Day length fluctuations refer to the variations in the duration of daylight experienced over the course of the year due to the tilt of the Earth's axis and its orbit around the Sun. This phenomenon is most noticeable at higher latitudes, where the difference between the longest and shortest days can be significant, particularly during the summer and winter solstices. The key factors contributing to day length fluctuations include: 1. **Tilt of Earth's Axis**: The Earth is tilted at an angle of approximately 23.
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