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A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
From: Brad Morris
Date: 2010 Feb 18, 14:21 -0500
Hi Bill
At Lunch, I took the following 10 readings, first off, then on, then off, etc. Vernier Type Sextant, 10x Scope; Upper and Lower limbs of the Sun brought into contact. Apparent SD for today,
18Feb2010, is 32 minutes 21.8 seconds (source:
http://sob.nao-rozhen.org/content/apparent-solar-diameter-and-basic-heliographic-data-2010 )
Reading |
Off |
Decimal⁰ |
Reading |
On |
Decimal⁰ |
||||
1 |
32 |
20 |
-0.53889 |
2 |
32 |
40 |
0.54444 |
||
3 |
33 |
10 |
-0.55278 |
4 |
32 |
20 |
0.53889 |
||
5 |
33 |
0 |
-0.55000 |
6 |
33 |
10 |
0.55278 |
||
7 |
32 |
30 |
-0.54167 |
8 |
32 |
40 |
0.54444 |
||
9 |
32 |
20 |
-0.53889 |
10 |
32 |
40 |
0.54444 |
||
From these 10 readings we can readily create 9 index error measurements. That is, we can group 1+2, 3+4, 5+6, 7+8 and 9+10. Additionally, we can easily see our way to group 2+3, 4+5, 6+7 and
8+9, as any of these pairs would be a natural pairing in that the on/off arc reading follows each other.
Here are the 9 index error measurements
Group |
Decimal⁰ |
degrees |
minutes |
seconds |
on/off |
||
1+2 |
0.00556 |
0 |
0 |
20 |
on |
||
3+4 |
-0.01389 |
0 |
0 |
50 |
off |
||
5+6 |
0.00278 |
0 |
0 |
10 |
on |
||
7+8 |
0.00278 |
0 |
0 |
10 |
on |
||
9+10 |
0.00556 |
0 |
0 |
20 |
on |
||
2+3 |
-0.00833 |
0 |
0 |
30 |
off |
||
4+5 |
-0.01111 |
0 |
0 |
40 |
off |
||
6+7 |
0.01111 |
0 |
0 |
40 |
on |
||
8+9 |
0.00556 |
0 |
0 |
20 |
on |
||
|
The average of these 9 index error measurements is 0 arc seconds, with a standard deviation of 31.6 arc seconds.
Extending the group/pair concept, we can permute every On the Arc against every Off the Arc reading. That is, I can pair 1 with 2,4,6,8 and 10. Next pair 3 with 2,4,6,8 and 10. Etc, yielding
25 IE measurements. In this case the average of all permutations is 2 arc seconds, with a standard deviation of 26.9 arc seconds.
The IE equal to zero outcome is a function of properly setting up the sextant in the first place. The sextant was carefully set to read zero when the index mirror angle is zero. Of course,
I did not get 1/10 minute (6 seconds) every time. That wasn’t possible as the smallest division on my vernier is 10 seconds. Nor did I get 10 seconds every time (although clearly sometimes).
For this reason, I don’t bother to check my IE before and after a round of sights. Firstly, I find this same result every time I make a serious attempt to measure the IE. Secondly, I treat
my sextant with kid gloves (in a gentle fashion for those not familiar with American slang). Essentially, as Frank has noted in his high magnification IE trick, the IE is stable for metal sextants. I have found the same thing and count on it.
No need to warm up the congratulation machine Bill. However, I would claim a very small IE for my sextant, certainly less than 6 seconds!
Best Regards
Brad
Bill, you wrote:
…if they can get the same result within a tenth of a minute each time, I will be among the first to congratulate their instrument.
Kind regards
Bill Morris
Pukenui
New Zealand
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