If you did, you have drawn your first Noon Curve.
Noon Curve drawn freehand from sights
What does this Noon Curve mean? It shows the path of Sun through the sky around Solar Noon on 12 July 2010. Before solar noon, the Sun climbed higher and higher into the sky; after solar noon, it began to sink again.
Solar noon occurred at the instant the Sun crossed my meridian. At that moment, the Sun reached it's highest point in the sky.
If you study the Noon Curve I've drawn, you will see that the top of the curve flattens out. The Sun seems to 'hang' in the sky at the top of the curve, for a minute or so. In fact, two of my sights had the same value: 71° 2.6'.
In fact, this flatness reveals a limitation of the sextant. The Sun actually continued to climb until exactly solar noon, but the changes in height were too small to be measured by an ordinary sextant.
The fact of this 'hanging Sun' has two consequences:
First, it's relatively easy to deduce the height of the Sun at solar noon. This makes it possible to determine your latitude with a fair degree of accuracy.
Second, it's more difficult to determine the exact moment of solar noon. When exactly did the Sun reach it's peak? It's impossible to tell just by looking at the top part of the curve. If we guess the wrong time, our position could be off by miles.
We'll tackle the easier part of the job -- latitude -- first, and leave the more difficult longitude till later (I eat the icing off the cake first, too!)
So, the first step is to look at our Noon Curve, and pick off what is called Hs, or Height of the celestial object as observed by the Sextant. (i.e., the 's' in Hs is for 'sextant', not for 'Sun'.)
Pretty obviously, Hs was 71° 2.6'.
You might wonder, at this point, why we drew the curve, at all? Hs was obvious from the raw data. Two reasons:
- we will need the curve for longitude
- sights are not normally so clean and smooth
But for our Hello World! problem, these sights are perfect, and let us see the flat, top part of the curve more clearly than sea-shot sights would have.
So, Hs is the height of the Sun above the horizon, as seen through a sextant. But this number is distorted by 5 errors that must be corrected for. Whole blog posts could be written about each error, but for our Hello World! problem we will just discuss them briefly.
Index Error: we already discussed this error, which is an error in the sextant, itself. I determined before taking my sights that the index error was 1.2' off the arc.
'Off the arc' means that the sextant's actual 0 point (the index) was 1.2' below the '0' marked on the arc. That is, the actual index was off the arc. Get it?
This means that all our measurements were 1.2' too high and we need to subtract 1.2' from Hs to correct for this error.
If the error was on the arc, then the sextant's actual 0 point would be above the '0' marked on the arc. I.e., the actual index was on the arc, and all our measurements were too low. Saying on or off the arc makes it easier to visualize the error, and thus the correction, making it less likely you will apply the wrong correction (which would double the error!) so take a bit of time to understand this wording.
Dip Error: as discussed previously, the only place you can get an accurate view of the horizon is with your eye at the suface of the water. I took my shots from 6' above the water, so the horizon I saw was below the horizon I would have seen, if I was in the water. This made Hs a bit higher than it should have been, so we must subtract a bit, to correct this error. But how much should we subtract? The Nautical Almanac has a handy DIP table that lets you look up this correction.
Correction table from Nautical Almanac
UK Hydrographic Office
If you look about half-way down the right hand colum, you will find the correction for 6 ft: -2.4'
So, as it says on the bottom of the correction page, Apparent altitude is the Sextant altitude (Hs) corrected for both index error and dip.
|Index Error Correction:||-1.2'|
|Apparent Altitude:||70° 59.0'|
And 'Apparent Altitude' is what we need to find our next correction, but will have to wait until next time, because I am out of time (these posts take a crazy amount of time to write, believe it or not!)
So, how am I doing? Too fast? Too slow? We are starting to get into the math with this post, but I think I've kept it pretty simple and understandable. At least, I hope I have!
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>>> Next Episode: More Corrections
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