Hi Peter,

I think your calculations may be correct but the scale of the graph isn't.
The x axis as in your attached picture has another scale then the y axis.

Best wishes, Fer.


Fer J. de Vries

De Zonnewijzerkring
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http://www.de-zonnewijzerkring.nl

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Eindhoven, Netherlands
lat.  51:30 N      long.  5:30 E

----- Original Message ----- 
From: "Peter Mayer" <[EMAIL PROTECTED]>
To: "Sundial List" <[email protected]>
Sent: Thursday, June 10, 2004 2:05 AM
Subject: Locus ofintersections in bifilar dial


> Hi,
>
>  I've been quietly gnawing on two sundial puzzles for a while now.  And
> rather than suffer silently, a prisoner of my own inadequacies, I
> decided to 'throw myself on the mercy of the court' so to speak.
>
> Puzzle the first.  (I'll leave the second puzzle for another day when I
> have the time to set it out with a bit of clarity...)
>
>
>
> I've been wondering, idly, for about a year, after having made a mock-up
> bifilar dial, what the locus of the intersection of the N-S and E-W
> threads is, during the day, and over the course of the year.
>
> More recently, partly inspired by the fantastic graphics on Fabio
> Savian's webpage (www.nonvedolora.it/bifilare.htm) (I finally figured
> out what a wonderful pun "non vedo lora" is; or I _think_ I have).  So.
> I got out my trigonometry books and tried to figure out what the
> equations for x and y would be.  I couldn't get Fabio's equations 2 and
> 3 for x and y to work for me.
>
> So I went back to the diagram in Fred Sawyer's article "Bifilar
> Gnomonics" _Journal of the British Astronomical Association_, Jun 1978,
> 88(4):334-351. and _Bulletin of the British Sundial Society_, Feb 1993,
> 93(1):36-44, also Feb 1995, 95(1):18-27. (Thanks, once again, Fred for
> sending me a copy).  After some stumbling around I derived equations for
> x and y.  And was both pleased, and mortified, to discover that Fred had
> presented the same equations later on in his article:
>
>
>
> x  =  g1 sin t/(sin theta tan delta + cos theta cos t)
>                   (10)
>
>
>
> y  =  g2(sin theta cos t - cos theta tan delta)/(sin theta tan delta
> +cos theta cos t)            (11)
>
>
>
> where: theta = latitude; t = solar hour angle; delta = solar
> declination; g1 is height of the thread along the y-axis (= 1/cos theta
> for a conventional bifilar dial); g2 is the height of the thread along
> the x-axis (= tan theta in the usual case).
>
>
>
> I then put the equations in a spreadsheet and calculated the x and y
> coordinates for a number of hour angles during the day.  And repeated
> the exercise for different solar declinations.  I put the resulting
> coordinates into a statistics software package and plotted the results.
> (see the attached .gif which is c. 7 kb in size). (I hope the cryptic
> legend is sufficiently clear for the purposes of my question)
>
> At first, I was quite pleased because the resulting family of curves was
> roughly what I anticipated, from my conceptualisation of the bifilar
> dial as a sort of dial cast by a vertical gnomon.  But then arose my
> puzzlement.  Although the lines though the hour marks converge to a
> point (as they should)...the angles _between_ hours are not equal.
> Hence my puzzlement.  Needless to add, I would be most grateful for an
> indication of what am I doing wrong!
>
> warmest wishes,
>
> Peter
>
> -- 
> Peter Mayer
> Politics Department
> Adelaide University, AUSTRALIA 5005
> Ph    : +61 8 8303 5606
> Fax   : +61 8 8303 3446
> e-mail: [EMAIL PROTECTED]
>
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