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#11
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Jon Isaacs wrote:
So how accurately do the holes have to be cut to provide that alignment? Each hole creates two images, each image separated by 90 degrees from the hole, in a manner of speaking. So if the holes in a two-hole mask are separated by 150 degrees instead of 180 degrees, you end up with two pairs of images, each separated by 30 degrees. Since the out-of-focus images are bloated, the alignment has to be off quite a bit before you see four distinct images with a two-hole mask. Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
#13
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If you make a mask with a collection of randomly located holes, you will see
that same pattern reflected in the multiple star images when out of focus. When in focus, you will see a single star image. But note that at high magnification, you will see a distinctly non-circular diffraction pattern around this single star image. Thanks Chris and Brian for explaining this too me. This explanation is something I can grab ahold of, it makes intuitive sense to me. So, what do you guys think about using a 4 hole mask to get rid of the Newtonian diffraction spikes while retaining as much mirror surface and resolution as possible? jon |
#14
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On 10 Jun 2004 01:01:39 GMT, (Jon Isaacs) wrote:
So, what do you guys think about using a 4 hole mask to get rid of the Newtonian diffraction spikes while retaining as much mirror surface and resolution as possible? The obstructed zones around the holes would just be a sort of "super spider", probably creating larger spikes than the spider they are hiding. You'll get sort of fuzzy diffraction spikes, widened because the masked areas have edges that are not orthogonal, and you will have a biased resolution, larger along one pair of axes than along others. In a way, what you are proposing is similar to a curved vane spider, but your's would be like having at least 8 vanes to diffract the incoming light. _________________________________________________ Chris L Peterson Cloudbait Observatory http://www.cloudbait.com |
#15
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In a way, what you are proposing is similar to a curved vane spider, but
your's would be like having at least 8 vanes to diffract the incoming light. Some people have suggested that this scheme provides a significant improvement over the full aperture Newt as well as the signal hole aperture mask. jon |
#16
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In message , Ted Kord
writes Martin Brown wrote in message ... In message , Jeff Polston writes Just found this on Cloudy Nights Telescope Reviews: http://www.cloudynights.com/howtos2/masks.htm Seems like the reviewer had very positive results from a multi-hole off-axis aperture mask. He cannot have been operating diffraction limited then. Looking at it another way multiple holes is like having a large weird shaped central obstruction. But why? Why would it be any different than having 2, 3 or 4 individual mirror sections of equal figure and f/ratio focused on the same spot? It isn't any different at all to that situation. The problem is fundamental and stems from the wave nature of light and diffraction from a finite aperture. The focussed image is related to the Fourier transform of the aperture used. Geometrical optics is inaccurate in this regime. Try looking up Young's slits on the net to get a simple example. I'm just having trouble getting my mind around this. Of course, I'm pretty optically ignorant, so maybe I'm out in left field. I urge you to try it out with a piece of card and two 1cm round holes separated by about 10cm (give or take). That should allow you to clearly see the diffraction patterns of both the small circular aperture and the effect of adding a second one at a moderate separation. Also if you point it at an equal brightness double you will be able to see the variation in the fringe intensity as you rotate the mask. Regards, -- Martin Brown |
#17
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In message , Jon Isaacs
writes If you make a mask with a collection of randomly located holes, you will see that same pattern reflected in the multiple star images when out of focus. So, what do you guys think about using a 4 hole mask to get rid of the Newtonian diffraction spikes while retaining as much mirror surface and resolution as possible? It really won't do what you hope for, but since you can make one so easily from card why not try it out and report back. It is essentially like replacing your nice thin spider supports with huge curved iron girders. It is useful as a focussing aid. You will end up with an image characterised by the resolution of the chosen small circular aperture, modulated by a finer fringe pattern determined by the separation of their centres. For certain well chosen parameters this might give an acceptable image, but it will still be inferior to the original full aperture. Regards, -- Martin Brown |
#18
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#19
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First of all, I appreciate everyone's responses and advice on this.
Although multiple holes might not yield "better results" over a single hole, my main concern was a degradation in the image. The plus side was going to be brighter images or shorter exposure times, but I didn't want that at the expense of image quality. I plan on doing some experimenting on the moon when it comes back around (and I have clear skies). I'll see if I can actually tell a difference in quality of the image with one hole versus three. Jeff http://www.mindspring.com/~jeffpo "Chris L Peterson" wrote in message ... On 10 Jun 2004 00:15:26 GMT, (Jon Isaacs) wrote: So how accurately do the holes have to be cut to provide that alignment? Not at all. You can hack a Hartman mask out of a paper plate with a pen knife. If you make a mask with a collection of randomly located holes, you will see that same pattern reflected in the multiple star images when out of focus. When in focus, you will see a single star image. But note that at high magnification, you will see a distinctly non-circular diffraction pattern around this single star image. There may be special cases where such a mask provides good results (such as looking at double stars of the appropriate spacing and angle), but in general, such an aperture will not yield better results than a simple, unobstructed circle. _________________________________________________ Chris L Peterson Cloudbait Observatory http://www.cloudbait.com |
#20
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![]() Although multiple holes might not yield "better results" over a single hole, my main concern was a degradation in the image. The plus side was going to be brighter images or shorter exposure times, but I didn't want that at the expense of image quality. I plan on doing some experimenting on the moon when it comes back around (and I have clear skies). I'll see if I can actually tell a difference in quality of the image with one hole versus three. It seems to me that the real comparison should first be whether the mask improves or degrades the image. A mask of any sort certainly lengthens the exposure times and reduces the possible resolution, or so it seems. jon |
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