_correct.png\|thumb\|Adaptive optics correcting distorted light waves.]]		[[File:Adaptive_optics_correct.png\|thumb\|Adaptive optics correcting distorted light waves.]]
	The air is never still. Turbulence in the air makes bubbles of changing density. And different densities of air let light go through them at slightly different speeds. When light goes from a medium where it travels at one speed to one where it travels at a different speed, the light will bend (this phenomenon is called <i>refraction</i>, and it should not be confused with diffraction which, although also causing light to bend, is a completely different phenomenon). Essentially, these turbulence bubbles act like a whole bunch of really weak lenses. So these random and unpredictable turbulence bubbles slightly bend the light in random and unpredictable directions. This is why stars twinkle at night. Your laser beam twinkling will make it hard to aim and keep on tight focus. Fortunately, there is a technological solution. See, those twinkling stars were a nuisance for astronomers. So they invented a way to measure the twinkle and and then bounce the incoming light off a mirror that is controllably warped in just the right way to refocus all the twinkly light into a nice tight spot on the detector.<ref name=van_Dam_2007>https://www2.keck.hawaii.edu/optics/aodocs/KAON489.pdf Performance on Keck II, June 2007 M. van Dam et al., KAON 489</ref> This is called adaptive optics. For lasers, we do this in reverse. The beam is bounced off the same deformable mirror, which de-focuses (or perhaps pre-focuses) the light in such a way that the turbulent air re-focuses it to the tight spot you want.		The air is never still. Turbulence in the air makes bubbles of changing density. And different densities of air let light go through them at slightly different speeds. When light goes from a medium where it travels at one speed to one where it travels at a different speed, the light will bend (this phenomenon is called <i>refraction</i>, and it should not be confused with [[Diffraction\|diffraction]] which, although also causing light to bend, is a completely different phenomenon). Essentially, these turbulence bubbles act like a whole bunch of really weak lenses. So these random and unpredictable turbulence bubbles slightly bend the light in random and unpredictable directions. This is why stars twinkle at night. Your laser beam twinkling will make it hard to aim and keep on tight focus. Fortunately, there is a technological solution. See, those twinkling stars were a nuisance for astronomers. So they invented a way to measure the twinkle and and then bounce the incoming light off a mirror that is controllably warped in just the right way to refocus all the twinkly light into a nice tight spot on the detector.<ref name=van_Dam_2007>https://www2.keck.hawaii.edu/optics/aodocs/KAON489.pdf Performance on Keck II, June 2007 M. van Dam et al., KAON 489</ref> This is called adaptive optics. For lasers, we do this in reverse. The beam is bounced off the same deformable mirror, which de-focuses (or perhaps pre-focuses) the light in such a way that the turbulent air re-focuses it to the tight spot you want.

	<table>		<table>

Lwcamp at 15:09, 29 September 2021

2021-09-29T15:09:32Z

← Older revision		Revision as of 08:09, 29 September 2021
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	<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>		<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>
	</table>		</table>

			[[Category:Lasers]]

Lwcamp: Created page with "Adaptive optics correcting distorted light waves. The air is never still. Turbulence in the air makes bubbles of changing density...."

2021-09-29T03:44:14Z

Created page with "thumb|Adaptive optics correcting distorted light waves. The air is never still. Turbulence in the air makes bubbles of changing density...."

New page

[[File:Adaptive_optics_correct.png|thumb|Adaptive optics correcting distorted light waves.]]
The air is never still. Turbulence in the air makes bubbles of changing density. And different densities of air let light go through them at slightly different speeds. When light goes from a medium where it travels at one speed to one where it travels at a different speed, the light will bend (this phenomenon is called <i>refraction</i>, and it should not be confused with diffraction which, although also causing light to bend, is a completely different phenomenon). Essentially, these turbulence bubbles act like a whole bunch of really weak lenses. So these random and unpredictable turbulence bubbles slightly bend the light in random and unpredictable directions. This is why stars twinkle at night. Your laser beam twinkling will make it hard to aim and keep on tight focus. Fortunately, there is a technological solution. See, those twinkling stars were a nuisance for astronomers. So they invented a way to measure the twinkle and and then bounce the incoming light off a mirror that is controllably warped in just the right way to refocus all the twinkly light into a nice tight spot on the detector.<ref name=van_Dam_2007>https://www2.keck.hawaii.edu/optics/aodocs/KAON489.pdf Performance on Keck II, June 2007 M. van Dam et al., KAON 489</ref> This is called adaptive optics. For lasers, we do this in reverse. The beam is bounced off the same deformable mirror, which de-focuses (or perhaps pre-focuses) the light in such a way that the turbulent air re-focuses it to the tight spot you want.

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[[File:Adaptive_optics_gas_giant.png|512 px]]
<tr><td>The improvement of resolution (corresponding to spot size of a laser when operating in reverse) for imaging astronomical objects with (left) and without (right) adaptive optics.<ref name=Wizinowich_2000>https://iopscience.iop.org/article/10.1086/316543 P. Wizinowich, D. S. Acton, C. Shelton, P. Stomski, J. Gathright, K. Ho, W. Lupton, K. Tsubota, O. Lai, C. Max, J. Brase, J. An, K. Avicola, S. Olivier, D. Gavel, B. Macintosh, A. Ghez, and J. Larkin, “First Light Adaptive Optics Images from the Keck II Telescope: A New Era of High Angular Resolution Imagery”, Publications of the Astronomical Society of the Pacific, Volume 112, Number 769, pp. 315-319 (2000) </ref>
</table>