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    Re: Destination from course and distance
    From: Bill B
    Date: 2005 Mar 14, 19:00 -0500

    Jeff
    
    I have played with the provide formula and it appears one can enter the
    course in cardinal coordinates (decimal degrees) directly.  No conversion
    from Cn to C seems to be needed.
    
    It would also appear that S and E must be negative.
    
    I used several scenarios to compare the formula to the trig/Bowditch
    meridional parts method and polar-to-rectangular calculator method.
    
    In mid latitudes they are identical for all practical (light-displacement
    boat) purposes.  The formula vs. meridional parts vs. calculator
    polar-to-rectangular do show differences near the equator over a relatively
    short distance.
    
    Given:
    
    Course 160 true
    Distance 350 nm
    L1 5d 55' North
    l1 80d 36' East
    
    Formula           Bowditch/Trig    Calculator P-R
    L2  00d 26!1 N    L2  00d 26!1 N   L2 00d 26!1 N
    l2  82d 35!9 E    l2  82d 35!1 E   l2 82d 35!9 E
    
    Bill
    
    >> I actually succeeded in using Paul Hirose's suggestion to "rotate" the
    >> triangle, substitute values, and use complements of values (90 - A).
    >> But I failed miserably in trying to simplify the formulae by
    >> substituting the complementary trig functions.  If I knew what I was
    >> doing (or received several more hints) I'd bet there was a much simpler
    >> formula hiding in there somewhere.
    >
    > If understood your initial question, it was:
    >
    > If I start out at a known position, and sail a constant course for a given
    > number of miles (nautical), where will I wind up?  You desire your new
    > location to be given as latitude and longitude.
    >
    > Susan P Howell's book, "Practical Celestial Navigation" gives three methods
    > under the chapter heading, "Mercator Sailing."
    > 1.  Formula
    > 2.  Simpler trig formula and Bowditch meridional-parts table
    > 3.  Totally tabular with Bowditch traverse table
    >
    > You asked for a formula, so I will try my best to relate it via text.
    >
    > L1 = starting latitude
    > L2 = finishing latitude
    > l1 = starting longitude
    > l2 = finishing longitude
    > C = Course
    > D = Distance
    > ln = natural log
    >
    > NOTE:  East and South are negative
    >
    > L2 = [(D cos C)/ 60] + L1
    >
    > l2 = l1 - tan C {180 [ln tan (45 + .5 L2) - ln tan (45 + .5 L1)] / pi}
    >
    > In the reverse of the this formula (given L1, l1, L2 and l2, find course and
    > distance) Howell notes that the you must inspect the direction between the
    > two points to be sure course is measured eastward from north.  C is labeled
    > north or south depending on direction between L1 and L2. C is labeled east
    > or west depending on direction between l1 and l2.
    >
    > Then the C derived is corrected to actual course (Cn) via the following:
    > Cn = NE
    > Cn = 360 - NW
    > Cn = 180 - SE
    > Cn = 180 + SW
    >
    > She does not state if course in the above formulas need to be adjusted from
    > Cn to C.  I will leave that to you to discover.
    >
    >
    > I am bad at converting formulas to ASCII, and worse at typing, so will scan
    > the page and email to you at your request.
    >
    > Since I am already using a calculator to do the above, for a distance of
    > less than 500 nm in my neck of the woods, I use a derivation of mid-latitude
    > sailings and the polar-to-rectangular feature on my TI-30Xa (which is very
    > intuitive).  I can enter the course in cardinal degrees and tenths and
    > obtain my corrections to L1 and l1 in nautical miles.  Latitude corrections
    > can be taken as minutes with no conversion.  The main tricks here are to
    > remember x and y distance answers are swapped as we are not in using trig
    > coordinates (y will become longitude, and x latitude); and longitude
    > distance must be converted from nautical miles to degrees and minutes
    > longitude.  This is basically as simple of adding L1 to L2, dividing that by
    > 2, and taking its cosine.  Invert the cosine (1/X key), then multiply that
    > by the nm distance for minutes longitude (convert to degrees/minutes if
    > necessary) to add or subtract from l1.
    >
    > If interested, I have the above polar-to-rectangular (as well as
    > rectangular-to-polar) written up with illustrations in Microsoft word, and
    > would be glad to send them to you at your request.  It sounds painful at
    > first, but after you do it a few times, it is almost automatic.
    >
    > Hope the above is of some use.
    >
    > Bill
    >
    > billyrem42@earthlink. net
    
    
    

       
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