NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: Lunar distance measurement in ideal conditions: attainable accuracy.
From: Alexandre Eremenko
Date: 2013 Jan 18, 18:00 -0500
From: Alexandre Eremenko
Date: 2013 Jan 18, 18:00 -0500
Frank, Thanks. Actually I did not miss this method of index correction. And I understand that most of my Lunars are not bad. (Not worse than Cook's astronomers were doing on land:-) And not worse than other published results that I know. But I still see some scientific problem here: there is a clear systematic bias that I cannot explain. Small, but it definitely exists. I never get undershots. This clearly shows that there is a bias of unknown origin. So there must be some reason for this. If the problem is with index correction, then this is another scientific problem: why over 10 years I get systematically and consistently a wrong index correction with every method that I use ? The only logical explanation I can imagine is that one or two teeth of the sextant arc near 0 are somehow defective, distorted. And the rest of the scale is perfect. The visual inspection shows that they look exactly the same as other teeth, but of course a 0'3 distortion of teeth cannot be visible with a naked eye. Alex. > During the period when you were not following NavList messages, I > described a method for checking index correction which is more reliable > and accurate than any other I have used. It's fairly simple, but it > requires a "spotting scope" --a small telescope with a magnification of > perhaps 30x. The method is simple. Remove the sextant's scope, and place > it on its side on a table where you can see some suitably distant > well-defined vertical pole or tower. Then put the spotting scope on a > tripod in line with the usual optical path to the horizon mirror. You may > need to build a cardboard shade or "umbrella", as Maskelyne put it, to > keep out direct images. Then use the usual method to test the index error, > lining up the direct and reflected images of that distant marker. Your > results should be identical to the tenth of a minute of arc on roughly > four out of five trials (based on my experience). I know of no better way > to check index correction. I don't know if that would explain your 0.3' > bias (which does not appear to be present in your current observations), > but it might help. > > But in any case, your results with lunars are just fine. You're getting > roughly two-thirds of individual observations within a quarter of a minute > of arc (that's another way of saying that the s.d. is about 0.25' on > single observations, which, of course, is what I have been saying for > years). And your average on sets of four is within a tenth of a minute of > arc most of the time. You mentioned a couple of weeks ago that you are > somewhat "pessimistic" about lunars. Doesn't all of this make you even a > little more "optimistic"? > > For others following along, if you shoot four lunars and average them > (with a properly-adjusted modern sextant under good conditions with a 6x > or better scope), as was common practice "back in the day", you can expect > an error in your observed distance of about +/-0.1' most of the time. This > is equivalent to an error in the resulting GMT of +/-12 seconds, which, of > course, is equivalent to an error in the corresponding longitude of +/-3' > at the equator, or at, e.g., 40 degrees latitude, an error of +/-2.3 > nautical miles in position. > > -FER > PS: Also, Alex, that same method setting a spotting scope in line with the > instrument on a table can be used to measure arc error if you add another > sextant with a KNOWN arc error (or better yet zero arc error). > > ---------------------------------------------------------------- > NavList message boards and member settings: www.fer3.com/NavList > Members may optionally receive posts by email. > To cancel email delivery, send a message to NoMail[at]fer3.com > ---------------------------------------------------------------- > > > > > : http://fer3.com/arc/m2.aspx?i=121997 > > >