Equation of time
 

The equation of time (EOT) is a formula used in the process of converting between solar time and clock time to compensate for the earth's elliptical orbit around the sun and its axial tilt. Essentially, the earth does not move perfectly smoothly in a perfectly circular orbit, so the EOT adjusts for that. Graphically, it appears as:

For example, the EOT adjustment in mid-February is about -14 minutes. So when converting clock time to local solar time, you'd subtract 14 minutes. When converting from local solar time to clock time, you'd add 14 minutes.

The EOT can be approximated by the following formula:

E = 9.87 * sin (2B) - 7.53 * cos (B) - 1.5 * sin (B)

Where:

B = 360 * (N - 81) / 365

Where:

N = day number, January 1 = day 1

Note: The SunAngle program currently uses a more sophisticated algorithm for EOT calculations, but the above formula is a decent approximation. Please view the source code of the main SunAngle page if you'd like to review the algorithm actually being used.

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