NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Re: Your paper in JoN.
From: George Huxtable
Date: 2008 Apr 7, 23:31 +0100
From: George Huxtable
Date: 2008 Apr 7, 23:31 +0100
In Navlist 4812 I posted the following message. I didn't intend to; it was the result of a bit of finger-trouble, as my intention was to send it off-list directly to Andres Ruiz. . However, no harm done. But I didn't explain the topic that Andres was writing about, in his paper in the latest issue of Journal of Navigation, so this message is to fill in that omission. It was "Vector solution for the intersection of two circles of equal amplitude", by Andes Ruiz Gonzalez. And the bit I was referring to was his section 2.3, "Correction for the motion of the observer", which stated- "When the two sights are not taken at the same time, it is necessary to move the first CoP [circle of position] to the time of the second one, or both to a common instant.Many methods have been presented, but the correct way to move a CoP is to advance or retire the GP [Geographical Position of the first observed body] due to the motion of the observer [refs 6,7] Using the technique described in reference [6], the correction is a function of the estimated position of the observer (Be,Le), and his motion: course and speed [C.S]. And since what we are looking for is the true position, an iterative process is required in order to reach the solution for the running fix. The algorithm is described in the Appendix." The appendix gives a block diagram of the decision boxes rather than a description. I have little doubt that Andres understands well how to tackle this question, and get the right answer, as he has explained it to us on Navlist. What I am questioning is his use of the term CoP, or circle of position, to describe the non-circle of the transferred locus of position. Presumably the program calculates the intersection of the second circle with that non-circle, or else with a different circle, which has its centre displaced further, so that it's tangential to the locus in the region that matters. This is what I wrote earlier- ===================== Dear Andres, Pleased to see your paper in Jounal of Navigation. Coming from an earlier generation, I didn't really take in vector mathematics as applied to such problems. So much of your paper went over my head. What I want to ask about are your words in 2.3 about correcting for the motion of an observer. An observer who has measured the altitude of a star to be, say 30 deg, knows that his locus is on a circle radius 60 deg centred at the GP of the star, (say, at dec = 0, GHA = 0, as in the example in paragraph 4 of my paper in JoN, 59, No3, pages 521-524, which I think you have). And then the observer moves a known distance, say 60 miles North. His new locus is a closed figure, somewhat egg-shaped, but NOT a circle any longer. Does your algorithm in A2 find the crossings of that non-circle with another circle centred on another star (say, at dec = 1deg N, GHA = 45 deg W, seen at 45 deg alt, as in that example).? What result does it give? Yours, George. contact George Huxtable at george@huxtable.u-net.com or at +44 1865 820222 (from UK, 01865 820222) or at 1 Sandy Lane, Southmoor, Abingdon, Oxon OX13 5HX, UK. --~--~---------~--~----~------------~-------~--~----~ Navigation List archive: www.fer3.com/arc To post, email NavList@fer3.com To , email NavList-@fer3.com -~----------~----~----~----~------~----~------~--~---