NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: Lunar Distances with Alex's SNO-T
From: Bill B
Date: 2006 Dec 06, 03:58 -0500
From: Bill B
Date: 2006 Dec 06, 03:58 -0500
In a recent post, I stated: "I also produced a card to sit on the mirror side of the horizon glass to indicate dead center (vertically in normal upright sextant position). This idea popped up while trying to determine index-mirror line of sight to horizon-glass line of sight distance using George's idea. Even when the sextant was tripod mounted, plumb, and zero-mag sight tube was level my measurements ranged from 65mm to 67mm depending on the height of the sextant--which was based on eyeballing the perceived vertical center of the horizon glass in relation to a target line." This has proved very interesting. All this time I have been operating under the assumption that I was using the vertical (physical) center of the horizon glass for observations. Once my card was in place dividing the physical horizon glass equally top and bottom I did a sanity check and moved the index mirror out to its limits, noting its location in relation to the card's dividing line as it moved. To my surprise the optical center of the foreshortened index mirror is about 5.5 mm below the physical center. Using George's method with the physical center the lines of sight increased from 66mm to 73mm. Adjusting the dividing line to the optical center it decreased to 65.5 mm. A couple of hours of playing produced results, some supported by my earlier thoughts, and some observations. 1. By tracing the laser path when the pointer is aligned with the scope barrel, the scope does not look at the physical center of the horizon glass mirror, but rather at a spot below the physical center that coincides with the point located by viewing the foreshortened surface of the index mirror. 2. It does matter whether the laser beam is is centered on the eye-end lens and spot on the horizon glass the scope is looking at. Keeping the entry point centered and using either extreme of the horizon glass/mirror juncture changed the point separation by >5 mm at 40 ft. 3. A zero-mag sight tube can produce sharp spikes if the beam hits the mirror/glass juncture dead nuts on. This is useful at shorter distances (10-30 ft), but its value diminishes at longer distances as the spike enlarges proportional to beam spread spread at larger distances. Working with a focused scope one can keep the spike sharp at greater distances, but vertical and horizontal alignment becomes increasingly demanding. Bill --~--~---------~--~----~------------~-------~--~----~ To post to this group, send email to NavList@fer3.com To , send email to NavList-@fer3.com -~----------~----~----~----~------~----~------~--~---