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I read that in a 90 degrees prism diagonal. Chromatic aberrations
are almost cancelled. I'd like to know to what extend it is true and what is the rule. For the entering light cone, it encounters flat surface via the air-glass interface, and since there is an angle of the incident light, chromatic deviation occurs from the splitting of the white light into the different wavelength inside the glass, But when the light cone exits on the other flat surface of the prism diagonal, the chromatic aberrations are cancelled from the opposite glass-to-air interface and the light cone returns to its original unchromatic aberrated form (this is assuming of course that the objective lens of the telescope is an apo or sct where chromatic aberrations are a nil compared to an achromat). Now what is the rule, like does shorter focal ratio or steeper light cone make the prism diagonal ineffective in cancelling the chromatic aberrations inside the prism diagonal? In long focal ratio scope or light cone entering and exiting a prism diagonal with parallel entry and exit surface (remembering that there is no chromatic aberrations from the internal reflections). How many percentage approximately of the light cone returns to its original unchromatic aberrated form after it exits the prism diagonal. If anyone has any site or articles about this in details. Let me know. Thanks. (Note: Some may say that a prism diagonal is obsolete and just buy a mirror diagonal. Well, the above inquiry is to understand better the behavior of chromatic aberrations in parallel entering and exiting surfaces such as a prism diagonal and novelty item like binoviewer (which has almost zero chromatic aberration when I observe thru one) and also to get some idea like how some products such as the chromacorr (which removes spherical aberrations) work. optidud |
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#3
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![]() optidud wrote: When you say the rays exits the prism at the same angle they enter, this means the red which has least dispersion when it enters the prism exits the same angle as well as the violet with more dispersion. This means that there is no secondary spectrum at the exit side as compared to achromat because the angle are as before they enter the prism. Yet the whole light cone is dispersed slightly... the same effect when you move the focuser a little off the focal plane. So why not just change the position of the focuser to bring the whole dispersed light cone back to focus?? While the light is inside the prism, it is typically converging. This implies that the change in focal position of the red will differ slightly from the change for blue. Simply refocussing will not recover that. Rick S. What's the different between the light cone in a defocused position and when it is deviated laterally? Hope someone can clear this up as this puzzle bugs me day and night for several days already. Thanks. optidud |
#4
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William Hamblen wrote in message . ..
On 13 Jul 2003 07:53:49 -0700, (optidud) wrote: I read that in a 90 degrees prism diagonal. Chromatic aberrations are almost cancelled. I'd like to know to what extend it is true and what is the rule. The rays exit the prism at the same angle they enter, but they are deviated laterally. The difference is pretty small at the focal ratios of most of the telescopes you use star diagonals with. When you say the rays exits the prism at the same angle they enter, this means the red which has least dispersion when it enters the prism exits the same angle as well as the violet with more dispersion. This means that there is no secondary spectrum at the exit side as compared to achromat because the angle are as before they enter the prism. Yet the whole light cone is dispersed slightly... the same effect when you move the focuser a little off the focal plane. So why not just change the position of the focuser to bring the whole dispersed light cone back to focus?? What's the different between the light cone in a defocused position and when it is deviated laterally? Hope someone can clear this up as this puzzle bugs me day and night for several days already. Thanks. optidud |
#5
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If the focal positions for red and blue is slight different inside
the prism as a result of passing thru the entry surface of the prism (and the dispersion that goes with it). Then won't exiting from the second surface bring back the focal positions to the original since it is opposite in effect to air-glass in the 1st entry surface versus glass-air in the 2nd entry surface?? No. Why? Because. Roland Christen |
#6
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In article , optidud wrote:
If the focal positions for red and blue is slight different inside the prism as a result of passing thru the entry surface of the prism (and the dispersion that goes with it). Then won't exiting from the second surface bring back the focal positions to the original since it is opposite in effect to air-glass in the 1st entry surface versus glass-air in the 2nd entry surface?? Optidud, think about Snell's law and why dispersion happens a little bit. Snell's law is sin(a1)*n1 = sin(a2)*n2 when a1 is the angle of the incident ray, a2 is the angle of the refracted ray, n1 is the index of refraction of the first medium and n2 is the index of refraction of the second medium. The angles are measured from the line normal to the surface between the two media. If the first medium is air, n1 is roughly 1 and if the second medium is glass n2 is roughly 1.5. This means than when a ray of light strikes the surface of a thick glass plate at an angle, it is refracted to make a slightly smaller angle in the glass. When it is refracted at the second surface it comes out at a slightly larger angle. Because you have air at both faces of the thick glass plate and the faces are parallel, the rays come out at the same angle they went in. You have that figured out already. The part you've missed is that because of refraction in the glass and the thickness of the plate, the rays are displaced a little to one side, compared to where they would be if the plate wasn't there. Dispersion happens because the index of refraction of glass isn't the same for every wavelength of light - it is slightly more for blue light than it is for red light. Imagine a ray of red light and a ray of blue light coming in at the same angle and hitting the same spot on the first face of the glass plate. The blue ray would be refracted differently from the red ray and the spot where the blue ray exits the second face of the glass plate would be displaced a little from the spot where the red ray exits. This causes some false color to appear around your star image. It isn't much. For slow telescopes where you usually use prism diagonals it is hardly noticeable. |
#7
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![]() "William Hamblen" wrote in message rthlink.net... The blue ray would be refracted differently from the red ray and the spot where the blue ray exits the second face of the glass plate would be displaced a little from the spot where the red ray exits. This causes some false color to appear around your star image. Hey!, even _I_ understood that (I think). :-) Good one Bill (if I can call you Bill). -Stephen Paul |
#8
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![]() optidud wrote: BTW.. The term for the above change of focal points for different wavelengths is called Spherochromatism, right. So prism diagonal and binoviewer introduces Spherochromatism, right? No. It's called color, or chromatic aberration. Spherochromatism is also affected by the prism, though. The effect caused by the same principal. The more steeply inclined the rays are, the larger the impact (in absolute terms). This causes the outer rays to be moved in focus relative to the inner rays. Rick S. optidud |
#9
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In article , optidud wrote:
BTW.. The term for the above change of focal points for different wavelengths is called Spherochromatism, right. So prism diagonal and binoviewer introduces Spherochromatism, right? Different focal points for light of different wavelengths produces chromatic aberration. You have longitudinal (measured along the optical axis) and lateral (measured across the optical axis) aberration. Spherochromatism is change in spherical aberration with wavelength. An ordinary doublet is corrected for spherical aberration at one color. For other colors the spherical aberration would be greater. I have a Celestron/Vixen 102 mm f/9.8 refractor. I can just see some spherical aberration with a deep blue filter. With a yellow or green filter I can't see any spherical aberration. If it was 1500 mm focal length instead of 1000 mm you probably couldn't see SA with the blue filter either. |
#10
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Yes, I've realized the Spherochromatism is not the same as primary
color error and I've consulted many references about this a while ago. But there is something that eludes me and I wonder if I'd figure it out by simply sketching on paper. They say that when spherochromatism is corrected for green light, it is undercorrected in red light and overcorrected in blue light, Which means that in red light, the outer rays focus closer to the lens than the paraxial rays, and the opposite is true in the blue. Well. if the lens is corrected for green light, that means the outer zones of the objective lens are curved to get a perfect spherical aberration correction for green light. Now how is that when red light passes thru the outer zones of the lens, it focuses nearer the lens than in the center rays. I'm still figuring out why this is the case. When manufacturers design lenses. They all use green light, and not white light to grind the lenses to correct for spherical aberrations even in cheap china achromats, right?? This means the optical factories have a lot of green laser or light source at the grinding site, has anyone seen this themselves in optical factories such as Stellarvue's or Televue's (I assume Astrophysics labs are restricted area)? optidud William Hamblen wrote in message arthlink.net... In article , optidud wrote: BTW.. The term for the above change of focal points for different wavelengths is called Spherochromatism, right. So prism diagonal and binoviewer introduces Spherochromatism, right? Different focal points for light of different wavelengths produces chromatic aberration. You have longitudinal (measured along the optical axis) and lateral (measured across the optical axis) aberration. Spherochromatism is change in spherical aberration with wavelength. An ordinary doublet is corrected for spherical aberration at one color. For other colors the spherical aberration would be greater. I have a Celestron/Vixen 102 mm f/9.8 refractor. I can just see some spherical aberration with a deep blue filter. With a yellow or green filter I can't see any spherical aberration. If it was 1500 mm focal length instead of 1000 mm you probably couldn't see SA with the blue filter either. |
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