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    Re: Timed Noon sights for position
    From: Joel Jacobs
    Date: 2004 Jan 23, 08:55 -0500

    George,
    
    I will be out much of our morning, but before leaving, I want to compliment
    you on a thorough and well crafted article on Noon Sight Navigation. Nothing
    was left unsaid.
    
    Joel Jacobs
    
    ----- Original Message -----
    From: "George Huxtable" 
    To: 
    Sent: Friday, January 23, 2004 8:34 AM
    Subject: Re: Timed Noon sights for position
    
    
    > Fred Hebard recommended Bob Young to visit my earlier posting on the
    > accuracy of trying to measure longitude from an around-noon Sun
    > observertion.
    >
    > That actually comprised two postings in the thread " Lat. and Lon at LAN"
    > on 8th Jan 2004, the second correcting a big numerical error that Fred had
    > uncovered in the first. Sorry about that.
    >
    > Because of that error, perhaps it's best if I post an amended (and
    somewhat
    > expanded) version of that earlier message. Note that it reflects the
    > discussion that had taken place up to that date, 8th Jan, and not more
    > recent postings, which I have been reading but not analysing closely.
    >
    > TIMED NOON SIGHTS FOR POSITION.
    >
    > There are two problems in determining the longitude..
    >
    > 1. Accuracy in determining the time of maximum altitude.
    >
    > Doug said, in a posting sent on on 7 Jan via Dick Savage-
    > >If the sight taker timed the noon sight within a few secounds of LAN(the
    > >Sun appears to >hang for 20-30 sec at LAN but still moves in that time
    > >frame to greater than 180* or less >than 360*)the sight taker has the
    > >vessel's longitude.
    >
    > But the Sun doesn't simply "hang for 20-30 seconds", it hangs near its
    > unchanging maximum altitude for MUCH longer than that. Take, as an
    example.
    > a winter-solstice Sun observation from my own latitude of 51deg North.
    > Local Apparent Noon (LAN) is at 11h 57m 53sec GMT, when the Sun altitude
    is
    > at 15deg 33.7'. The Sun doesn't drop by 0.5' from that value until it is
    5
    > minutes (in time) away from LAN, before or after.
    >
    > How little a change of altitude can Doug reliably detect before he can
    say,
    > with confidence, that it's past the maximum and has started to descend
    > again? Perhaps, as an experienced observer, he might claim to detect that
    > 0.5' change, but it would require a
    > crystal-sharp horizon to do so, I suspect. Perhaps he can do even better,
    > but it takes about two minutes before or after LAN for the Sun to drop by
    a
    > mere 0.1', and nobody is going to claim to improve on that.
    >
    > So there's no way for an observer to time the noon sight within a few
    > seconds, as Doug claims. If the time of LAN could be determined within 5
    > minutes, then it would establish longitude within about 75 arc-minutes.
    Not
    > a great result. In the unlikely event of a timing precision to 2 minutes,
    a
    > longitude determination to 30 arc-minutes would result.
    >
    > An observer can do much better by timing an altitude sometime before noon,
    > and timing the same altitude after noon, and splitting the difference
    > between those times. This is the age-old method of determining LAN by
    > equal-altitudes. And the more widespread that these two times depart from
    > Noon, the more accurate such a measurement will be. At noon itself is the
    > very worst moment to try to determine when LAN occurs. If the Sun appears
    > only at the moment of noon, and no other, it would be best to rely on
    > whatever DR information exists, rather than fool yourself by presuming you
    > can determine longitude at noon.
    >
    > 2. Time difference between moment of maximum altitude and LAN on a moving
    ship.
    >
    > This second problem affects Doug's big-ships more than it does the small
    > vessels that most of us sail. I don't know the speed of Doug's ships, but
    > let's choose 20 knots as a round number. Let's say that he is steaming
    > South at 20 knots, toward the Sun, from 51deg N, at the exact LAN of 11 h
    > 57m 53s GMT. A stationary observer with a sextant, on a raft that he
    > passes, will indeed see the Sun "hanging" with a constant maximum altitude
    > at that time. On his bridge, however, Doug WON'T see the Sun's altitude as
    > stationary, he will see it as increasing at 20' per hour, because he is
    > steaming toward the Sun at 20 knots, or 20' per hour. To him, the Sun
    won't
    > appear to "hang" in the sky until somewhat later, when it's real altitude
    > (to the man in the raft) is falling by 20' per hour, but on Doug's vessel,
    > just matches the rise that's caused by his own speed.
    >
    > So his LAN will appear to be too late, because what he takes for local
    > apparent noon isn't LAN at all, it's just the moment of maximum altitude.
    >
    > How big will that error be?  Charles H Cotter (in  A History of Nautical
    > Astronomy) deals with the matter on pages 264 to 266, but gets very
    > confused.
    >
    > The moment of maximum altitude will be delayed on LAN by 15.3 (tan lat -
    > tan dec) * v seconds of time, where v is the Southerly component of the
    > speed in knots, and lat and dec are positive if North, negative if South.
    > If lat = +51deg and dec = -23.5deg, this works out at 511 sec, or all of
    > 8.5 minutes late. Unless allowed for, this will give rise to an error (not
    > an uncertainty this time, but an actual error) of 128' in the longitude!
    >
    > Note that the moment of maximum altitude is delayed after LAN, if the
    > vessel has a Southward component of speed, and the Sun is to her South, as
    > in the case referred to above. If sailing toward the Sun when the Sun is
    to
    > her North, the delay is the same way. If the Sun has a direction that's
    aft
    > of her beam, so her course is to some extent away from the Sun, then the
    > maximum altitude is correspondingly before LAN.
    >
    > =================
    > Effect of Sun declination changing.
    >
    > Even in the case of the man in the raft (whose latitude isn't changing),
    he
    > will see a displacement between the times of max. altitude and LAN of the
    > Sun, even though he has no motion toward or away from it, because the Sun
    > can have a North-South motion toward or away from him. Not at a solstice
    > (which is why I chose that example) but at the equinoxes, when the Sun's
    > declination is changing fastest. At the Spring equinox, the Sun is moving
    > toward him at about 1 arc-minute per hour, so that can be thought  of
    quite
    > simply as the Sun having a Northerly speed of 1 knot. Even for the
    > stationary observer on the raft, then, there can be a time-difference
    > between the maximum altitude of the Sun and the true LAN, which unless
    > corrected will give rise to an error in longitude of 6 arc-minutes.
    >
    > This correction, for the time-difference due to changing declination of
    the
    > Sun, is referred to as the Equation of Equal Amplitudes, and can be found
    > under this heading in older editions of Norie or Raper. It was important
    > for accurate determination of longitudes of harbours from on-land
    > observations.
    >
    > It's one of the factors that makes meridian altitudes of the Moon so
    > complicated, because its declination can change over 35 x faster than the
    > Sun's.
    >
    > Except at the solstices, that North-South motion of the Sun needs to be
    > taken into account, even for the observer on a moving vessel, and added to
    > his own speed..
    >
    > ============
    >
    > For slow-moving vessels, determining LATITUDE by a Sun meridian altitude
    > won't be badly affected by measuring max-altitude at the wrong moment in
    > time, away from LAN by (say) a couple of minutes, because altitude hovers
    > so steady for so long. But for faster vessels (20 knots North or South
    > affecting the timing by over 8 minutes) the resulting errors in latitude
    > can become rather significant. Correction methods exist (e.g. Raper, 1864,
    > par. 798-800). Or a mariner can ignore the maximum altitude reading (and
    > its time) and instead measure the altitude at the true moment of LAN,
    > predicted from his chronometer and the equation of time: but to do that
    his
    > longitude needs to be known, at least approximately. Did Doug Royer depend
    > on such a prediction for choosing the appropriate time to measure his Sun
    > altitude, I wonder?
    >
    > But that was just for latitude. Determining LONGITUDE from a noon sight
    is,
    > as we have seen above, fraught with very serious error.
    >
    > There's little hope of using such a technique to make an improvement on a
    > previous DR longitude, unless that DR was very dodgy indeed. So I think
    > it's dangerous to encourage novice navigators to presume that they can
    > deduce a longitude from their LAN, when that just ain't so; not with any
    > accuracy that's worthwhile.
    >
    > George.
    >
    >
    > ================================================================
    > contact George Huxtable by email at george@huxtable.u-net.com, by phone at
    > 01865 820222 (from outside UK, +44 1865 820222), or by mail at 1 Sandy
    > Lane, Southmoor, Abingdon, Oxon OX13 5HX, UK.
    > ================================================================
    
    
    

       
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