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Ruud

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Posts posted by Ruud

  1. Hi,

    I've repaired my formula and now I get amazingly exact results. Baader certainly provides the effective field stop diameters, rather than the dimensions of the front lenses.

    Here's a screenshot of the field stop results I get with the new formula, compared with the values Baader gives.

    post-38669-0-59509100-1442468062.png

    See how the field stop of the 4.5 mm is calculated with a precision of 0.01mm?

    Attached you find a short pdf document which explains the two formulas I used: one to calculate pincushion distortion (the Morpheus have 15.1% of it), and another to calculate field stops.

    Both formulas are very easy! Have a go and read the pdf. It will take no more than a minute or two.

    The pdf: FS SGL.pdf

    Meanwhile I'm very happy with the 6.5 mm. I've even decided that I have an eyepiece gap in the 17.5 mm range.

    Bye!

  2. Ruud,

    Can you show your formula for calculation field stops? How do you estimate how much Rectilinear in an eyepice? I mean in term of measurement, not the calculated geometrical distortion.

    For eyepieces I just look at straight lines to estimate rectilinear distortion (RD). Some have a lot for their afov (panoptics, my Nagler 4.8), others seem to have very little (Delos). RD in eyepieces is always of the pincushion type. I've read that correcting for pincushion distortion increases astigmatism which would explain why so many eyepiece designs allow for it.

    Measuring RD is difficult because angular magnification distortion (AMD) can be present as well. With AMD, the magnification (focal length) of the eyepiece varies from the centre to the edge of the field. If AMD is of the barrel type, the image looks like it is pasted on the outside of a sphere, and if the AMD is of the pincushion type the image looks pasted on the inside of a sphere.

    Measuring distortion for camera lenses is easy. To undistort images from camera lenses you can use Adobe Camera Raw (expensive and not always successful) or Hugin panorama stitcher (free and it always works). The settings of the parameters in both programs would give you a reproducible measurement of the distortions present in the original images. There's a guy at ESA who uses Huging for just that purpose.

    My formula to calculate field stops is empirical. I just tried lots of variations with tangents. Here's a screenshot with some comments, and below it is the worksheet itself, if you want to try it:

    post-38669-0-39797500-1441659034_thumb.g

    ScopeCalculator11 .xls  (Please see post number 46 for corrected version of this spreadsheet)

    By the way, I read that the afovs of some of the Delos are smaller than 72°, and that the afovs of the Hyperions are larger than 68°.

    Now, if the avofs of the Morpheus are slightly bigger than the stated 76°, my field stop errors are as I've come to expect them from the worksheet. In my 500 mm fl telescope it takes a star at the equator just 240 seconds to travel across a 8.75 mm field stop. I'll need no more 15 minutes of clear sky and I can do the drift test three times. 

  3. Possibly, the field stops Baader mentions are the diameters of the field lenses, rather than the actual effective field stop diameters. 


    Of the 6.5 mm Morpheus, Baader says the field stop is 8.75 mm, but I calculate 8.62 mm, and my calculated field stops always come out slightly too high. 


    For this Morpheus I get an unexpected 0.13 mm too low. Actually, for all of the Morphs I get results that are too low.


    Because of this I first expected that the Morpheus would have unusually low rectilinear distortion, but the 6.5 mm doesn't. Rectilinear distortion is quite distinct, about what you would expect in an eyepiece as wide as 76°. (Rectilinear distortion, by the way, is not a shortcoming of an eyepiece. It is far more important that angular magnification distortion is absent, and is saw no trace of that.)


    By Wednesday the sky should clear up again. I’ll do a star drift test then, to see what the effective field stop diameter really is.

    • Like 1
  4. I got rid of my Explore Scientific 100 degree EPs, I like the Televues better in my Dobs. I tend to use the 10mm Ethos and Paracorr II most of the time. The cases were made by Ron Burrows at Wood Wonders in the US http://www.wood-wonders.com/

    Beautiful cases, Barry, and a wonderful collection of glass. I enjoyed looking around at Wood Wonders' website. 

    This is my final collection, my wife's words........ :rolleyes:

    Hi Trazor, you have some great eyepieces in your collection and you're obviously more dexterous than most of us with pluck foam. Neat job!

  5. Vixen says 65° on their website. That's what GotGazer 's says on the barrel, but Michael's says 72°.

    You'd think that Vixen reduced the afov without changing the name of the eyepiece. That's confusing!!

    Pincushion plays a role in how big the true fov is. The 10 mm 90° Takahashi UW (the king of pincushion distortion) has a bout the same true field as the 10 mm 82° Celestron Luminous.

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