Analemmatic sundial

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Analemmatic sundial

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Analemmatic sundial at Saint-Etienne, France in which the user's head forms the gnomon of the dial
Analemmatic sundial on a meridian line in the garden of the Herkenrode Abbey in Hasselt (Flanders in Belgium)

Analemmatic sundials are a common feature at science museums , planetariums and occasionally in public places. They exploit the fact that the sun travels in a predictable pattern over the course of a year called the analemma and trace the projection of an object's shadow to measure time, not only the hours, as in normal sundials, but also weeks and months.

Contents

Description

Accurate dials of this type are popular in public places, using a ball at the tip of a flagpole as the nodus, with the sundial face painted on or inlaid in the pavement. A less accurate version of the sundial is to lay out the hour marks on a pavement, and then let the user stand in a square marked with the month. The user's head then forms the gnomon of the dial. In middle latitudes, the ellipse with the hour-marks will be about six meters wide, so the shadow of the head of the beholder falls near it most of the time.[1] The month standing positions are arranged to correct the sundial for the time of year. [2]

Construction

An analemmatic sundial uses a vertical gnomon and its hour lines are the vertical projection of the hour lines of a circular equatorial sundial onto a flat plane.[3] Therefore, the analemmatic sundial is an ellipse, where the short axis is aligned North-South and the long axis is aligned East-West. The noon hour line points true North, whereas the hour lines for 6am and 6pm point due West and East, respectively; the ratio of the short to long axes equals the sine sin(Φ) of the local geographical latitude, denoted Φ. All the hour lines converge to a single centre; the angle θ of a given hour line with the noon hour is given by the formula[4]


\tan \theta = \frac{\tan (15^{\circ} \times t)}{\sin \phi }

where t is the time (in hours) before or after noon. However, the vertical gnomon does not always stand at the centre of the hour lines; rather, to show the correct time, the gnomon must be moved northwards from the centre by the distance[5]


Y = W \cos \phi \tan \delta \,

where W is half the width of the ellipse and δ is the Sun's declination at that time of year. The declination measures how far the sun is above the celestial equator; at the equinoxes, δ=0 whereas it equals roughly ±23.5° at the summer and winter solstices.


See also

References

  1. ^ "Analemmatic sundials: How to build one and why they work" by C.J. Budd and C.J. Sangwin
  2. ^ Sunclocks - Human Sundials, using your own shadow to tell correct time
  3. ^ Rohr (1965), pp. 100–106; Waugh (1973), pp. 108–115; Mayall and Mayall, p. 60–61, 186–190.
  4. ^ Rohr (1965), p. 106; Waugh (1973), p. 113.
  5. ^ Rohr (1965), pp. 103, 111; Waugh (1973), p. 111.

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