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Index error check Question
From: Rick Emerson
Date: 1998 Dec 12, 13:49 EST
From: Rick Emerson
Date: 1998 Dec 12, 13:49 EST
In my reading, I came across a way to test for index error using the sun's diameter as the point of reference instead of the horizon. The procedure is (as described by Bruce Stark in "Tables for Clearing the Lunar Distance"): 1) Set the sextant to 0D 30.0' (that is, 30' on arc) and adjust the images so the two limbs just touch (as in a regular sight). Record the actual reading. Re-set the micrometer to 0D 30.0' and again re-align the images. Repeat this process a third time. 2) Set the sextant to -0D 30.0' (that is, 30' off arc) and again adjust the micrometer until the limbs in each image just meets. Record the actual reading. Re-set the micrometer to -0D 30.0' and again re-align the images. Repeat this process a third time. 3) Sum up the three on arc readings (no need to convert from arc minutes to degrees) and then total the off arc readings. Subtract the off arc total from the on arc total. Divide the difference by 6. The resulting quotient is the index error. To determine if the error is on or off arc, inspect the two totals (on and off arc). If the on arc error total is greater, the index error is on arc. If the off arc error total is greater, the index error is off arc. An example: on | off ----|---- 32.8|32.6 32.6|32.2 32.8|32.3 ----|---- 98.2|97.1 98.2 - 97.1 = 1.1 1.1 / 6 = 0.2 on arc With a little effort, it becomes apparent that this same technique can be used to remove much of the index error. By adjusting the horizon mirror, the amount of error relative to 30' (this is the angular diameter of the sun) can be equalized, giving an index error of 0' or very close to it. I tried this with two sextants and found the constant or offset varied from one sextant to the other. That is, with an Astra, setting the sextant to +/- 31.5' will cause the desired image to appear in the 3.5x scope. Repeating the process with a Plath sextant the value is +/- 32.0'. The question, then, is where is the extra 1.5' or 2.0' coming from and why does it vary from one instrument to the other? I assume this is a function of either the scopes' magnification (anybody with a 6x scope - or, better still, both a 4x or 3.5x scope and a 6x scope - is invited to report on their experiences) or the sextant's construction (arc radius???). Rick S/V One With The Wind, Baba 35 =-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=--=-= =-= TO UNSUBSCRIBE, send this message to majordomo@XXX.XXX: =-= =-= navigation =-= =-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=--=-=