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| subject: | Re: ATM Wire spiders. |
From: "Tom Krajci" To: Cc: Reply-To: "Tom Krajci" >From: Rik Hill >I did experiments with different "spiders" in the 1970s and reported >on these in the Warren Astronomical Society newsletter. Among the >designs tried were wide spider supports, narrow ones and 8 wire supports. >The latter was the worst. As I eventually learned (and refused to learn >by simply reading) was that the diffraction is caused by EDGES not >by obstruction.... I could have sworn, that Suiter, in this book: http://www.willbell.com/tm/tm5.htm mentions that amount of aperture blocked (area) also plays a role in diffraction patterns. (In other words, a thin wire/vane/whatever and a thick wire/vane/whatever...both have two edges of equal length...but the area of obstruction changes.) If I'm wrong on this citation, please let me know. Also, anecdotally I've heard that wires are better than vanes because they have smaller mass...and as they cool by radiation to the night sky...the smaller mass of a wire support produces a smaller boundary layer that perturbs incoming light less, compared to a vane. >Recently, in the work I do with the Catalina Sky Survey, we ran >an experiment where we were looking for the support that would >provide the LEAST diffraction for a 4-vane spider support for our >camera.... >...the best was a vane (regardless of >the number of vanes) that had small circles along the entire edge.... >...I would be glad to post a before/after image >on my website if you think it would be useful. Yes, please! Tom Krajci Tashkent, Uzbekistan -+- Outgoing mail is certified Virus Free. Checked by AVG anti-virus system (http://www.grisoft.com). Version: 6.0.483 / Virus Database: 279 - Release Date: 5/19/2003 --- BBBS/NT v4.01 Flag-4* Origin: Email Gate (1:379/100) SEEN-BY: 633/267 270 @PATH: 379/100 1 106/1 2000 633/267 |
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