Analemma layout and proportions on a sundial

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SUMMARY

The discussion focuses on the layout of an analemmatic sundial, specifically utilizing a true figure 8 analemma for the gnomon position. Key factors include the ordinates of the analemma being determined by the sun's declination and the abscissae being influenced by the equation of time, which can be sourced from Meeus' Astronomical Algorithms. The user seeks clarification on the proportional relationship between the abscissae (E) and the height of the analemma (D), with a conversion from minutes to degrees necessary for accurate plotting. The conversion indicates that 15 minutes of equation of time corresponds to an angular deviation of 3.75 degrees.

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  • Understanding of analemmatic sundials
  • Knowledge of sun's declination and its impact on sundial design
  • Familiarity with the equation of time and its calculation
  • Basic geometry for converting time measurements into angular measurements
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  • Research the mathematical principles behind analemmatic sundials
  • Study the sun's declination and its seasonal variations
  • Learn how to calculate the equation of time using Meeus' Astronomical Algorithms
  • Explore methods for converting time measurements into angular measurements for sundial design
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Amateur astronomers, sundial enthusiasts, and educators in geometry or astronomy who are interested in the precise construction and understanding of analemmatic sundials.

1940LaSalle
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TL;DR
Looking for proportions and similar guidance in laying out an analemma: specifically, the abscissa (equation of time) component. Sun declination is fairly easy to get.
I want to lay out an analemmatic sundial, with a true figure 8 analemma for the gnomon position instead of the more common date marks. Everything I read shows that the ordinates of the points on the curve are a function of the sun's declination on a given date. Further, I'm also given to understand that the abscissae are functions of the equation of time on a given date--and the equation of time is fairly easy to get from a source like Meeus' Astronomical Algorithms. What has me baffled is the proportions of the analemma.

I recall that the height of the analemma is some fraction of the major axis of the ellipse on which the hour points are laid out. Let's call that D, since it comes from the sun's declination. I believe that the equation of time varies from about -15 minutes (sun lags behind clock time) to +15 minutes (sun precedes clock time) over the course of a year. Let's call the range of abscissae that cover that ±15 minutes E, for equation of time. What I haven't found and need is the proportion of E to D--or if not a set proportion, a range of values. And a reference for this information would be extremely valuable.

Thanks very much.
 
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I think your problem is that you have one axis (D) in degrees, and the other axis (E) in minutes. You need to convert E into degrees so you can plot them both in the same units. Since the sun moves 360 degrees in 24*60 = 1440 minutes, E of 15 minutes is an angular deviation E = 15 * 360 / 1440 = 3.75 degrees. Does this help? This link might be useful.
 
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